It has been suggested that Earth's ambipolar electric field be merged into this article. (Discuss) Proposed since September 2024. |
The polar wind or plasma fountain is a permanent outflow of plasma from the polar regions of Earth's magnetosphere.[2]: 29 [3] Conceptually similar to the solar wind, It is one of several mechanisms for the outflow of ionized particles. Ions accelerated by a polarization electric field known as an ambipolar electric field[2] is believed to be the primary cause of polar wind. Similar processes operate on other planets.[4]
History
In 1966 Bauer[5] and, separately, Dessler ahd Michel[6] noted that since the Earth's geomagnetic field above the poles forms a long tail away from the Sun out beyond the Moon's orbit, ions should flow from the higher pressure region in the ionosphere out into space.[7] The term "polar wind" was coined in 1968 in a pair of articles by Banks and Holzer[8] and by Ian Axford.[9] Since the process by which the ionospheric plasma flows away from the Earth along magnetic field lines is similar to the flow of solar plasma away from the Sun's corona (the solar wind), Axford suggested the term "polar wind."
The idea for the polar wind originated with the desire to solve the paradox of the terrestrial helium budget. This paradox consists of the fact that helium in the Earth's atmosphere seems to be produced (via radioactive decay of uranium and thorium) faster than it is lost by escaping from the upper atmosphere. The realization that some helium could be ionized, and therefore escape the Earth along open magnetic field lines near the magnetic poles (the 'polar wind'), is one possible solution to the paradox.
Causes
After 30 years of research, the "classical" cause of the polar wind has been shown to be ambipolar outflow of thermal plasma: ion acceleration by a polarization electric field at high altitudes.[2]: 451 In this region the ionospheric plasma expands and the low density allows gravity to pull ions down relative to the electrons in the plasma. The charge separation results in the electric field which then sends some of the ions up and out of the atmosphere.[11]: 147 This mechanism is known as "ambipolar outflow"[12] and the field as "ambipolar electric field" or "polarization electric field". Additional mechanisms include ion acceleration by solar photoelectrons escaping along magnetic field lines.[12]
The outflow of ions due to the ambipolar electric field end up accumulating in the plasmasphere if they follow closed magnetic field lines but ions following open magnetic field lines exit the Earth system.[11]: 167 Ions following open magnetic field lines are push away from the Sun by forces of the solar wind (anti-solar convection).[11]{rp|149}}
Measurements
Numerous investigations of the polar wind have launched,including ISIS-2, Dynamics Explorer, the Akebono satellite, and the Polar satellite, covering a variety of altitudes, latitudes, and times relative to the solar cycle. Some of the conclusions include:[13]
- electrons, and the ions H+,He+, O+ are the primary ingredients in the polar wind; O+ dominates at below 4000km,
- polar wind velocity increases with altitude, and is higher on the dayside of the Earth,
- all three ion species reach supersonic velocities above 7000km.
The polarization or ambipolar electric field was measured in 2022 by a sounding rocket launched from Svalbard. This NASA mission was called Endurance.[10] Comparing the electrical potential at altitude of 250 km to that at 768 km gave a difference of +0.55 volt with an uncertainty of 0.09 volt.[14] The voltage is similar to that used in a wristwatch battery but is sufficient to account for the polar wind.[15]
See also
References
- ^ Plasma fountain Source, press release: Carlowicz, Mike; "Solar Wind Squeezes Some of Earth's Atmosphere into Space", December 1998
- ^ a b c Schunk, R. W.; Nagy, Andrew (2000). Ionospheres: physics, plasma physics, and chemistry. Cambridge atmospheric and space science series. New York: Cambridge University Press. ISBN 978-0-521-63237-9.
- ^ "AMS Glossary". Archived from the original on 2007-10-31. Retrieved 2008-05-08.
- ^ Gronoff, G.; Arras, P.; Baraka, S.; Bell, J. M.; Cessateur, G.; Cohen, O.; Curry, S. M.; Drake, J. J.; Elrod, M.; Erwin, J.; Garcia-Sage, K.; Garraffo, C.; Glocer, A.; Heavens, N. G.; Lovato, K. (August 2020). "Atmospheric Escape Processes and Planetary Atmospheric Evolution". Journal of Geophysical Research: Space Physics. 125 (8). Bibcode:2020JGRA..12527639G. doi:10.1029/2019JA027639. ISSN 2169-9380.
- ^ Bauer, S.J. (1966). "The structure of the topside ionosphere". In Frihagen, J. (ed.). Electron Density Profiles in Ionosphere and Exosphere. North-Holland.
- ^ Dessler, A. J.; Michel, F. C. (1966-03-01). "Plasma in the geomagnetic tail". Journal of Geophysical Research. 71 (5): 1421–1426. doi:10.1029/JZ071i005p01421.
- ^ Schunk, R. W.; Sojka, J. J. (June 1997). "Global ionosphere‐polar wind system during changing magnetic activity". Journal of Geophysical Research: Space Physics. 102 (A6): 11625–11651. doi:10.1029/97JA00292. ISSN 0148-0227.
- ^ Banks, Peter M.; Holzer, Thomas E. (1968). "The Polar Wind". Journal of Geophysical Research. 73 (21): 6846–6854. Bibcode:1968JGR....73.6846B. doi:10.1029/JA073i021p06846.
- ^ Axford, W. Ian (1968). "The Polar Wind and the Terrestrial Helium Budget". Journal of Geophysical Research. 73 (21): 6855–6859. Bibcode:1968JGR....73.6855A. doi:10.1029/JA073i021p06855.
- ^ a b Lacey Young (28 August 2024), Discovering Earth’s Third Global Energy Field, NASA
- ^ a b c Welling, Daniel T.; André, Mats; Dandouras, Iannis; Delcourt, Dominique; Fazakerley, Andrew; Fontaine, Dominique; Foster, John; Ilie, Raluca; Kistler, Lynn; Lee, Justin H.; Liemohn, Michael W.; Slavin, James A.; Wang, Chih-Ping; Wiltberger, Michael; Yau, Andrew (2015). "The Earth: Plasma Sources, Losses, and Transport Processes". Space Science Reviews. 192 (1–4): 145–208. Bibcode:2015SSRv..192..145W. doi:10.1007/s11214-015-0187-2. ISSN 0038-6308.
- ^ a b Schunk, R. W. (2007-11-01). "Time-dependent simulations of the global polar wind". Journal of Atmospheric and Solar-Terrestrial Physics. Recent Advances in the Polar Wind Theories and Observations. 69 (16): 2028–2047. Bibcode:2007JASTP..69.2028S. doi:10.1016/j.jastp.2007.08.009. ISSN 1364-6826.
- ^ Yau, Andrew W.; Abe, Takumi; Peterson, W. K. (2007-11-01). "The polar wind: Recent observations". Journal of Atmospheric and Solar-Terrestrial Physics. Recent Advances in the Polar Wind Theories and Observations. 69 (16): 1936–1983. doi:10.1016/j.jastp.2007.08.010. ISSN 1364-6826.
- ^ Collinson, Glyn A.; Glocer, Alex; Pfaff, Robert; Barjatya, Aroh; Conway, Rachel; Breneman, Aaron; Clemmons, James; Eparvier, Francis; Michell, Robert; Mitchell, David; Imber, Suzie; Akbari, Hassanali; Davis, Lance; Kavanagh, Andrew; Robertson, Ellen (2024-08-28), "Earth's ambipolar electrostatic field and its role in ion escape to space", Nature, 632 (8027): 1021–1025, doi:10.1038/s41586-024-07480-3, ISSN 1476-4687
- ^ "Discovering Earth's Third Energy Field". svs.gsfc.nasa.gov. Retrieved 2024-09-12.
External links
- Young, Lacey (2024-08-28). "Discovering Earth's Third Global Energy Field". NASA Scientific Visualization Studio. NASA. Retrieved 2024-09-12.