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Access via FulcrumEnergy distribution of electrons with E < 800 eV in the areomagnetosphere
| dc.contributor.author | Shutte, N. M. | en_US |
| dc.contributor.author | Dyachkov, A. V. | en_US |
| dc.contributor.author | Gringauz, K. I. | en_US |
| dc.contributor.author | Sheronova, S. M. | en_US |
| dc.contributor.author | Verigin, M. I. | en_US |
| dc.contributor.author | Kiraly, P. | en_US |
| dc.contributor.author | Szego, K. | en_US |
| dc.contributor.author | Szemerey, I. | en_US |
| dc.contributor.author | Szucs, I. T. | en_US |
| dc.contributor.author | Tatrallyay, M. | en_US |
| dc.contributor.author | Cravens, Tom E. | en_US |
| dc.contributor.author | Gombosi, Tamas I. | en_US |
| dc.contributor.author | Nagy, Andrew F. | en_US |
| dc.contributor.author | Sharp, W. F. | en_US |
| dc.date.accessioned | 2006-04-10T14:52:32Z | |
| dc.date.available | 2006-04-10T14:52:32Z | |
| dc.date.issued | 1991 | en_US |
| dc.identifier.citation | Shutte, N. M., Dyachkov, A. V., Gringauz, K. I., Sheronova, S., Verigin, M. I., Kiraly, P., Szego, K., Szemerey, I., Szucs, I. T., Tatrallyay, M., Cravens, T. E., Gombosi, T. I., Nagy, A. F., Sharp, W. F. (1991)."Energy distribution of electrons with E < 800 eV in the areomagnetosphere." Planetary and Space Science 39(1-2): 147-151. <http://hdl.handle.net/2027.42/29560> | en_US |
| dc.identifier.uri | http://www.sciencedirect.com/science/article/B6V6T-46YK45Y-1VH/2/fe4a2a8c47524061f89958c21d1f6b1a | en_US |
| dc.identifier.uri | https://hdl.handle.net/2027.42/29560 | |
| dc.description.abstract | The electron distribution functions measured in the neighborhood of Mars by means of the Hyperbolic Retarding Potential Analyzer (HARP) carried aboard the Phobos 2 spacecraft are presented. The measurements were carried out over an energy/charge (E/q) from ~0.3 eV to ~800 eV in eight independent angular sectors ~ 20[deg] x 10[deg] covering the FOV ~ 180[deg] in the X-Z plane in the antisolar directions.The total intensity and energy distribution function of electrons downstream of the bow shock clearly differ from those in the undisturbed solar wind. The electron fluxes are significantly increased and the energy distribution of electrons in the magnetosheath was found to be characterized by the double-peaked structure. The high energy fluxes often exceed the flux values for the low energy peak. | en_US |
| dc.format.extent | 396316 bytes | |
| dc.format.extent | 3118 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.format.mimetype | text/plain | |
| dc.language.iso | en_US | |
| dc.publisher | Elsevier | en_US |
| dc.title | Energy distribution of electrons with E < 800 eV in the areomagnetosphere | en_US |
| dc.type | Article | en_US |
| dc.rights.robots | IndexNoFollow | en_US |
| dc.subject.hlbsecondlevel | Atmospheric, Oceanic and Space Sciences | en_US |
| dc.subject.hlbtoplevel | Science | en_US |
| dc.description.peerreviewed | Peer Reviewed | en_US |
| dc.contributor.affiliationum | University of Michigan, Ann Arbor, MI 48109-2143, U.S.A. | en_US |
| dc.contributor.affiliationum | University of Michigan, Ann Arbor, MI 48109-2143, U.S.A. | en_US |
| dc.contributor.affiliationum | University of Michigan, Ann Arbor, MI 48109-2143, U.S.A. | en_US |
| dc.contributor.affiliationother | Space Research Institute, U.S.S.R. Academy of Sciences, Profsoyuznaya 84/32, Moscow 117810, U.S.S.R. | en_US |
| dc.contributor.affiliationother | Space Research Institute, U.S.S.R. Academy of Sciences, Profsoyuznaya 84/32, Moscow 117810, U.S.S.R. | en_US |
| dc.contributor.affiliationother | Space Research Institute, U.S.S.R. Academy of Sciences, Profsoyuznaya 84/32, Moscow 117810, U.S.S.R. | en_US |
| dc.contributor.affiliationother | Space Research Institute, U.S.S.R. Academy of Sciences, Profsoyuznaya 84/32, Moscow 117810, U.S.S.R. | en_US |
| dc.contributor.affiliationother | Space Research Institute, U.S.S.R. Academy of Sciences, Profsoyuznaya 84/32, Moscow 117810, U.S.S.R. | en_US |
| dc.contributor.affiliationother | Central Research Institute for Physics, PO Box 49, H-1525, Budapest, Hungary | en_US |
| dc.contributor.affiliationother | Central Research Institute for Physics, PO Box 49, H-1525, Budapest, Hungary | en_US |
| dc.contributor.affiliationother | Central Research Institute for Physics, PO Box 49, H-1525, Budapest, Hungary | en_US |
| dc.contributor.affiliationother | Central Research Institute for Physics, PO Box 49, H-1525, Budapest, Hungary | en_US |
| dc.contributor.affiliationother | Central Research Institute for Physics, PO Box 49, H-1525, Budapest, Hungary | en_US |
| dc.contributor.affiliationother | University of Kansas, Lawrence, KS 66045, U.S.A. | en_US |
| dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/29560/1/0000648.pdf | en_US |
| dc.identifier.doi | http://dx.doi.org/10.1016/0032-0633(91)90137-Y | en_US |
| dc.identifier.source | Planetary and Space Science | en_US |
| dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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