002025802 001__ 2025802
002025802 003__ SzGeCERN
002025802 005__ 20151107000001.0
002025802 0247_ $$2DOI$$9World Scientific$$a10.1142/9789814603164_0011
002025802 0248_ $$aoai:inspirehep.net:1320833$$pcerncds:CERN$$qINSPIRE:HEP$$qForCDS
002025802 035__ $$9http://inspirehep.net/oai2d$$aoai:inspirehep.net:1320833$$d2015-06-15T12:35:38Z$$h2015-06-17T04:00:08Z$$mmarcxml
002025802 035__ $$9Inspire$$a1320833
002025802 041__ $$aeng
002025802 100__ $$aBobik, P
002025802 245__ $$aEVALUATION OF ENERGETIC PROTON PRESSURE DURING SOLAR EVENTS AND POSSIBLE EFFECTS ON THE MAGNETOSPHERE
002025802 260__ $$c2014
002025802 300__ $$a6 p
002025802 520__ $$9World Scientific$$aDuring solar events (such as flares or CME), energetic protons are accelerated in interplanetary medium. These particles are called briefly SEP (solar energetic particles). We estimated the SEP contribution to solar wind pressure. We used data collected by ACE and GOES, in particular during 4 periods, each one of 15 days. Each period is centered on a significant solar flare. We investigated possible effects on terrestrial geomagnetic field.
002025802 65017 $$2SzGeCERN$$aAstrophysics and Astronomy
002025802 690C_ $$aCERN
002025802 700__ $$aBoschini, M J
002025802 700__ $$aTorre, S Della
002025802 700__ $$aGervasi, M
002025802 700__ $$aGrandi, D
002025802 700__ $$aKudela, K
002025802 700__ $$aVacca, G La
002025802 700__ $$aMallamaci, M$$uCERN
002025802 700__ $$aPensotti, S
002025802 700__ $$aRancoita, P G
002025802 700__ $$aRozza, D$$uCERN
002025802 700__ $$aTacconi, M
002025802 773__ $$c67-72$$wC13-09-23.3$$y2014
002025802 960__ $$a13
002025802 962__ $$b1599993$$k67-72$$ncomo20130923
002025802 980__ $$aARTICLE
002025802 980__ $$aConferencePaper