The status of the AMANDA high-energy neutrino detector (p. 1) |
by Barwick, S W |
The angular dependence of comptonised radiation from a disk (p. 13) |
by Gieseler, U D |
Muon reconstruction with AMANDA-B (p. 13) |
by Wiebusch, C |
Study of neutrinos from stellar collapses with the LVD experiment in the Gran Sasso Laboratory (p. 33) |
by Aglietta, M |
Measurement of elemental composition in the Knee region from the DICE experiment (p. 37) |
by Boothby, K |
Observation of upgoing charged particles in MACRO produced by high energy interactions of muons (p. 37) |
by Ambrosio, M |
Study of the proton-air inelastic cross section at $\sqrt{s}$=1.6-2.4 TeV from EAS-TOP (p. 37) |
by Aglietta, M |
The measurement of the atmospheric muon neutrino flux using MACRO (p. 41) |
by Ambrosio, M |
Study of the primary cosmic ray composition in the knee region with EAS-TOP and MACRO (p. 41) |
by Aglietta, M |
Neutrino astronomy with the MACRO detector (p. 45) |
by Ambrosio, M |
Time dilation in gamma-ray bursts (p. 49) |
by Norris, J P |
Data transmission electronics for Nestor Telescope (p. 53) |
by Capone, A |
Solar neutrino results from super-Kamiokande (p. 69) |
by Conner, Z |
Search for AGN neutrinos with the Soudan 2 detector (p. 81) |
by Demuth, D M |
COMPTEL all-sky imaging at 2,2 MeV (p. 93) |
by McConnell, M |
Three-neutrino Vacuum oscillations and the solar-neutrino problem (p. 113) |
by Portella, H M |
Inelastic cross-sections and their influence on air shower development (p. 121) |
by Knapp, J |
Study of the knee of the cosmic ray spectrum in the electron component (p. 125) |
by Aglietta, M |
The Multi-telescope trigger of the HEGRA IACT system (p. 129) |
by Daum, A |
Cosmic-ray electrons and the diffuse galactic gamma ray emission (p. 141) |
by Porter, T A |
The cosmic ray energy spectrum above 10$^{19}$ eV determined by AGASA (p. 145) |
by Doi, T |
Electron Acceleration In Impulsive Solar Flares : extract of a thesis (p. 145) |
by Lenters, G T |
Magnetic monopole search with the MACRO detector at Gran Sasso (p. 157) |
by Ambrosio, M |
Study of the EAS cores in the knee region (p. 161) |
by Aglietta, M |
Observations of the crab during moonshine (p. 169) |
by Raubenheimer, B C |
A search for TeV gamma-ray emission from the crab Pulsar (p. 185) |
by Gillanders, G |
Indirect search for Wimps with the MACRO detector (p. 185) |
by Ambrosio, M |
Centauro Events (p. 189) |
by Barroso, S L C |
Detecting UHE muons and neutrinos with the Pierre Auger Air Shower array (p. 201) |
by Parente, G |
Energy spectra of electrons and positrons from 5 to 100 GeV (p. 237) |
by Müller, D |
Cosmic ray electron observations from 10 to 100 GeV with BETS detector (p. 241) |
by Torii, S |
The galactic antideuterium production in a diffusion model (p. 249) |
by Chardonnet, P |
Galactic diffusion and the antiproton signal of supersymmetric dark matter (p. 253) |
by Chardonnet, Pascal |
TeV gamma rays from Markarian 421 (p. 261) |
by Kajino, F |
Search for 30-50 TeV $\gamma$-rays from Markarian 421 (p. 269) |
by Aglietta, M |
Computed age of cosmic ray protons in the local zone of the galactic disk and its dependence on the magnetic field (p. 277) |
by Brunetti, M T |
The lateral distribution of EAS electrons (p. 285) |
by Lagutin, A A |
An energy signature for very deep underground muons observed by the LVD experiment (p. 337) |
by Aglietta, M |
Upper limit on the prompt muon flux derived from the LVD data (p. 341) |
by Aglietta, M |
The gamma-ray emission of clusters of galaxies (p. 341) |
by Völk, H J |
Radio controlled light sources for atmospheric monitoring at HiRes (p. 357) |
by Abu-Zayyad, T |
Ion leakage from quasiparallel shocks and the problem of injection (p. 393) |
by Malkov, M |
Galactic propagation of ultra-high energy cosmic ray (p. 485) |
by MedinaTanco, G |
The solar flare event on 15 June 1991 (1-4 (v.1)) |
by Rank, G |
Implications of enhanced perpendicular diffusion in the heliospheric modulation of cosmic rays (1-4 (v.2)) |
by Potgieter, M S |
Highlights from the Rosat soft X-ray mission (1-4 (v.3)) |
by Voges, W |
Cosmic ray proton and helium spectra -results from JACEE (1-4 (v.4)) |
by Cherry, M L |
A Gas-rich detector for cosmic ray studies (1-4 (v.5)) |
by Barbiellini, G |
Study of multifragmentation reactions of Pb ions at 158 A GeV (1-4 (v.6)) |
by Huntrup, G |
Observations of very high energy solar heavy ions from IMP-8 (101-104 (v.1)) |
by Tylka, A J |
Asymmetric cosmic ray transverse gradients at high rigidities (101-104 (v.2)) |
by Ahluwalia, H S |
Multifractal moments analysis of the core of PeV air showers for an estimate of the cosmic ray composition (101-104 (v.4)) |
by Haungs, A |
Threshold effects in emulsion calorimeters (101-104 (v.6)) |
by Haungs, A |
NOE: A scintillating fiber calorimeter to search for long baseline neutrino oscillations (101-104 (v.7)) |
by Barbarino, G C |
The advanced composition explorer mission (105-108 (v.1)) |
by Garrard, T L |
Computation of transverse cosmic ray particle density gradients (105-108 (v.2)) |
by Ahluwalia, H S |
The gamma-ray blazer PKS 0208-512 from MeV to GeV energies (105-108 (v.3)) |
by Stacy, J G |
How to infer the mass composition from EAS observations demonstrated with KASCADE data (105-108 (v.4)) |
by Chilingarian, A A |
The cause of the EAS spectrum break (105-108 (v.6)) |
by Nikolsky, S I |
Optical properties of deep ocean water and south pole ice (105-108 (v.7)) |
by He, Y |
A science center for the advanced composition explorer (109-112 (v.1)) |
by Garrard, T L |
Three activity cycle periodicity in galactic cosmic rays (109-112 (v.2)) |
by Ahluwalia, H S |
The gas deficiency of the galactic halo (109-112 (v.3)) |
by Salati, P |
Primary Mass composition from studying muons in EAS (109-112 (v.4)) |
by Blake, P R |
On the performance of ground based arrays of imaging atmospheric (109-112 (v.5)) |
by Aharonian, F A |
The high energy neutrino-nucleon cross section from recent HERA Parton densities (109-112 (v.7)) |
by Parente, G |
The solar Isotope spectrometer (SIS) (113-116 (v.1)) |
by Cohen, C M |
Modulation of galactic cosmic ray near the heliospheric current sheet (113-116 (v.2)) |
by El-Borie, M A |
The radial gradient of cosmic rays in the galaxy and the existence of a giant halo (113-116 (v.3)) |
by Erlykin, A D |
Primary proton spectrum between I and 50 TeV observed by hadron-detector at 5200m (113-116 (v.4)) |
by Inoue, N |
Status and new results of the HEGRA experiment (113-116 (v.5)) |
by Lindner, A |
Silicon strip detectors with custom VLSI readout electronics for the SIS instrument on ACE (117-120 (v.1)) |
by Wiedenbeck, M E |
Features of GCR 27-day variations in the maximum epoch of solar activity (117-120 (v.2)) |
by Alania, M V |
Diffuse gamma-ray search from the galactic plane using the TIBET AS data (117-120 (v.3)) |
by Kajino, F |
The energy spectrum and chemical composition of primary cosmic rays above 100 TeV derived from size spectrum at Mt. Norikura (117-120 (v.4)) |
by Ito, N |
The steoroscopic system of imaging atmospheric Cherenkov telescopes of the HEGRA-collaboration (117-120 (v.5)) |
by Daum, A |
Correlations p - central rapidity density and cosmic ray collisions at UHE (117-120 (v.6)) |
by Capedevielle, J N |
GeV muons in the atmosphere (117-120 (v.7)) |
by Circella, M |
Spectral variations of the solar protons producing the gamma ray and neutron emissions during the 1990 May 24 solar flare event (121-124 (v.1)) |
by Debrunner, H |
27 - Day cosmic ray variation and its relation to the interplanetary neutral current sheet Tilt (121-124 (v.2)) |
by Valdés-Galicia, J F |
On the nature of the diffuse sub-MeV galactic gamma-ray emission (121-124 (v.3)) |
by Morsberger, U |
Measurement of the allparticle energy spectrum of cosmic rays with the HEGRA detector (121-124 (v.4)) |
by Wiebel-Sooth, B |
The data acquisition of the HEGRA Cherenkov telescope system (121-124 (v.5)) |
by Daum, A |
A new calculation of atmospheric neutrino fluxes at low energies (121-124 (v.7)) |
by Volkova, L V |
Computational study of particle energetization in solar flares (125-128 (v.1)) |
by Pumar, M |
Observed solar diurnal variation of cosmic rays 1965-1994 (125-128 (v.2)) |
by Ahluwalia, H S |
The so-called diffuse extragalactic gamma ray flux (125-128 (v.3)) |
by Erlykin, A D |
Observation of Markarian 501 with the stereoscopic IACT system of the HEGRA collaboration (125-128 (v.5)) |
by Hermann, G |
Regge model and new results for p p and p p reactions (125-128 (v.6)) |
by Rashid, H |
The zenith angle distribution of high energy atmospheric neutrinos: statistical issues (125-128 (v.7)) |
by Longley, N P |
Dual acceleration and/or release of relatuivistic solar cosmic rays (128-132 (v.1)) |
by Shea, M A |
Study of high and low diurnal amplitude wave train events in cosmic rays (129-132 (v.2)) |
by Tiwari, A K |
Hogh energy neutrinos and gamma rays from AGN sporadic central accretion shocks (129-132 (v.3)) |
by Battersby, S |
The first results of TUNKA-13 EAS Cherenkov light experiment (129-132 (v.4)) |
by Gress, O A |
The Monte Carlo simulation for iron emulsion chambers using GEANT code and the bootstrap method (129-132 (v.6)) |
by Fu, Y |
Form factors of three-particle Kaon decay and atmospheric neutrino flavour ratio at high energies (129-132 (v.7)) |
by Misaki, A |
A search for MeV Gamma-ray emission from the Quiet-time Sun (13-16 (v.1)) |
by McConnell, M |
Towards a realistic diffusion tensor for galactic cosmic rays (13-16 (v.2)) |
by Hattingh, M |
A primary composition analysis from muons in EAS (13-16 (v.4)) |
by Alessandro, B |
Charge determination method for RUNJOB experiment (13-16 (v.5)) |
by Apanasenko, A V |
Transverse momenta of helium fragments from gold projectiles in selected classes of nucleus-nucleus collisions (13-16 (v.6)) |
by Wilcznska, B |
Heliospheric enrichment of rare isotopes and of heavy ions in impulsive solar flares (133-136 (v.1)) |
by Roth, I |
Study of diurnal wave trains during solar cycle 22 (133-136 (v.2)) |
by Tiwari, A K |
Particle acceleration and gamma-ray emission in the Orion complex (133-136 (v.3)) |
by Dogiel, V A |
Primary proton with PeV energy detected by RUNJOB experiment (133-136 (v.4)) |
by Apanasenko, A V |
Pulse shape analysis and timing information using the flash-ADC readout of the HEGRA - IACTs (133-136 (v.5)) |
by Hess, M |
Simulations of energy spectra of different primary nuclei at 10 g/cm (133-136 (v.6)) |
by Beresovskaya, V A |
ICESHOW: A Monte Carlo generator of particle showers in ice (133-136 (v.7)) |
by Costa, C G |
The rigidity dependence of solar electron mean free paths in the range 0.3 to 20 MV (137-140 (v.1)) |
by Dröge, W |
Gaussian analysis of the two hemisphere observations of sideral daily variations of galactic cosmic ray (137-140 (v.2)) |
by Hall, D I |
Diffuse gamma ray emission from the galactic plane (137-140 (v.3)) |
by Protheroe, R J |
Proton and Helium spectra obtained by the first RUNJOB-campaign (137-140 (v.4)) |
by Apanasenko, A V |
New 89 pixel camera for BIGRAT telescope (137-140 (v.5)) |
by Dazeley, S A |
Influence of light scattering and finite size of shower particle disk on space-temporal structure of Cherenkov radiation emitted in water by high energy electromagnetic cascade (137-140 (v.7)) |
by Plyasheshnikov, A V |
Cascading alfven wave acceleration in solar flares (141-144 (v.1)) |
by Miller, J A |
Annual variations of cosmic ray intensity and anisotropy (141-144 (v.2)) |
by Gigolashvili, M |
Heavy component spectra obtained by the first RUNJOB-campaign (141-144 (v.4)) |
by Apanasenko, A V |
A new reconstruction method for low energy air cerenkov arrays (141-144 (v.5)) |
by Paré, E |
The status of the extensive air shower experiment KASCADE (141-144 (v.6)) |
by Klages, H O |
The sensibility of the LVD experiment to characterize the parameters of neutrino emission from stellar collapses (141-144 (v.7)) |
by Kemp, E |
Anisotropies at high rigidities: theoretical modeling (145-148 (v.2)) |
by Kota, J |
Nuclear gamma-ray lines and lithium production in pure helium accretion disks (145-148 (v.3)) |
by Guessoum, N |
Initial tests for the Celeste experiment (145-148 (v.5)) |
by Quebert, J |
Hadron distribution in the core of 100 TeV extensive air showers (145-148 (v.6)) |
by Unger, J |
Characteristics of individual LPM showers in water (145-148 (v.7)) |
by Konishi, E |
Particle acceleration by magnetic reconnection in filamentary current sheets (149-152 (v.1)) |
by Kliem, B |
Long-term variations of the cosmic ray anisotropy (149-152 (v.2)) |
by Krymsky, G F |
Positron annihilation in the Orion cloud (149-152 (v.3)) |
by Guessoum, N |
Primary cosmic ray spectrum measured using Cherenkov light reflected from the snow surface (149-152 (v.4)) |
by Antonov, R A |
First results from the Mini-GRAAL project for gamma-ray astronomy above 50 GeV (149-152 (v.5)) |
by Arqueros, F |
Measurements of arrival time distributions of EAS muons with the facilities of the KASCADE central Detector (149-152 (v.6)) |
by Foller, M |
Neutrino detection of halo dark matter (149-152 (v.7)) |
by Bergström, L |
Statistical signatures of the correlation between low-energy (1.6 Mev) protons and X-ray flare (153-156 (v.1)) |
by Rodriguez-Pacheco, J |
Gamma-ray lines and LiBeB production by massive stars of various metallicities (153-156 (v.3)) |
by Cassé, M |
A study on fine features in the energy spectrum of primary cosmic rays over the energy range 1x10 -3x10 eV with the grapes II EAS array at OOTY (153-156 (v.4)) |
by Gupta, S K |
Monte Carlo simulation for the Mini-GRAAL project (153-156 (v.5)) |
by Arqueros, F |
The electron/muon ratio in EAS at and above theKnee region (153-156 (v.6)) |
by Weber, J |
On a search for the extremely high energy particles from the sun by the baksan underground scintillation telescope data (157-160 (v.1)) |
by Karpov, S N |
Radial and latitudinal gradients of cosmic rays in 1974-1977 and 1984-1987 from north-south anisotropy observations (157-160 (v.2)) |
by Belov, A V |
Metal rich wolf-rayet stars and the gamma-ray line emission of the inner galaxy (157-160 (v.3)) |
by Parizot, E |
How to infer the primary energy spectrum from EAS observations demonstrated with KASCADE data (157-160 (v.4)) |
by Roth, M |
The solar tower Atmospheric Cherenkov effects experiment STACEE (157-160 (v.5)) |
by Williams, D A |
Electron and muon size spectra of EAS below and above the Knee (157-160 (v.6)) |
by Glasstetter, R |
Generation and propagation characteristics of relativistic solar proton during the GLE of September 29, 1989 (161-164 (v.1)) |
by Vashenyuk, E V |
Solar tridurnal anisotropy of cosmic rays (161-164 (v.2)) |
by Ahluwalia, H S |
Structure in the EAS size spectrum (161-164 (v.4)) |
by Erlykin, A D |
On-site observations with the STACEE Cherenkov detector Prototype (161-164 (v.5)) |
by Covault, C E |
On possible cosmic ray-origine exotic and rare particles, as monopoles, their properties and their terrestrialo effects (161-164 (v.7)) |
by Szocs, H L |
Relativistic protons near the sun on September 29, 1989 (165-168 (v.1)) |
by Miroshnichenko, L I |
The effect of IMF upon cosmic ray modulation (165-168 (v.2)) |
by Sabbah, I |
The cosmic ray incident directions observed from the northern and southern hemispheres (165-168 (v.4)) |
by Sun, L |
Atmospheric effects on Cerenkov light generated by air showers (165-168 (v.5)) |
by Badran, H M |
Large TeV and GeV muon multiplicities in EAS: separation of P and very heavy primaries at 10 eV (165-168 (v.6)) |
by Antonioli, P |
Experiments of TL-Stack for heavy slowly particles (165-168 (v.7)) |
by Aglietta, M |
Phases of charged particles acceleration during powerful solar gamma - flares detected by the gamma - 1 (169-172 (v.1)) |
by Galper, A M |
Cosmic ray modulations during high speed solar wind streams of different origin (169-172 (v.2)) |
by Sabbah, I |
Arrival directions of cosmic rays with energies 10 eV (169-172 (v.4)) |
by Kolosov, V A |
The image brightness as a new parameter for the TeV background rejection (169-172 (v.5)) |
by Badran, H M |
Multi-core air showers yesterday and tomorrow (169-172 (v.6)) |
by Lidvansky, A S |
Current limits on the cold dark matter flux obtained by the UK collaboration (169-172 (v.7)) |
by Quenby, J J |
Peculiar temporal variations of solar hard X -ray emission (17-20 (v.1)) |
by Yoshimori, M |
A 3D simulation of intensities along Ulyssses' trajectory (17-20 (v.2)) |
by Hattingh, M |
Time-variability of iron lines due to reprocessing of X-rays (17-20 (v.3)) |
by Leahy, D A |
The improved method of the primary nuclear composition determination at energies 10 - 10 eV (17-20 (v.4)) |
by Fomin, Yu A |
Emulsion chamber experiments for the international space station (17-20 (v.5)) |
by Osamu Miyamura, O M |
Total charge changing cross sections of 158 A GeV Pb ions in different targets with nuclear track detectors (17-20 (v.6)) |
by Giacomelli, G |
The ANTARES demonstrator towards a high energy neutrino undersea telescope (17-20 (v.7)) |
by De Botton, |
Maximum entropy spectral analysis of cosmic rays intensity (173-176 (v.2)) |
by Sabbah, I |
Observations of the crab nebula gamma-ray emission above 220 GeV by the CAT Cherenkov imaging telescope (173-176 (v.3)) |
by Goret, P |
The arrival direction of EAS at energies 1 EeV according on tien-shan data (173-176 (v.4)) |
by Nesterova, N M |
Cosmic ray composition around the Knee from simultaneous surface and underground measurements at BAKSAN (173-176 (v.6)) |
by Chudakov, A |
Constraints on coronal transport and acceleration times from charges States of interplanetary ions from gradual solar flare events (173-176(v.1)) |
by Ruffolo, D |
Solar particle acceleration by high energy density MHD turbulence (177-180 (v.1)) |
by Perez-Peraza, J A |
The vtelescope Nina to investigate the nuclear flux in the near earth space (177-180 (v.2)) |
by Vacchi, A |
Arrival direction distribution of extremely high energy cosmic rays recorded by AGASA (177-180 (v.4)) |
by Hayashida, N |
The project for a 1 7 m diameter advanced air cerenkov telescope with a gamma ray energy threshold of 20 GeV (177-180 (v.5)) |
by Lorenz, E C |
A measurement of the EAS differential size spectrum around the Knee (177-180 (v.6)) |
by Chudakov, A |
Search for nuclearities with the MACRO detector at GRAN SASSO (177-180 (v.7)) |
by Popa, V |
Acceleration of coronal mass ejections in the apper corona: observations from Lasco/Soho (181-184 (v.1)) |
by Simnett, G M |
Isotope discrimination with the experiment NINA (181-184 (v.2)) |
by Sparvoli, R |
Search for TeV gamma rays from the crab nebula with the Tibet AS array (181-184 (v.3)) |
by Ohnishi, M |
Observation of the galactic latitude distribution of UHE EAS with the Yakutsk array (181-184 (v.4)) |
by Ivanov, A A |
Monte-Carlo studies for the MAGIC telescope project (181-184 (v.5)) |
by González, J C |
About the nature of delayed pulses in scintillation detectors observed by EAS arrays (181-184 (v.6)) |
by Atrashkevich, V B |
Search for proton decay in SOUDAN 2 (181-184 (v.7)) |
by Goodman, M |
Solar energetic-particle spectra and the structure of coronal mass ejections (185-188 (v.1)) |
by Reames, D V |
Large-area silicon detectors for the advanced composition explorer (ACE) solar isotope spectrometer (SIS) (185-188 (v.2)) |
by Dougherty, B L |
Anisotropies between 10 eV and 10 eV (185-188 (v.4)) |
by Clay, R W |
New approach to the EAS size determination (185-188 (v.6)) |
by Kalmykov, N N |
Influence of coronal mass ejections on the time behavior of energetic electrons in sep-events (189-192 (v.1)) |
by Stolpovskii, V G |
Continuons observation of the cosmic-ray shadow by the sun to study a time variation of the Large-scale structure of the solar and interplanetary magnetic fields (189-192 (v.2)) |
by Amenomori, M |
The neutrons in cosmic ray spectrum for E 10 eV (189-192 (v.4)) |
by Tkaczyk, W |
Time structure of individual EAS (189-192 (v.6)) |
by Ambrosio, M |
The G.L.E. May 24 1990: Kinetic approach to anisotropic Event (193-196 (v.1)) |
by Fedorov, Y |
A correlation between the deviation of the sun's shadow for 10 TeV cosmic rays and the North-south asymmetry of solar activity (193-196 (v.2)) |
by Amenomori, M |
Propagation of ultra high energy cosmic rays in a galactic halo (193-196 (v.4)) |
by Lampard, R |
Measurement of angular distribution of Cherenkov photons in extensive air showers using the DICE detector (193-196 (v.5)) |
by Boothby, K |
Analysis of time structure of EAS front (193-196 (v.6)) |
by Ambrosio, M |
Ramifications of particle physics models for the final stages of black hole evaporation (193-196 (v.7)) |
by Coyne, D |
A search for magnetic helicity effects in the rise times of ground level events (197-200 (v.1)) |
by Kahler, S W |
Neutron monitor sensitivity to solar modulation changes: altitude vs. cutoff rigidity (197-200 (v.2)) |
by Pyle, K R |
Mapping of supernova remnants associated with pulsar B1706-44 and other young pulsars by the Mauritius radio telescope (197-200 (v.3)) |
by Udaya Shankar, N |
A search for nonrandom time series of extensive air showers (197-200 (v.4)) |
by Katayose, T |
Detection Capabilities of a very large array of atmospheric Cherenkov detectors (197-200 (v.5)) |
by Kieda, D B |
Comparison of individual time distributions with the inclusive distribution in EAS front at PeV energies (197-200 (v.6)) |
by Ambrosio, M |
Use of decay electrons from stopping muons as a tool for calibration of cerenkov tanks of the Pierre Auger project (197-200 (v.7)) |
by Villaseñor, L |
Neutron monitor sensitivity to primary proton below 3 GeV derived from data of ground level events (201-204 (v.1)) |
by Belov, A V |
Period of unsual cosmic ray modulation in late 20th cycle : correlative study of cosmic ray variations vs. solar activity(201-204 (v.2)) |
by Usoskin, I G |
On the possible sources of ultra-high energy cosmic rays (201-204 (v.4)) |
by Khristiansen, G B |
First light in the Milagrito detector (201-204 (v.5)) |
by Berley, D |
An analysis of local feature of cosmic ray air showers (201-204 (v.6)) |
by Ohara, S |
Intensity of protons with energy E above 500 GeV during GLES (205-208 (v.1)) |
by Karpov, S N |
variations of the burst frequency detected with the ionization chamber in Yakutsk (205-208 (v.2)) |
by Krivoshapkin, P A |
Limitations of the transport of cosmic ray antimatter from distant galaxies (205-208 (v.4)) |
by Tarle, G |
The Pierre AUGER observatory project: an overview (205-208 (v.5)) |
by Boratave, M |
Core structure of EAS at Akeno (205-208 (v.6)) |
by Sakuyama, H |
Proposal for the optical system of the fluorescence detectors of the Auger project (205-208 (v.7)) |
by Cordero, A |
Extended analysis of the flash phase of charged particle propagation (209-212 (v.1)) |
by Earl, J A |
Including marked periodic variations (209-212 (v.2)) |
by Yasue, S I |
Upper limits on 10 TeV gamma-rays from 58 SNR's and a check for piled up enhancement using the Tibet-I data (209-212 (v.3)) |
by Kajino, F |
Measurements of the cosmic ray positron fraction with the HEAT spectrometer (209-212 (v.4)) |
by Musser, J |
Simulated performance of the AUGER observatory water Cherenkov arrays (209-212 (v.5)) |
by Pryke, C L |
The first results from vrga array at Tien-Shan (209-212 (v.6)) |
by Yakolev, V I |
Trigger sensitivity of the FADC instrumented HiRes fly's eye (209-212 (v.7)) |
by Abu-Zayyad, T |
Neutron transport in the solar atmosphere (21-24 (v.1)) |
by Young, CA |
A new model to study cosmic ray modulation in an asymmetric heliosphere (21-24 (v.2)) |
by Haasbroek, L J |
Observations of cosmic Gamma-ray bursts and solar flares hard electromagnetic radiation in the experiment on-board Mir-spectr orbital complex (21-24 (v.3)) |
by Bogomolov, A V |
Cosmic ray composition measured by HiRes in coincidence with FE2 (21-24 (v.4)) |
by Abu-Zayyad, T |
A two scale hard X-and gamma-ray wide field camera (21-24 (v.5)) |
by Caroli, E |
Fission of gold nuclei at 10.6 A GeV in nuclear emulsions (21-24 (v.6)) |
by Popa, V |
The lake Baikal neutrino oroject: status report (21-24 (v.7)) |
by Kuzmichev, L A |
Energy changes of particles moving along field lines (213-216 (v.1)) |
by Kota, J |
Evaluation of the valid fractal dimension of cosmic ray time series - I including the high level background white noise (213-216 (v.2)) |
by Yasue, S I |
A search for gamma-rays above 20 Tev from herX-1 in the data of 1994/1995 of the HEGRA scintillator and AIROBICC arrays (213-216 (v.3)) |
by Prahl, J |
Cosmic-ray positrons : are there primary sources?(213-216 (v.4)) |
by Coutu, S |
Simulated performance of the AUGER observatory hybrid detectors (213-216 (v.5)) |
by Dawson, B R |
The future of the very large EAS arrays will be on the mountains slopes (213-216 (v.6)) |
by Kabanova, N V |
Calibration and stability measurements of a FADC based data acquisition system for the HiRes fly's eye experiment (213-216 (v.7)) |
by Abu-Zayyad, T |
Cosmic Ray pitch angle diffusion coefficients in the hot and disperse plasma (217-220 (v.1)) |
by Schmidt, J M |
Secular trend removal and harmonic analysis of cosmic ray data (217-220 (v.2)) |
by Duldig, M L |
A search for gamma-rays from potential galactic sources for energies above 20 TeV with the HEGRA scintillator and AIROBICC arrays (217-220 (v.3)) |
by Prahl, J |
The antiproton flux near solar minimum measured with the caprice experiment (217-220 (v.4)) |
by Barbiellini, G |
Shower characteristics of the AUGER prototype water Cherenkov detector observed at Akeno giant air shower array (AGASA) (217-220 (v.5)) |
by Sakati, N |
Results of Gauhati university mini array (217-220 (v.6)) |
by Bezboruah, T |
Cerenkov installation to study EAS at energies of 10 - 10 eV (217-220 (v.7)) |
by Afanasiev, B N |
Scattering of cosmic rays at MHD waves with different cross helicity and polarization (221-224 (v.1)) |
by Schmidt, J M |
The influence of pickup ions, anomalous and galactic cosmic rays on the structure of the heliospheric termination shock- a self-constituent approach (221-224 (v.2)) |
by Le Roux, J A |
Search for isotropic gamma-radiation at ultrahigh energies (221-224 (v.3)) |
by Catanese, M A |
Measurement of the positron and electron spectra with the caprice experiment (221-224 (v.4)) |
by Barbiellini, G |
Results from the Fermilab ground array prototype for the AUGER observatory (221-224 (v.5)) |
by Ravignani, D |
Properties of extensive air showers measured by project GRAND (221-224 (v.6)) |
by Gress, J |
A new data acquisition system for the NBU EAS array (221-224 (v.7)) |
by Chakrabarti, C |
Cosmic ray transport in the large-scale Random magnetic field (225-228 (v.1)) |
by Katz, M |
On the relation of the three-dimensional distribution of anomalous cosmic rays and the structure of the global heliosphere (225-228 (v.2)) |
by Fichtner, H |
A search for TeV emission from AE aquarii (225-228 (v.3)) |
by Colombo, E |
A measurement of antiproton spectrum in the energy range 0.18 to 1.4 GeV (225-228 (v.4)) |
by Matsunaga, H |
Development of water Cherenkov detectors at Fermilab for the PIERRE AUGER project (225-228 (v.5)) |
by Mazur, P O |
Measured direction angle differences for extensive air shower muons (225-228 (v.6)) |
by Gress, J |
GRAPES III: A new large EAS experiment at Ooty Y (225-228 (v.7)) |
by Ito, N |
Numerical determination of mean free paths from Ulysses data as a function of helio-latitude and upstream of a reverse shock (229-232 (v.1)) |
by Drolias, B |
The energy spectrum of anomalous cosmic rays (229-232 (v.2)) |
by Jokipii, J R |
Search for TeV gamma-ray emission from supernova remnants (229-232 (v.3)) |
by Hess, M |
Antihelium flux attenuation from the intragalactic space to the solar cavity (229-232 (v.4)) |
by Codino, A |
A new air-Cherenkov detector array at the south pole operating in coincidence with the SPASE-2 scintillator array (229-232 (v.5)) |
by Dickinson, J E |
EAS characteristics by Yakutsk array data and QGS model (229-232 (v.6)) |
by Afanasiev, B N |
A New small air shower array for teaching and research (229-232 (v.7)) |
by Clay, R W |
Cosmic ray modulation in the heliosphere calculated from a self-consistent diffusion tensor (233-236 (v.1)) |
by Pauls, H L |
Species scaling of modulated anomalous cosmic ray spectra (233-236 (v.2)) |
by Steenberg, C D |
Observation of primary electron spectrum and its astrophysical significance (233-236 (v.4)) |
by Nishimura, J |
The performance of SPASE-2 (233-236 (v.5)) |
by Dickinson, J E |
Lateral distribution of charged particles in EAS with E 10 - 5x10 eV (233-236 (v.6)) |
by Glushkov, A V |
Shower arrival direction determination in the Turku air shower experiment (233-236 (v.7)) |
by Elo, A M |
On the mean free path discrepancy of solar cosmic rays (237-240 (v.1)) |
by Schlickeiser, R |
Low energy anomalous cosmic rays and structure of the heliosheath (237-240 (v.2)) |
by Czechowski, A |
Analysis of SPASE-AMANDA coincidence events (237-240 (v.5)) |
by Miller, T C |
LF radiopulses from UHE air Showers (237-240 (v.6)) |
by Baishya, R |
Error sources and evaluation of their contributions in shower arrival direction determination (237-240 (v.7)) |
by Elo, AM |
Adiabatic deceleration of solar energetic particles as deduced from Monte Carlo simulations of the focused transport (241-244 (v.1)) |
by Kocharov, L G |
Modeling the solar wind/interstellar wind interaction (241-244 (v.2)) |
by Pauls, H L |
AGN studies above 1,5 TeV with the HEGRA 5 m2 Cherenkov telescope (241-244 (v.3)) |
by Petry, D |
The shadow of the moon as seen by Milagrito (241-244 (v.5)) |
by Berley, D |
Muons in giant air showers observed by AGASA and its implications (241-244 (v.6)) |
by Hayashida, N |
The observation of EAS at Taro (241-244 (v.7)) |
by Sakuyama, H |
The effect of adiabatic deceleration on angular distributions of solar energetic particles (245-248 (v.1)) |
by Hatzky, R |
The self-consistent stochastic acceleration of pickup ions in the outer heliosphere in the presence of MHD wave-wave interaction and wave damping (245-248 (v.2)) |
by Le Roux, J A |
Observation of TeV gamma rays from markarian 501 with the first HEGRA Cherenkov telescope (245-248 (v.3)) |
by Deckers, T |
On the Energy spectrum and propagation of cosmic ray electrons in the galaxy (245-248 (v.4)) |
by Van der Walt, D J |
The performance of the Tibet high-density air shower array to search for 2 TeV gamma-ray sources (245-248 (v.5)) |
by Amenomori, M |
Recent extensions to the air shower simulation program CORSIKA (245-248 (v.6)) |
by Heck, D |
Observation of time correlations in cosmic air showers (245-248 (v.7)) |
by Wada, T |
Simulations of the transport of energetic charged particles in the vicinity of an oblique shock (249-252 (v.1)) |
by Ruffolo, D |
An investigation on the heliospheric structure by means of titius - bode's law (249-252 (v.2)) |
by Takahashi, H |
Simultaneous observation of air showers and gamma families to obtain the primary proton flux around the Knee energy region in Tibet (249-252 (v.5)) |
by Amenomori, M |
CHESS, a Cherenkov and electromagnetic shower simulator (249-252 (v.6)) |
by Vasilev, V V |
Search for cosmic ray induced coincidences with detectors in the LEP tunnel (249-252 (v.7)) |
by Grupen, C |
Simulation of solar neutron scattering and attenuation in the earth's atmosphere for different initial Zenith angles (25-28 (v.1)) |
by Dorman, L I |
3-D simulations of heliospheric transport: a comparison of models (25-28 (v.2)) |
by Kota, J |
Initial results from the gamma-ray burst monitor aboard the X-ray astronomy satellite BEPPOSAX (25-28 (v.3)) |
by Frontera, F |
Comparison of fly's eye and AGASA Mass composition measurements (25-28 (v.4)) |
by Dawson, B R |
A gamma-ray burst polarimeter study (25-28 (v.5)) |
by Cline, T L |
The status of Felix, an experiment under study for the Cern LHC which will explore H.E. phenomena seen in cosmic rays at 100 PeV (25-28 (v.6)) |
by Eggert, K |
Reconstruction of atmospheric neutrinos with the Baikal neutrino telescope NT- 96 (25-28 (v.7)) |
by Wiebusch, C |
Effect of focusing on interplanetary shock acceleration (253-256 (v.1)) |
by Vainio, R |
Evolution of the energy spectra of anomalous cosmic rays in the outer heliosphere (253-256 (v.2)) |
by Stone, Edward C |
Detection of VHE gamma-rays from Mrk 501 with the CAT imaging telescope (253-256 (v.3)) |
by Punch, M |
Results from the CACTI experiment: Air Cherenkov & particle measurements of PeV air showers at Los Alamos (253-256 (v.5)) |
by Paling, S |
Methods for the energy determination of cosmic ray showers (253-256 (v.6)) |
by Cortina, J |
Particle acceleration by interplanetary shocks (257-260 (v.1)) |
by Berezhko, E G |
intensity gradients of anomalous cosmic ray oxygen throughout the heliosphere (257-260 (v.2)) |
by Cummings, A C |
Pion eye at Apache Point: an innovative EAS array (257-260 (v.5)) |
by Catalano, O |
Mechanisms of formation of time characteristics of Muon fluxes in extensive air showers (257-260 (v.6)) |
by Beisembaev, R U |
EAS-1000 status 1997 (257-260 (v.7)) |
by Ameev, S S |
Role of the shock thickness on the drift acceleration of electrons (261-264 (v.1)) |
by Vandas, M |
Temporal and spatial variations in the spectra of low energy ions in the outer heliosphere (261-264 (v.2)) |
by Hamilton, D C |
Path-length distribution for cosmic rays in galactic diffusion model (261-264 (v.4)) |
by Ptuskin, V S |
World array: A Worldwide network of pion eye observatories for the investigation of the Extreme energy cosmic rays (261-264 (v.5)) |
by Catalano, O |
Power-spectrum analysis and multifractal study of fluctuations of secondary particles in Monte-Carlo simulation of EAS (261-264 (v.6)) |
by Faleiro, E |
The big muon detector of the Yakutsk EAS array (261-264 (v.7)) |
by Afanasiev, B N |
Acceleration of solar energetic particles at the earth's bow shock (265-268 (v.1)) |
by Dwyer, J R |
The acceleration time of ACR: constraints from pioneer 10 data (265-268 (v.2)) |
by Scherer, K |
Recent observations of X-ray selected active galactic nuclei made with the university of Durham Mark 6 telescope (265-268 (v.3)) |
by Chadwick, P M |
Production of antiprotons in the interstellar gas under special consideration of nucleus-nucleus interactions (265-268 (v.4)) |
by Simon, M |
The ARGO full coverage detector (265-268 (v.5)) |
by Bacci, C |
Absorption of high energy hadrons in the atmosphere (265-268 (v.6)) |
by Bialobrzeska, H |
On the calibration accuracy of light sensors in atmospheric Cherenkov fluorescence and neutrino experiment (265-268 (v.7)) |
by Mirzoyan, R |
Burst - like electron acceleration associated with plasma heating in a solar flare on 22 April 1994 (269-272 (v.1)) |
by Yoshimori, M |
Multiply charged anomalous cosmic rays above 15 MeV/nucleon (269-272 (v.2)) |
by Selesnick, R S |
Simulation of the propagation of primary cosmic rays with energies of 500 TeV accelerated at VELA SNR (269-272 (v.4)) |
by Senda, D |
Characteristics of gamma-hadron families in CORSIKA and MCO models (269-272 (v.6)) |
by Bielawska, H |
Development of high sensitive light detectors for underwater neutrino telescopes (269-272 (v.7)) |
by Lubsandorzhiev, B K |
Angular distributions of solar energetic particles and the nature of pitch angle scattering (273-276 (v.1)) |
by Hatzky, R |
Multiply charged anomalous cosmic ray N. O and Ne: observations with IIILT/SAMPEX (273-276 (v.2)) |
by Klecker, B |
Observation of the galactic and extragalactic sources of gamma-quanta of about 1 TeV (273-276 (v.3)) |
by Sinitsyna, V G |
Computed beryllium age in the local zone of the galactic disk and its dependence on the energy (273-276 (v.4)) |
by Brunetti, M T |
Orbiting wide-angle light collectors (OWL): A pair of earth orbiting eyes (273-276 (v.5)) |
by Ormes, J F |
Factorial and fractal structure of gamma-hadron families in CORSIKA and MCO models (273-276 (v.6)) |
by Bielawska, H |
Application of feed-forward networks for separation of photon and hadron induced extended air showers with the HEGRA scintillator and the wide angle Cherenkov light counter arrays (273-276 (v.7)) |
by Patzold, K |
Perpendicular diffusion of heavy ions accelerated in corotating interaction regions (277-280 (v.1)) |
by Dwyer, J R |
The abundance of anomalous cosmic ray carbon in the inner heliosphere (277-280 (v.2)) |
by Oetliker, M |
First results from a search for TeV emission from BL lacs out to z + o.2 (277-280 (v.3)) |
by Catanese, M A |
Statistical parameters of Cherenkov light signals (277-280 (v.5)) |
by Aliaga, Z |
Can the knee in the EAS size spectrum be due to some change of hadron interactions at energy above 10 eV (277-280 (v.6)) |
by Kalmykov, N N |
Energy determination for RUNJOB experiment (1) - Proton and helium component (277-280 (v.7)) |
by Nanjo, H |
Solar flare electrons propagation in converging interplanetary magnetic structures (281-284 (v.1)) |
by Malandraki, O |
Energy spectrum of anomalous cosmic ray helium, oxygen, nitrogen, and neon (281-284 (v.2)) |
by Makela, P |
On the cosmic ray halflife of Mn (281-284 (v.4)) |
by Chan, Y D |
Directional spectrometry method for high energy gamma-ray astronomy (R, 10 GeV) (281-284 (v.5)) |
by Baskov, V A |
Longitudinal development of large air shower (281-284 (v.6)) |
by Gaisser, T K |
Energy determination for RUNJOB experiment (2)- heavy component (281-284 (v.7)) |
by Nanjo, H |
Simultaneous observations of SEP events by the Ulysses and IMP-8 S/C (285-288 (v.1)) |
by Sidiropoulos, N |
The first observation of sulfur in anomalous cosmic ray by the GEOTAIL and the WIND spacecrafts (285-288 (v.2)) |
by Takashima, T |
Results from the milagrisimo air shower detector (285-288 (v.3)) |
by Berley, D |
On the cosmic-ray half Life on Pm (285-288 (v.4)) |
by Chan, Y D |
The role of fluctuations in atmospheric Cherenkov technique (285-288 (v.5)) |
by Bhat, P N |
Recurrence of energetic particle flux anisotropy observed by ERNE on july, 9, 1996 (289-292 (v.1)) |
by Torsti, J J |
Evidence for anomalous cosmic ray S, Si, and FE in the Outer heliosphere and for a non-ACR source of S at 1 AU (289-292 (v.2)) |
by Stone, Edward C |
Search for Enhancements from Nearby AGNs with identified single muons (289-292 (v.3)) |
by Poirier, J |
effect from diffusive reacceleration on propagating cosmic rays (289-292 (v.4)) |
by Simon, M |
Simulation of gamma-rays produced in cosmic-ray interactions and their utilization for chemical composition investigation (289-292 (v.5)) |
by Masarik, J |
New scaling property of the lateral distribution function of the electrons in the electromagnetic air shower (289-292 (v.6)) |
by Lagutin, A A |
Application of pattern recognition to analysis of emulsion spectrometers (289-292 (v.7)) |
by Iyono, A I |
Analytical approximation to solar neutron scattering and attenuation in the Earth's atmosphere (29-32 (v.1)) |
by Dorman, L I |
Some modulation effects of termination shock accelerated galactic and jovian electrons (29-32 (v.2)) |
by Haasbroek, L J |
EGRET observations of GeV emission from gamma-ray bursts (29-32 (v.3)) |
by Dingus, B L |
Multi-component observations of 10 eV EAS with a hybrid fluorescence and surface detector (29-32 (v.4)) |
by Abu-Zayyad, T |
The international gamma ray astrophysics laboratory: INTEGRAL, a future mission for gamma ray astronomy (29-32 (v.5)) |
by Palumbo, G |
Results from the minimax experiment at Fermilab (29-32 (v.6)) |
by Jones, I W |
Implications of proton anisotropy development observed by ERNE instrument during the 9 July 1996 (293-296 (v.1)) |
by Kocharov, L G |
Partially-Ionized ions of cosmic rays in the vicinity of the earth (293-296 (v.2)) |
by Gagarin, Yu F |
Analysis of HEGRA data with respect to 20 TeV Photon emission from AGN (293-296 (v.3)) |
by Magnussen, N |
The cosmic ray diffusion in galactic magnetic fields and the problem of the knee in PCR energy spectrum at energy 3x10 eV (293-296 (v.4)) |
by Kalmykov, N N |
Triggering and data acquisition systems for the AUGER observatory (293-296 (v.5)) |
by Nitz, D F |
Simulation of the fluorescent component in giant EAS (293-296 (v.6)) |
by Capdevielle, J N |
Automated reconstruction of cascade paths in emulsion chambers (293-296 (v.7)) |
by Zager, E L |
Electron spectra and associated type II and type III radio bursts of the july 9, 1996 solar event (297-300 (v.1)) |
by Sierks, H |
A study of the C/O ratio of low-energy Ions (0.5-7 MeV/nuc) at high heliospheric latitude (297-300 (v.2)) |
by Blake, J B |
Search for 10 TeV Gamma-rays from nearby AGNs with the Tibet AS array (297-300 (v.3)) |
by Mizutani,K |
Comparison of computational techniques for low-energy cosmic ray transport (297-300 (v.4)) |
by Duvernois, M A |
Concept of an integrated Trigger system for the Pierre Auger fluorescence detector (297-300 (v.5)) |
by Espenlaub, G |
Cerenkov detection of electromagnetic showers in ice including the LPM effect (297-300 (v.6)) |
by Alvarez-Muñiz, J |
Study of the performance of first supermodules of large area coordinate detector (Décor) (297-300 (v.7)) |
by Aglietta, M |
EPHIN observations of energetic particles during solar minimum (301-304 (v.1)) |
by Müller-Mellin, R |
Numerical studies of the geomagnetic trapping of anomalous cosmic rays (301-304 (v.2)) |
by Blake, J B |
A search for ultralighh energy gamma-ray emission from redshift-selected blazars (301-304 (v.3)) |
by Catanese, M A |
Constraints on the cosmic infrared/visible background radiation using the celeste and cat experiments at thermis (301-304 (v.4)) |
by De Naurois, Mathieu |
The development of triangulation methods of searching for vertex points in emulsion chambers (301-304 (v.5)) |
by Apanasenko, A V |
General solutions of the yang equation with ionization loss and the excess-path-length distribution of fast charged particles (301-304 (v.6)) |
by Nakatsuka, T |
A new project: using the detector of L3+cosmics phase II (301-304 (v.7)) |
by Ding, L K |
Temporal variations of shock accelerated proton/Alpha ratios at E 100 MeV/n in a large solar particle event (305-308 (v.1)) |
by Kahler, S W |
Geomagnetically trapped anomalous cosmic rays at solar minimum (305-308 (v.2)) |
by Selesnick, R S |
Gamma ray modulation in A.G.N. by interaction with X-rays from an accretion disk hot spot (305-308 (v.3)) |
by Bednarek, W |
X-rays from hybrid accretion disks around compact objects (305-308 (v.4)) |
by Wandel, A S |
On board neutral networks for PAMELA cosmic ray space experiment on satellite (305-308 (v.5)) |
by Castellano, M |
Properties of excess - Path - Length distribution of fast charged particles with ionization loss (305-308 (v.6)) |
by Nakatsuka, T |
L3, a new tool for cosmic ray muon research (305-308 (v.7)) |
by Le Coultre, Pierre |
Corotating interaction regions observed by the particle experiment SMS on the WIND -S/C (E = 0.5 -226 keV/e) (309-312 (v.1)) |
by Kirsch, E T |
Observations on geomagnetically trapped oxygen and neon ions measured on LDEF (309-312 (v.2)) |
by Barz, S |
Gamma rays from star- Jet interactions in A.G.N. (309-312 (v.3)) |
by Protheroe, R J |
Elemental fragmentation cross sections of iron in hydrogen and heavier targets (309-312 (v.4)) |
by Flesch, F |
Imaging simulations of the IBIS hard X-ray/soft gamma-ray telescope on board the INTEGRAL observatory (309-312 (v.5)) |
by Goldwurm, A |
Moments and statistical values of excess - path - length distribution of fast charged particles with ionization loss (309-312 (v.6)) |
by Nakatsuka, T |
Radio detection of EHE particles in the moon (309-312 (v.7)) |
by Alvarez-Muñiz, J |
Long - term variations of ion density Ultra low frequency power spectra (313-316 (v.1)) |
by El-Borie, M A |
Cosmos observations of anomalous cosmic ray in 1995-1996 (313-316 (v.2)) |
by Bobrovskaya, V V |
Gamma-rays and neutrinos from relativistic protons accelerated by magnetic reconnection on an A.G.N. accretion disk (313-316 (v.3)) |
by Bednarek, W |
Neutron production at O degrees from Ca H at E lab + 357 and 565 A MeV (313-316 (v.4)) |
by Tuvé, C |
Neutral network identification of cosmic ray antiprotons in the wizard/CAPRICE experiment (313-316 (v.5)) |
by Bellotti, R |
The model study of the muon lateral distribution (313-316 (v.6)) |
by Sleptsova, V R |
Periodic variations of the cosmic-ray diffusion coefficient related to interplanetary and solar phenomena (313-316 (v.7)) |
by Mavromichalaki, H |
Interplanetary Plasma and Magnetic field observations at 1 AU (317-320 (v.1)) |
by El-Borie, M A |
The systematics of isotopic production cross sections and implications for cosmic ray astrophysics (317-320 (v.4)) |
by Guzik, T G |
A hight precision CAMAC standard GPS timing system for high energy astrophysics applications (317-320 (v.5)) |
by Burdett, A M |
A measurement of the ratio at the top of the atmosphere with the CAPRICE experiment (317-320 (v.6)) |
by Barbiellini, G |
Cosmic rays and ion production in the atmosphere (317-320 (v.7)) |
by Ermakov, V I |
Observations of low energy neutral particle fluxes from Jupiter : gas/Ulysses results(321-324 (v.1)) |
by Witte M |
Updated measurements of the isotopic composition of interplanetary and geomagnetically trapped anomalous cosmic rays (321-324 (v.2)) |
by Leske, R A |
Production of gamma-rays in the crab Nebula by protons from decays of neutrons injected by the crab pulsar (321-324 (v.3)) |
by Bednarek, W |
Up-dated partial cross sections of proton-nucleus reactions (321-324 (v.4)) |
by Silberberg, R |
Physics with HiRes stage 0.5 and stage 2 (321-324 (v.5)) |
by Abu-Zayyad, T |
Relative abundances ofb positive and negative muons in the atmosphere (321-324 (v.6)) |
by Tarle, G |
On the angular distribution of cosmic ray intensity in the earth's atmosphere (321-324 (v.7)) |
by Bazilevskaya, G A |
Low energy interplanetary particles at northern solar latitudes (325-328 (v.1)) |
by Lanzerotti, L J |
The source of anomalous He acceleration and the determination of the interplanetary transport coefficient (325-328 (v.2)) |
by Savopoulos, M |
Inverse Compton model for the TeV emission from vela (325-328 (v.3)) |
by Harding, A K |
Progress report on partial cross sections of nucleus - nucleus reactions (325-328 (v.4)) |
by Tsao, C H |
The capabilities of the high resolution fly's eye detector (325-328 (v.5)) |
by Abu-Zayyad, T |
Muon flux measurements with the Altazimuthal telescope with a magnet spectrometer (325-328 (v.6)) |
by Yamamoto, I |
Effects in cosmic ray modulation during 4 Minima of solar activity (325-328 (v.7)) |
by Stozhkov, Yu I |
Extremely Low Fluxes of Energetic charged particles in the high latitude (329-332 (v.1)) |
by Keppler, E |
Rigidity dependence of the interplanetary mean free path (329-332 (v.2)) |
by Cummings, A C |
Gamma-rays and neutrinos resulting from ion acceleration in young pulsars (329-332 (v.3)) |
by Protheroe, R J |
Computational calculation of partial inelastic cross-sections for nuclear reactions (329-332 (v.4)) |
by Rodriguez-Frias, M D |
Status of the high resolution fly's eye detector: operation and installation (329-332 (v.5)) |
by Abu-Zayyad, T |
Cosmic ray muon investigations with big liquid argon spectrometer (329-332 (v.6)) |
by Belikov, S V |
Rigidity dependence of cosmic ray modulation in 1990-1996 inferred from stratospheric observations (329-332 (v.7)) |
by Svirzhevskaya, A |
The event of 24 May 1990 and the Refraction effect exist (33-36 (v.1)) |
by Dorman, L I |
Effects of the tilt of the heliospheric neutral sheet on the cosmic ray intensity variation at neutron monitor energies (33-36 (v.2)) |
by Singh, M |
EGRET fluxes and upper limits for energetic gamma-ray bursts (33-36 (v.3)) |
by Catelli, J R |
Measurements of energy dependence of the depth of shower maximum in the knee region from the DICE experiment (33-36 (v.4)) |
by Boothby, K |
The IBIS telescope on board integral (33-36 (v.5)) |
by Di Cocco, G |
PHOBOS experiment at RHIC collider (33-36 (v.6)) |
by Holynski, R |
The effects of coronal mass ejections on galactic Rays in the high latitude heliosphere: Observations from Ukysse' first Orbit (333-336 (v.1)) |
by Bothmer, V |
Energy spectra of stationary and unstable electron radiation belts (333-336 (v.2)) |
by Galper, A M |
High energy gamma-ray emission from the PSR1259-63/SS2883(Be) binary system (333-336 (v.3)) |
by Naito, T |
Isotopic production cross sections of relativistic Ca in hydrogen (333-336 (v.4)) |
by Guzik, T G |
The HiRes detector: absolute calibration and alignment (333-336 (v.5)) |
by Abu-Zayyad, T |
The electromagnetic calorimeter Willi - A device for studing cosmic ray muons (333-336 (v.6)) |
by Brancus, I M |
Two groups of large solar proton events (333-336 (v.7)) |
by Bazilevskaya, G A |
Effects of the 5 October 1996 CME at 4,4 AU : Ulysses observations(337-340 (v.1)) |
by Marsden, R G |
Properties of energetic electron fluxes near the Brazil anomaly and geomagnetic Equator: the results of the experiment on-board MIR-spectra orbital complex (337-340 (v.2)) |
by Bogomolov, A V |
Spallation of stellar material by ions accelerated in binary pulsars: limits on high-energy ion flux from pulsars (337-340 (v.3)) |
by Luo, Q |
Isotope production in hydrogen by relativistic Ar and Ar nuclei (337-340 (v.4)) |
by Waddington, C J |
A monte Carlo study of reconstruction of monocular events having limited track lengths for the high resolution Fly's eye (337-340 (v.5)) |
by Abu-Zayyad, T |
Depression in cosmic ray variations during the inversions of the polar magnetic field of the sun (337-340 (v.7)) |
by Astafyeva, N M |
Neutron monitors and space weather (341-344 (v.1)) |
by Bieber, J W |
Strong pulsations of energetic electrons precipitating into the atmosphere : active satellite data(341-344 (v.2)) |
by Kudela, K |
Can source abundance be reliably deduced from measured cosmic ray abundances ? (341-344 (v.4)) |
by Waddington, C J |
Stereo reconstruction of EAS with the Hires detector (341-344 (v.5)) |
by Abu-Zayyad, T |
Solar-cycle changes of cosmic ray propagation parameters and heliospheric terminal shock wave (341-344 (v.7)) |
by Dorman, L I |
An untwisted flux tube model for a magnetic cloud (345-348 (v.1)) |
by Cid, C |
A three dimensional model of the electron radiation belt at high energies (345-348 (v.2)) |
by Pugacheva, G I |
Gamma-ray burst spectral signatures in the 1 GeV-1 TeV range (345-348 (v.3)) |
by Baring, M |
Propagation of the heaviest UH-cosmic ray nuclei (345-348 (v.4)) |
by Waddington, C J |
Atmospheric monitoring at the high resolution fly's eye: atmospheric scattering (345-348 (v.5)) |
by Abu-Zayyad, T |
On the expected CR intensity global modulation in the heoliosphere in the last several hundred years (345-348 (v.7)) |
by Dorman, L I |
Bidirectional particle fluxes in magnetic clouds and their environs (349-352 (v.1)) |
by Fischer, S |
High-energy charged particle waves on the low boundary of the radiation belt (349-352 (v.2)) |
by Galper, A M |
Study on the cosmic ray spectrum and chemical composition using the imaging air Cherenkov Technique (349-352 (v.3)) |
by Konopelko, A K |
How cosmics rays get startyed - The injection problem revited (349-352 (v.4)) |
by Shapiro, M M |
Testing the high resolution fly's eye using laserscope (349-352 (v.5)) |
by Abu-Zayyad, T |
Expected time-variations of neutron monitor counting rate caused by CR particle energy change in the oeriods of thunderstorms (349-352 (v.7)) |
by Dorman, L I |
Features of cosmic ray Transient decreases in associatioin with arrival of magnetic clouds (353-356 (v.1)) |
by Tiwari, A K |
The 1-9 Mev/nucleon HE flux dynamics in the inner magnetosphere during 1984-1986 (353-356 (v.2)) |
by Pugacheva, G I |
Results from the trek ultraheavy collector (353-356 (v.3)) |
by Weaver, B A |
Energetics of injection and acceleration of the galactic cosmic rays (353-356 (v.4)) |
by Shapiro, M M |
Cloud detection for fluorescence and Cherenkov detectors (353-356 (v.5)) |
by Bird, D |
Photonuclear interactions of extremely high energy cosmic-rays (353-356 (v.7)) |
by Anchordoqui, L A |
Development and effects of corotating interaction regions: workshop report (357-360 (v.1)) |
by Kunow, H |
The influence of synchrotron energy losses on the inner radiation zone electron deceleration process (357-360 (v.2)) |
by Pugacheva, G I |
Study of elemental and isotopic composition of cosmic ray nuclei Ca, Ti, V, Cr, Mn and Fe (357-360 (v.3)) |
by Lukasiak, A |
GCR composition : volatility or FIP ? SNR shock acceleration of gas and dust(357-360 (v.4)) |
by Meyer, J P |
Software tools in high energy physics (357-360 (v.7)) |
by Swain, J |
Confinement of electrons, accelerated at distant high latitude corotating interaction regions, to the inner heliosphere (361-364 (v.1)) |
by Simnett, G M |
Production of light element isotopes in the inner magnetosphere (361-364 (v.2)) |
by Spjeldvik, W N |
A charge spectrum of ultra heavy cosmic ray nuclei, including actinides detected on the LDEF (361-364 (v.3)) |
by Keane, A J |
Understanding elemental and isotopic abundance anomalies in the galactic cosmic ray (361-364 (v.4)) |
by Duvernois, M A |
Atmospheric monitoring at the high resolution fly's eye: data from the HiRes2 flasher array (361-364 (v.5)) |
by Abu-Zayyad, T |
Computing trends in high energy physics (361-364 (v.7)) |
by Swain, J |
Energetic Particle acceleration at corotating interaction regions: Ulysses results (365-368 (v.1)) |
by Desai, M I |
On the periodic variations of secondary cosmic rays in the Brazilian magnetic anomaly region (BMAR) (365-368 (v.2)) |
by Martin, I M |
The response of particle detectors to gold nuclei at 11 GeV/nucleon (365-368 (v.3)) |
by Wiedenbeck, M E |
Primaty cosmic rays composition around the Knee in the model of particle acceleration by shock front ensembles in galactic superbubbles (365-368 (v.4)) |
by Bykov, A M |
Atmospheric monitoring at the high resolution fly's eye: monitoring data via the HiRes laser/lidar system (365-368 (v.5)) |
by Abu-Zayyad, T |
Gamma ray burst detection by air scintillastion observations from space (GRASS) (365-368 (v.7)) |
by Catalano, O |
Corotating Ion enhancements observed by IMP 8 and sampex at earth, and by ULYSSES at high heliographic Latitudes (369-372 (v.1)) |
by Richardson, I G |
The cosmic ray asymptotic directions for station oulu in the magnetic field of the tsyganenko 1989 model (369-372 (v.2)) |
by Danilova, O A |
A measurement of the proton spectrum at 1 AU near solar minimum with the caprice experiment (369-372 (v.3)) |
by Barbiellini, G |
Short wavelength instabilities in cosmic ray modified shocks (369-372 (v.4)) |
by Webb, G |
Telescope array as an extremely high energy cosmic ray detector (369-372 (v.5)) |
by Sasaki, G J |
Comparison between hexagon and superman configurations for the Auger observatory (369-372 (v.7)) |
by Biral, A R |
A new solar neutron telescope in Hawaii (37-40 (v.1)) |
by Matsubara, Y |
Evolution of cosmic ray electron spectra above 350 MeV along the Ulysses trajectory (37-40 (v.2)) |
by Raviart, A |
MeV measurements of gamma-ray bursts by CGRO-COMPTEL (37-40 (v.3)) |
by Connors, A |
Cosmic Ray induced background in the SPI INTEGRAL spectrometer (37-40 (v.5)) |
by Diallo, N |
The solar activity dependence of relationship between CIR MeV ion enhancement and solar wind speed (373-376 (v.1)) |
by Kobayashi, M |
Secondary and Re-entrant albedo electrons in the atmosphere (373-376 (v.2)) |
by De Nolfo, G A |
Measurement of cosmic-ray H and He isotopes by BESS and its implications for cosmics-ray propagation (373-376 (v.3)) |
by Seo, E S |
The role of solar wind and pick-up ions in the termination shock acceleration process (373-376 (v.4)) |
by Jones, F C |
The telescope array project (373-376 (v.5)) |
by Aiso, S |
Monte Carlo calculation of radio emission from extensive air showers (373-376 (v.7)) |
by Dova, M T |
New spectral and abundance features in low energy CIR Heavy ions (377-380 (v.1)) |
by Mason, G M |
Effects of the magnetosheath magnetic field on cosmic ray propagation near earth (377-380 (v.2)) |
by Butikofer, R |
The He/ He ratio with the CAPRICE apparatus (377-380 (v.3)) |
by Barbiellini, G |
New nonlinear effects in particle acceleration by strong shock waves (377-380 (v.4)) |
by Toptygin, I N |
Proposed fluorescence detectors for the AUGER observatory (377-380 (v.5)) |
by Dawson, B R |
Particle interaction modeling in high energy physics (377-380 (v.7)) |
by Swain, J |
Time and energy dependence of 26-day recurrent decreases of 100MeV protons in the inner southern heliosphere and its correlation to latitudinal gradients: Ulysses COSPIN/KET results (381-384 (v.1)) |
by Kunow, H |
Geomagnetic cutoff variations during solar energetic particle events-implications for the space station (381-384 (v.2)) |
by Leske, R A |
High resolution measurements of the isotopic composition of galactic cosmic ray C, N, O, Ne, Mg and Si from Ulysses HET (381-384 (v.3)) |
by Connell, J |
The role of the cross shock potential in perpendicular shock structure (381-384 (v.4)) |
by Jones, F C |
Space-airwatch for cosmic rays: a new method category (381-384 (v.5)) |
by Linsley, J |
An analysis of the energy spectrum of the highest energy cosmic rays (381-384 (v.7)) |
by Dova, M T |
Distinct shock acceleration processes: ULYSSES observations (385-388 (v.1)) |
by Marhavilas, P |
Apparent geomagnetic cutoffs and the cosmic ray anomaly in the Cape Town region (385-388 (v.2)) |
by Stoker, P H |
Galactic cosmic ray confinement time : Ulysses HET measurements of the secondary radio-nuclide Be(385-388 (v.3)) |
by Connell, J |
Cosmic ray acceleration at ultra-relativistic shock waves (385-388 (v.4)) |
by Bednarz, J |
Space air watch: observation of the earth atmosphere from the ISSA space station (385-388 (v.5)) |
by Linsley, J |
Comparison of experimental and simulation data on absorption lengths for electromagnetic component and gamma-hadron families induced by primary particles at energies 1-100 PeV (385-388 (v.7)) |
by Slavatinsky, S A |
Periodicity of the energetic particle fluxes measured by SOHO/ERNE in 1996 (389-392 (v.1)) |
by Torsti, J J |
Efficient computation of apparent cutoffs (389-392 (v.2)) |
by Bieber, J W |
Voyager measurements of the isotopic composition of Li, Be and B nuclei (389-392 (v.3)) |
by Lukasiak, A |
Microphysics of particle injection into the first order Fermi process in shocks (389-392 (v.4)) |
by Malkov, M |
Possible scenarios for a space airwatch mission devoted to the observation of the atmospheric fluorescence induced by the cosmic radiation (389-392 (v.5)) |
by Attina, P |
Analysis of Halo properties in high-energy gamma-hadron families (389-392 (v.7)) |
by Slavatinsky, S A |
Energetic ions in the outer heliosphere, 1992-1997 (393-396 (v.1)) |
by Krimigis, S M |
Secular changes in the geomagnetic cutoff rigidities and their effect on cosmic ray measurements (393-396 (v.2)) |
by Shea, M A |
Al in the galactic cosmic radiation: measurements, with the Ulysses HET instrument (393-396 (v.3)) |
by Connell, J |
Physics objectives for a superconducting magnetic facility on ISSA (393-396 (v.5)) |
by De Pascale, M P |
Properties of the biggest shower recorded by the kiel array (393-396 (v.7)) |
by Kempa, J |
Two-step forbush decreases in the inner solar system and their relevance for models of transient disturbances (397-400 (v.1)) |
by Wibberenz, G |
Calculated cosmic ray cutoff rigidities at 450 knm for epoch 1990.0 (397-400 (v.2)) |
by Smart, D F |
The galactic cosmic ray CI Clock : ULYSSES HET results(397-400 (v.3)) |
by Connell, J |
Cosmic ray driven dynamical haloes: galactic winds or galactic breezes? (397-400 (v.5)) |
by Fichtner, H |
Analytic evaluation of neutron and proton intensities in the atmosphere (397-400 (v.7)) |
by Liland, A |
The large -scale structures in the interstellar medium (401 (v.5)) |
by Katz, M |
Cosmic ray modulation during the 24 March 1991 forbush decrease (401-404 (v.1)) |
by Hofer, M Y |
World grid of calculated cosmic ray vertical cutoff rigidities for epoch 1990.0 (401-404 (v.2)) |
by Smart, D F |
The galactic cosmic ray all-particle spectrum (401-404 (v.3)) |
by Adams, J H |
Non linear shock acceleration: Bifurcation analysis in the Bohm limit (401-404 (v.4)) |
by Malkov, M |
A new measurement of the energy spectra of light nuclei from 20-150 GeV/n (404-408 (v.3)) |
by Diehl, E |
Characteristics of precursory decrease of forbush decrease inferred from world wide observations of muon and neutron intensities (405-408 (v.1)) |
by Morishita, I |
World grids of cosmic ray vertical cutoff rigidities for epoch 1600, 1700, and 1800 (405-408 (v.2)) |
by Smart, D F |
Re-acceleration of GeV-electrons in weak intergalactic shocks (405-408 (v.4)) |
by Von Rauchhaupt, U |
Measurement of the absolute proton and helium flux at the top of the atmosphere using IMAX (409 (v.3)) |
by Menn, W |
To forecast huge forbush decreases during solar activity cycles (409-412 (v.1)) |
by Storini, M |
Environmental radiation monitoring along the course of the expeditions from Italy to Antarctica and returnt (409-412 (v.2)) |
by Galli, M |
Non-linear shock acceleration and gamma-ray production in supernova remnants (409-412 (v.4)) |
by Baring, M |
Scintillation fiber telescope for detecting neutrons in a satellite experiment (41-44 (v.1)) |
by Muraki, Y |
The cosmic Ray recovery and solar minimum phase of solar cycle 22: an interim report (41-44 (v.2)) |
by McDonald, F B |
Analysis of the space distributions of two classes of classical GRBs (41-44 (v.3)) |
by Belli, B M |
High energy imaging observations with INTEGRAL/IBIS (41-44 (v.5)) |
by Stephen, J B |
Auto-model solution for the nonstationary problem described the cosmic ray preincrease effect and forbush-decrease (413-416 (v.1)) |
by Dorman, L I |
Environmental radiation monitoring at Terra Nova Bay base and Ross Sea in various energy bands (413-416 (v.2)) |
by Galli, M |
Temporal changes of GCR forbush decreases energy spectron (417-420 (v.1)) |
by Alania, M V |
The sea - land transition of the environmental radiation during the expeditions Italy - Antarctica - Italy (417-420 (v.2)) |
by Cecchini, S |
Effects of rock density unhomogeneities in muon flux underground (417-420 (v.6)) |
by Budino |
Forbush-effects 1977-1979 (421-424 (v.1)) |
by Belov, A V |
Latitude survey of the cosmic ray nucleonic component (Italy - Antarctic - Italy, 1996-1997) (421-424 (v.2)) |
by Villoresi, G |
Acceleration of cosmic ray electrons by ion-excited waves at quasi-perpendicular shocks (421-424 (v.4)) |
by McClements, K G |
Zenithal distribution of atmospheric muons (421-424 (v.6)) |
by Portella, H M |
Scale-invariant features of cosmic ray fluctuation dynamics in a solar Cycle (425-428 (v.1)) |
by Kozlov, V I |
Power spectra of neutron monitor time series at frequencies F 1.15x10 Hz (425-428 (v.2)) |
by Kudela, K |
Interstellar dust, shock acceleration and the galactic cosmic ray composition (425-428 (v.4)) |
by Ellison, D C |
Transition curves for Cherenkov radiation induced by high energy muon for KM3 project (425-428 (v.6)) |
by Takahashi, N |
Cumulative effect of high speed solar wind streams on cosmic ray modulation (429-432 (v.1)) |
by Shrivastava, P K |
ELFO : experiment for light flash observation in space(429-432 (v.2)) |
by Bartalucci, S |
Short wavelength wave interactions in two fluid cosmic ray hydrodynamics and gas dynamics (429-432 (v.4)) |
by Webb, G |
Muon pair production by gammas in extensive air showers (429-432 (v.6)) |
by Hudryavtsev, V A |
Muon simulation and the primary cosmic ray composition at 10 5x10 eV (433 (v.6)) |
by Cheung, T |
Mean free path of cosmic rays in the disturbance region behind IMF-shock causing forbush decrease at September 9, 1992 (433-436 (v.1)) |
by Fujimoto, K |
Monitoring of air crew exposure by an active dose assessment system (433-436 (v.2)) |
The effect of nonlinear front distortion on particle injection rate in the regime of shock wave acceleration (433-436 (v.4)) |
by Toptygin, I N |
Modulation effects in 1991-19982 years (437-440 (v.1)) |
by Belov, A V |
Effect of interplanetary clouds on geomagnetic storms (437-440 (v.2)) |
by Kumar, S |
New narrow angle muon telescope at Mt. Norikura (441 (v.1)) |
by Ohashi, Y |
Neutron flux from earth surface at new moon and full moon (441-444 (v.2)) |
by Volodichev, N N |
Is geminga the source of the Pleistocene beryllium-10 spikes ? (441-444 (v.4)) |
by Sonett, C P |
Barometric effect of cosmic rays as a function of several variables (445-448 (v.2)) |
by Yanchukovsky, V L |
Evidence of X-ray synchrotron emission from electrons accelerated to 30 TeV in the supernova Remnant Cassiopeia A (445-448 (v.4)) |
by Allen, G E |
Angular and temporary cosmic ray muon flux characteristics measured with large aperture scintillator hodoscope (449-452 (v.2)) |
by Borog, V V |
Is the mystery of the origin of galactic cosmic rays solved ? (449-452 (v.4)) |
by Allen, G E |
Calibration of neutron monitor using an accelerator (45-48 (v.1)) |
by Shibata, S |
Cosmic ray spectra deduced from neutron monitor surveys (45-48 (v.2)) |
by Bieber, J W |
On the possible correlation between gamma-ray bursts and radio-quiet quasars (45-48 (v.3)) |
by Hurley, K |
A study of cosmic ray composition using the CASA-MIA detector (45-48 (v.4)) |
by Catanese, M A |
Cosmic ray studies on the MIR space station: The experiment sileye (45-48 (v.5)) |
by Morselli, A |
Stratospoheric cosmic ray and ozone variations during last three cycles (453-456 (v.2)) |
by Martin, I M |
On pulsar wind effect on cosmic ray energy spectra produced by SNR (453-456 (v.4)) |
by Giller, M |
Multi-station comparative study of the nucleonic barometric coefficient dependences with altitude, cut-off rigidity and level of solar activity (457-460 (v.2)) |
by Dorman, L L |
Progenitors of cosmic-ray producing supernova remnants (457-460 (v.4)) |
by Lacey, C K |
Monte Carlo simulation of particle fluxes and cosmogenic nuclide production in the earth's atmosphere (461-464 (v.2)) |
by Masarik, J |
The pair production spectrum from photon-phon annihilation (461-464 (v.4)) |
by Böttcher, M |
Solar modulation of GCR in the last two centuries by radionuclides in meteorites (465-468 (v.2)) |
by Bonino, G |
The origin of cosmics rays above 10 eV (465-468 (v.4)) |
by Al-Dargazelli, S S |
Common long term periodicities in cosmogenic and climatic records over the last 3000 years (469-472 (v.2)) |
by Cini-Castagnoli, G |
Continuous observation of Be-7 in the atmosphere for 5 years (473-476 (v.2)) |
by Sakuraï, H |
The origin of the GCRII component (473-476 (v.4)) |
by Zank, G P |
Search for the origin of quiet-time particle fluxes in the inner heliosphere (477-480 (v.2)) |
by Kiraly, P |
The effects of voids and cores of galaxy clusters on the propagation of ultra-high energy cosmic rays (477-480 (v.4)) |
by Medina Tanco, G |
Proton and alpha particle fluxes during quiet conditions (481-484 (v.2)) |
by Kiraly, P |
Clustering of ultra-high energy cosmic rays: sources and time delay (481-484 (v.4)) |
by Medina Tanco, G |
Pesca instrument for low-energy cosmic ions study in photon satellite (485 (v.2)) |
by Del Peral, L |
Ultra high energy shock acceleration including photodisintegration (489-492 (v.4)) |
by Morfill, G E |
Direct deduction of the number of neutrons injected from the sun on the basis of neutron monitor response (49-52 (v.1)) |
by Kananen, H |
Different crossovers (49-52 (v.2)) |
by Reinecke, J P |
Measuring the cosmic ray composition at the Knee with BLANCA (49-52 (v.4)) |
by Fortson, L F |
Status of the PAMELA experiment for the study of cosmic antimatter in space (49-52 (v.5)) |
by Adriani, O |
Wstatus of the NESTOR Project (49-52 (v.7)) |
by Capone, A |
Energetic particle cross-field diffusion in turbulent magnetic fields (497-500 (v.4)) |
by Ostrowski, M |
Extended Gamma-Ray emission of the solar flares in june 1991 (5-8 (v.1)) |
by Rank, G |
Perpendicular diffusion and drift in solar modulation (5-8 (v.2)) |
by Bieber, J W |
Minute-timescale periodicities in Her X-1 (5-8 (v.3)) |
by Leahy, D A |
A new study on the composition of primary cosmic ray flux over the energy range 3X10 - 3x10 cV with the GRAPES III EAS array at OOTY (5-8 (v.4)) |
by Kawakami, S |
Cosmic ray Shower simulation and reconstruction for the ATIC experiment (5-8 (v.5)) |
by Wang, J Z |
Fragmentation of the projectile Pb nucleus in Pb-Pb interactions at 158 A GeV (5-8 (v.6)) |
by Wolter, W |
First look at AMANDA-B data (5-8 (v.7)) |
by Tilav, S |
Cosmic ray acceleration by a system of spherical shocks (501-504 (v.4)) |
by Klepach, E G |
Shock acceleration in non linear test particle picture (505 (v.4)) |
by Ko, C M |
The 64 m 2 solar neutron telescope at Norikura (53-56 (v.1)) |
by Muraki, Y |
Cycle 22 recovery for cosmic ray modulation (53-56 (v.2)) |
by Ahluwalia, H S |
The chemical composition of primary cosmic rays with energies from 10 to 10 eV (53-56 (v.4)) |
by Shirasaki, Y S |
On the possibility of measuring cosmic ray with energies up to 10 eV by direct methods on light satellites (53-56 (v.5)) |
by Grigorov, N L |
Detection efficiency of the first solar neutron telescope at Nirikura (57-60 (v.1)) |
by Matsubara, Y |
Features of GCR long-period modulation in heliosphere (57-60 (v.2)) |
by Alania, M V |
Status and results of the search for Gamma-ray bursts above 1 TeV with the HEGRA experiment (57-60 (v.3)) |
by Padilla, L |
A method to reconstruct the energy and determine the composition of cosmics rays from Cherenkov light and particle densities measurements of extended air showers (57-60 (v.4)) |
by Lindner, A |
Access-advanced cosmic ray composition experiment for the space station (57-60 (v.5)) |
by Isbert, J |
Unidimensional properties of hadronic matter above 10 GeV (57-60 (v.6)) |
by Capdevielle, J N |
Perspectives for neutrino astrophysics with NESTOR (57-60 (v.7)) |
by Bottai, S |
Detection efficiency of the Bolivian solar neutron detector (61-64 (v.1)) |
by Matsubara, Y |
Long-term cosmic ray variations: spectrum and relation with solar activity (61-64 (v.2)) |
by Belov, A V |
The search for the TeV counterparts in gamma ray bursts (61-64 (v.3)) |
by Boyle, P J |
The pulse shape of atmospheric Cerenkov signals (61-64 (v.4)) |
by Sinnott, M D |
Charge resolution parametrization for DE-E telescopes (61-64 (v.5)) |
by Bronchalo, E |
Comparison of experimental and simulated data on coplanar emission of extremely high-energy particles in multiple production (61-64 (v.6)) |
by Borisov, A S |
On the Kamiokande 8B solar neutrinos measurement (61-64 (v.7)) |
by Kitamura, T |
Impact of magnetic environment on the generation of high-energy neutron and gamma-rays during solar flares (65-68 (v.1)) |
by Kocharov, L G |
Characteristics of long-term cosmic ray modulation during different phases of sun spot cycles in relation with polarity of solar magnetic field (65-68 (v.2)) |
by Shrivastava, P K |
A southern hemisphere search for gamma ray bursts at the PeV and TeV energies (65-68 (v.3)) |
by Dazeley, S A |
Changes of the cosmic0ray mass composition at the Knee (65-68 (v.4)) |
by Bernlöhr, K |
An experiment to measure the elemental abundances of ultra-heavy cosmic rays (65-68 (v.5)) |
by Binns, W R |
Some regularities observed in hadronic interactions (65-68 (v.6)) |
by Shibuya, E H |
Origin of background events in the Kamiokande measurement (65-68 (v.7)) |
by Kitamura, T |
Simulation of energy spectra of ions from impulsive solar flares (69-72 (v.1)) |
by Kartavykh, Yu Yu |
High rigidity CR-SA hysteresis phenomenon and the dimension of modulation region in the heliosphere in dependence of particle rigidity (69-72 (v.2)) |
by Dorman, L I |
Gamma-ray burst studies with GLAST (69-72 (v.3)) |
by Bonnell, J T |
Cerenkov light based measurement of the chemical composition and energy spectrum of cosmic rays with the HEGRA detector (69-72 (v.4)) |
by Cortina, J |
GLAST: GeV astronomy with thousands of sources (69-72 (v.5)) |
by Dingus, B L |
Alignment of the energy distinguished cores and azimuthal effects at the superhigh energies EO 3.10 eV (69-72 (v.6)) |
by Yuldashbaev, T S |
Restoration and properties of solar proton spectra from different sources (73-76 (v.1)) |
by Miroshnichenko, L I |
Low rigidity CR-SA hysteresis phenomenon and average dimension of the modulation region and heliosphere (73-76 (v.2)) |
by Dorman, L I |
Search for gamma-ray bursts of E 1 GeV at Mt Chacaltaya (73-76 (v.3)) |
by Barthelemy, S |
Composition of cosmic rays from coincidences between atmospheric Cherenkov light and underground muons (73-76 (v.4)) |
by Mualem, L |
Detection of High energy electrons by GLAST (73-76 (v.5)) |
by Ormes, J F |
Spectral characteristics of SPEs related to Gamma ray events (77-80 (v.1)) |
by Pérez-Enriquez, R |
Long-term variation of cosmic-ray diurnal anisotropy observed by a network of multi-directional muon telescopes in a wide range of rigidity (77-80 (v.2)) |
by Munakata, K |
A search for cosmetic gamma ray bursts at GeV energies from simultaneous observations with grapes II and grapes III arrays at OOTY (77-80 (v.3)) |
by Tonwar, S C |
Cosmic ray composition in the Knee region inferred from underground multiple muons at Soudan (77-80 (v.4)) |
by Kasahara, K |
Hodoscopic CsI calorimeter for GLAST (77-80 (v.5)) |
by Norris, J P |
Frequency Distributions of solar proton events (81-84 (v.1)) |
by Mendoza, B S |
The magnetic cycle in cosmic ray anisotropies (81-84 (v.2)) |
by Bieber, J W |
SIGMA observations of X-ray novae (81-84 (v.3)) |
by Goldwurm, A |
About the new method of primary energy estimation selecting EAS at mountain altitudes (81-84 (v.4)) |
by Brankova, M |
The cosmic ray isotope spectrometer (CRIS) (v.5) (81-84 (v.5)) |
by Von Rosenvinge, T T |
The hadron spectrum at 840 g.cm average atmospheric depth (81-84 (v.6)) |
by Aglietta, M |
Observational signatures of the influence of solar ejecta on the associated low-energy protons events (85-88 (v.1)) |
by Rodriguez Pacheco, J |
Latitudinal and radial variation of 2 GeV protons and alpha particles derived by Ulysses COSPIN/KET and neutron monitor network observations (85-88 (v.2)) |
by Herber, B |
Spin modulated GeV Gamma-ray emission from centaurus X-3 (85-88 (v.3)) |
by Vestrand, W T |
A local source of high energy cosmic rays (85-88 (v.4)) |
by Erlykin, A D |
The ACE-CRIS scintillating optical fiber trajectory (SOFT) detector: calibrations at the NSCI, and GSI (85-88 (v.5)) |
by Hink, P L |
Experimental study of adronic interaction models using coincident data from EAS-Top and MACRO (85-88 (v.6)) |
by Spinetti, M |
Status of radio ice Cerenkov experiment (RICE) (85-88 (v.7)) |
by Allen, C |
Evidence for historical solar proton events from NO(X) precipitation in polar ice cores (89-92 (v.1)) |
by Dreschoff, G |
The radial intensity gradients of galactic and anomalous cosmic ray (89-92 (v.2)) |
by Fujii, Z |
Detection of the COS-B/EGRET source GRO J2227+61 (89-92 (v.3)) |
by Iyudin, A |
Estimation of the primary cosmic ray composition around 10 PeV (89-92 (v.4)) |
by Yuldashbaev, T S |
Intensity of super high energy hadrons observed with emulsion chambers at Yangbajing (89-92 (v.6)) |
by Lu, S L |
Alpha-alpha fusion reactions in solar flares: accelerated and ambient He abundances and Li production (9-12 (v.1)) |
by Mandzhavidze, N |
The cosmic ray diffusion tensor in the heliosphere (9-12 (v.2)) |
by Zank, G P |
6 and 20 cm observations of 1E survey X-ray sources (9-12 (v.3)) |
by Leahy, D A |
A new measurement on the composition of primary cosmic ray flux over the energy range 10 - 10 eV with the grapes II EAS array at OOTY (9-12 (v.4)) |
by Tonwar, S C |
Methodology for the primary cosmic-ray observation in RUNJOB-program-chamber designing and data processing (9-12 (v.5)) |
Charged particle production in the Pb + Pb system at 158 GeV/c per nucleon (9-12 (v.6)) |
by Deines-Jones, P. |
Analysis of cascades in AMANDA (9-12 (v.7)) |
by Porrata, R |
The ionic charge of solar energetic particles with energies of 0.3-70 MeV per nucleon (93-96 (v.1)) |
by Oetliker, M |
Compton-getting factor and latitude variation of cosmic rays (93-96 (v.2)) |
by Paizis, C |
A silicon-tungsten imaging calorimeter for high energy cosmic ray measurements (93-96 (v.4)) |
by Bravar, U |
Crimean Cherenkov Gamma-ray-telescope performance simulations and gamma-ray selection criterion (93-96 (v.5)) |
by Anokhina, A M |
Estimation of the cosmic ray composition with the KASCADE hadron calorimeter (93-96 (v.6)) |
by Hörandel, J R |
First results of a search of neutrino-induced muons on the earth's surface (93-96 (v.7)) |
by Aynutdinov, W |
Radial diffusion coefficient of galactic cosmic ray hydrogen and helium in the heliosphere (97-100 (v.2)) |
by Fujii, Z |
EGRET gamma ray poinbt sources above 1 GeV (97-100 (v.3)) |
by Reimer, O |
Correlations in arrival time and angle of incidence distributions of EAS muons (97-100 (v.4)) |
by Brancus, I M |
Telescope SHALON - 2 (97-100 (v.5)) |
by Sinitsyna, V G |
Energy deposition of 10 TeV Hadrons in the KASCADE Calorimeter (97-100 (v.6)) |
by Milke, J |
Systems development for a large - Scale astrophysical neutrino observatory (97-100 (v.7)) |
by He, Y |
A deconvolution technique to determine injection profiles and spectra of solar cosmic rays (97-100(v.1)) |
by Ruffolo, D |
Study of muon energy losses in the LVD experiment (v.6) |
by Sartorelli, G P |
The high energy muon spectrum in extensive air showers: first data from LVD and EAS-TOP at GRAN SASSO (v.6) |
by Sartorelli |
High Energy Muon - showers observed with emulsion chambers at Mt. Kanbala (v.6) |
by Ren, J R |
Single muon angular distribution for project GRAND (v.6) |
by Fields, B |
Search for stellar point sources with an enlarged sample of identified single muons (v.6) |
by Poirier, J |
Analyses of muons from the direction of Cygnus X-3 at large zenith angles 1992-1996 (v.6) |
by Wada, T |
A sky syurvey using muons in the MACRO detector (v.6) |
by Giglietto, N |
Measurements of the cosmic ray muon component in the atmosphere from ground level to balloon altitudes (v.6) |
by Basini, G |
Inelastic interactions of muons deep underground (v.6) |
by Aynutdinov, V M |
Monte Carlo simulation of muon transport in rock (v.6) |
by Lagutin, A A |
Simulation of neutron production by deep underground muons (v.6) |
by Ruddick K |
Intrinsic uncertainty in Monte Carlo Models of the underground muon flux (v.6) |
by Longley, N P |
A measurement of the mu+/mu- ratio at the top of the atmosphere with the Caprice experiment |
by Barbiellini, G |
The hadron spectrum at 840 $gcm^{-2}$ average atmospheric depth |
by Aglietta, M |
Primary composition analysis from muons in EAS |
by Aglietta, M |
Experimental study of hadronic interaction model using coincident data from EAS-TOP and MACRO |
by Aglietta, M |
The atmospheric neutrino flavor ratio in Soudan 2 |
by Goodman, M |