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Global Zones of Particle Precipitation: EXOS-C’s Observation

DOI: 10.4236/oalib.1115274, PP. 1-20

Subject Areas: Astrophysics

Keywords: EXOS-C, LEO, SEPs, Magnetosphere, Response Function, Absolute Flux, L-Parameter

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Abstract

This article pertains to EXOS-C’s LEO observations during 1984-1986 of quasi-trapped protons (0.64 - 35 MeV) and electrons (0.19 - 3.2 MeV) with the main focus on the former. The temporal variation of proton population near the geomagnetic equator reveals that the peak value of the equatorially mirroring component may increase by a factor of 50 or more between a solar maximum and a minimum condition, and that the peak flux profile of protons in the equatorial, low latitude, midlatitude, and auroral zones lying to the north and south of the equator, exist in parallel with the minimum magnetic field equator. Further, the proton and the electron populations in the said midlatitude zone show longitude and altitude dependencies. The locations of the peak profiles in all three zones in L-space depend upon the pitch angles of particles the distribution of which shows a second peak in addition to the one at 90? pitch angle. Particle flux does not depend on the local time. However, there is a great seasonal variation in e and p fluxes, possibly due to the solar condition. Particle flux variations are indicative of the presence of scattering by electromagnetic waves generated by both solar wind disturbances and magnetospheric instabilities. These waves and the ring current particles interact to redistribution of particles spatially and energy-wise. The energy spectra of both p and e fluxes run almost parallel. Theoretical understanding of these observations is in progress with the work of data analysis of other parts of the global zones. Subject AreasAstrophysics

Cite this paper

Adel, M. M. (2026). Global Zones of Particle Precipitation: EXOS-C’s Observation. Open Access Library Journal, 13, e15274. doi: http://dx.doi.org/10.4236/oalib.1115274.

References

[1]  Zhang, J., Blanco-Cano, X., Nitta, N., Srivastava, N. and Mandrini, C.H. (2018) Editorial: Earth-Affecting Solar Transients. <i>Solar Physics</i>, 293, Article No. 80. <br>https://doi.org/10.1007/s11207-018-1302-9
[2]  Gopalswamy, N. (2016) History and Development of Coronal Mass Ejections as a Key Player in Solar Terrestrial Relationship. <i>Geoscience Letters</i>, 3, Article No. 8. <br>https://doi.org/10.1186/s40562-016-0039-2
[3]  Banu, S.A., Lugaz, N., Zhuang, B., Al-Haddad, N., Farrugia, C.J. and Galvin, A.B. (2025) Investigating Coronal Mass Ejections through Multispacecraft Measurements: STEREO-A and L1 in 2022-2023. <i>The Astrophysical Journal</i>, 982, Article No. 47. <br>https://doi.org/10.3847/1538-4357/adb60c
[4]  Zhuang, B., Lugaz, N., Wood, B.E., Braga, C.R., Temmer, M., Gou, T., <i>et al</i>. (2025) Evolution of a Coronal Mass Ejection with an Eruptive Prominence from the Corona to Interplanetary Space. <i>The Astrophysical Journal</i>, 990, Article No. 181. <br>https://doi.org/10.3847/1538-4357/adf2a9
[5]  Pal, S., Mac Cormack, C., Kilpua, E.K.J., Yogesh, Jian, L.K. and Nieves-Chinchilla, T. (2025) Magnetic Interaction Analysis of Multiple Interplanetary Coronal Mass Ejections That Led to a Historic Geomagnetic Storm in May 2024. <i>Astronomy & Astrophysics</i>, 702, A150. <br>https://doi.org/10.1051/0004-6361/202555908
[6]  Mohil, M., Singh, S. and Jha, R. (2025) Hybrid LSTM-GRU Model for Predicting Solar Activity and Geomagnetic Indices. <i>Astrophysics and Space Science</i>, 370, Article No. 118. <br>https://doi.org/10.1007/s10509-025-04510-y
[7]  M&#246;stl, C., Davies, E.E., Weiler, E., R&#252;disser, H.T., Amerstorfer, U.V., Weiss, A.J., <i>et al</i>. (2026) On the Magnetic Field Evolution of Interplanetary Coronal Mass Ejections from 0.07 to 5.4 Au. <i>The Astrophysical Journal</i>, 1001, Article No. 70. <br>https://doi.org/10.3847/1538-4357/ae50fe
[8]  Lamy, P., Boursier, Y. Loirat, J. and Zhukov, A. (2025) Three-Dimensional Reconstruction and Propagation of an Asymmetric Flux-Rope Coronal Mass Ejection.
[9]  R&#252;disser, H.T., Nguyen, G., Le Lou&#235;dec, J., Davies, E.E. and M&#246;stl, C. (2026) ARCANE-Early Detection of Interplanetary Coronal Mass Ejections. <i>Space Weather</i>, 24, e2025SW004537. <br>https://doi.org/10.1029/2025sw004537
[10]  R&#252;disser, H.T., Davies, E.E., Amerstorfer, U.V., <i>et al</i>. (2026) Towards a Fully Automated Pipeline for Short-Term Forecasting of <i>in Situ</i> Coronal Mass Ejection Magnetic Field Structure.
[11]  Mannucci, A.J., Tsurutani, B.T., Iijima, B.A., Komjathy, A., Saito, A., Gonzalez, W.D., <i>et al</i>. (2005) Dayside Global Ionospheric Response to the Major Interplanetary Events of October 29-30, 2003 &#8220;Halloween Storms&#8221;. <i>Geophysical Research Letters</i>, 32, L12S02. <br>https://doi.org/10.1029/2004gl021467
[12]  Tsurutani, B.T. and Lakhina, G.S. (2014) An Extreme Coronal Mass Ejection and Consequences for the Magnetosphere and Earth. <i>Geophysical Research Letters</i>, 41, 287-292. <br>https://doi.org/10.1002/2013gl058825
[13]  Hayakawa, H., Ebihara, Y., Mishev, A., Koldobskiy, S., Kusano, K., Bechet, S., <i>et al</i>. (2025) The Solar and Geomagnetic Storms in 2024 May: A Flash Data Report. <i>The Astrophysical Journal</i>, 979, Article No. 49. <br>https://doi.org/10.3847/1538-4357/ad9335
[14]  Li, G., Zank, G.P. and Rice, W.K.M. (2003) Energetic Particle Acceleration and Transport at Coronal Mass Ejection-Driven Shocks. <i>Journal of Geophysical Research</i>:<i> Space Physics</i>, 108, Article No. 1082. <br>https://doi.org/10.1029/2002ja009666
[15]  Tsurutani, B., Mannucci, A., Iijima, B., Abdu, M.A., Sobral, J.H.A., Gonzalez, W., <i>et al</i>. (2004) Global Dayside Ionospheric Uplift and Enhancement Associated with Interplanetary Electric Fields. <i>Journal of Geophysical Research</i>:<i> Space Physics</i>, 109, A08302. <br>https://doi.org/10.1029/2003ja010342
[16]  Tsurutani, B.T., Verkhoglyadova, O.P., Mannucci, A.J., Saito, A., Araki, T., Yumoto, K., <i>et al</i>. (2008) Prompt Penetration Electric Fields (PPEFs) and Their Ionospheric Effects during the Great Magnetic Storm of 30-31 October 2003. <i>Journal of Geophysical Research</i>:<i> Space Physics</i>, 113, A05311. <br>https://doi.org/10.1029/2007ja012879
[17]  Zong, Q., Reinisch, B.W., Song, P., Wei, Y. and Galkin, I.A. (2010) Dayside Ionospheric Response to the Intense Interplanetary Shocks-solar Wind Discontinuities: Observations from the Digisonde Global Ionospheric Radio Observatory. <i>Journal of Geophysical Research</i>:<i> Space Physics</i>, 115, A06304. <br>https://doi.org/10.1029/2009ja014796
[18]  Liu, Y.D., Hu, H., Wang, R., Yang, Z., Zhu, B., Liu, Y.A., <i>et al</i>. (2015) Plasma and Magnetic Field Characteristics of Solar Coronal Mass Ejections in Relation to Geomagnetic Storm Intensity and Variability. <i>The Astrophysical Journal</i>, 809, L34. <br>https://doi.org/10.1088/2041-8205/809/2/l34
[19]  Baker, D.N., Jaynes, A.N., Kanekal, S.G., Foster, J.C., Erickson, P.J., Fennell, J.F., <i>et al</i>. (2016) Highly Relativistic Radiation Belt Electron Acceleration, Transport, and Loss: Large Solar Storm Events of March and June 2015. <i>Journal of Geophysical Research</i>:<i> Space Physics</i>, 121, 6647-6660. <br>https://doi.org/10.1002/2016ja022502
[20]  Baker, D.N., Jaynes, A.N., Turner, D.L., Nakamura, R., Schmid, D., Mauk, B.H., <i>et al</i>. (2016) A Telescopic and Microscopic Examination of Acceleration in the June 2015 Geomagnetic Storm: Magnetospheric Multiscale and Van Allen Probes Study of Substorm Particle Injection. <i>Geophysical Research Letters</i>, 43, 6051-6059. <br>https://doi.org/10.1002/2016gl069643
[21]  Reiff, P.H., Daou, A.G., Sazykin, S.Y., Nakamura, R., Hairston, M.R., Coffey, V., <i>et al</i>. (2016) Multispacecraft Observations and Modeling of the 22/23 June 2015 Geomagnetic Storm. <i>Geophysical Research Letters</i>, 43, 7311-7318. <br>https://doi.org/10.1002/2016gl069154
[22]  Liu, Y., Fu, L., Wang, J. and Zhang, C. (2018) Studying Ionosphere Responses to a Geomagnetic Storm in June 2015 with Multi-Constellation Observations. <i>Remote Sensing</i>, 10, Article No. 666. <br>https://doi.org/10.3390/rs10050666
[23]  Liu, G., Huang, W., Shen, H., Aa, E., Li, M., Liu, S., <i>et al</i>. (2019) Ionospheric Response to the 2018 Sudden Stratospheric Warming Event at Middle-and Low-Latitude Stations over China Sector. <i>Space Weather</i>, 17, 1230-1240. <br>https://doi.org/10.1029/2019sw002160
[24]  Venkatesh, K., Tulasi Ram, S., Fagundes, P.R., Seemala, G.K. and Batista, I.S. (2017) Electrodynamic Disturbances in the Brazilian Equatorial and Low-Latitude Ionosphere on St. Patrick&#8217;s Day Storm of 17 March 2015. <i>Journal of Geophysical Research</i>:<i> Space Physics</i>, 122, 4553-4570. <br>https://doi.org/10.1002/2017ja024009
[25]  Astafyeva, E., Zakharenkova, I. and Alken, P. (2016) Prompt Penetration Electric Fields and the Extreme Topside Ionospheric Response to the June 22-23, 2015 Geomagnetic Storm as Seen by the Swarm Constellation. <i>Earth</i>,<i> Planets and Space</i>, 68, Article No. 152. <br>https://doi.org/10.1186/s40623-016-0526-x
[26]  Anastasiadis, A., Papaioannou, A., Sandberg, I., Georgoulis, M., Tziotziou, K., Kouloumvakos, A., <i>et al</i>. (2017) Predicting Flares and Solar Energetic Particle Events: The FORSPEF Tool. <i>Solar Physics</i>, 292, Article No. 134. <br>https://doi.org/10.1007/s11207-017-1163-7
[27]  Belakhovsky, V.B., Pilipenko, V.A., Antonova, E.E., Miyoshi, Y., Kasahara, Y., Kasahara, S., <i>et al</i>. (2023) Relativistic Electron Flux Growth during Storm and Non-Storm Periods as Observed by ARASE and GOES Satellites. <i>Earth</i>,<i> Planets and Space</i>, 75, Article No. 189. <br>https://doi.org/10.1186/s40623-023-01925-1
[28]  Kalegaev, V.V., Ivanova, A.R., Gruzdov, D.S., Vlasova, N.A., Bazilevskaya, G.A. and Makhmutov, V.S. (2023) Energetic Electrons Precipitation into the Earth&#8217;s Atmosphere during Magnetic Storm on 1-5 February 2015. In: Kosterov, A., <i>et al</i>., Eds., <i>Springer Proceedings in Earth and Environmental Sciences</i>, Springer International Publishing, 301-312. <br>https://doi.org/10.1007/978-3-031-40728-4_22
[29]  Gao, L., Shen, C., Zhou, Y., Ji, Y., Pu, Z., Parks, G., <i>et al</i>. (2024) Observational Features of Charge Distribution in Earth&#8217;s Inner Magnetosphere. <i>Communications Physics</i>, 7, Article No. 63. <br>https://doi.org/10.1038/s42005-024-01553-5
[30]  Papaioannou, A., Sandberg, I., Anastasiadis, A., Kouloumvakos, A., Georgoulis, M.K., Tziotziou, K., <i>et al</i>. (2016) Solar Flares, Coronal Mass Ejections and Solar Energetic Particle Event Characteristics. <i>Journal of Space Weather and Space Climate</i>, 6, A42. <br>https://doi.org/10.1051/swsc/2016035
[31]  Laurenza, M., Cliver, E.W., Hewitt, J., Storini, M., Ling, A.G., Balch, C.C., <i>et al</i>. (2009) A Technique for Short-Term Warning of Solar Energetic Particle Events Based on Flare Location, Flare Size, and Evidence of Particle Escape. <i>Space Weather</i>, 7, S04008. <br>https://doi.org/10.1029/2007sw000379
[32]  Tsyganenko, N.A. and Sitnov, M.I. (2005) Modeling the Dynamics of the Inner Magnetosphere during Strong Geomagnetic Storms. <i>Journal of Geophysical Research</i>:<i> Space Physics</i>, 110, A03208. <br>https://doi.org/10.1029/2004ja010798
[33]  Sun, X., Zhima, Z., Duan, S., Hu, Y., Lu, C. and Ran, Z. (2024) Statistical Analysis of the Correlation between Geomagnetic Storm Intensity and Solar Wind Parameters from 1996 to 2023. <i>Remote Sensing</i>, 16, Article No. 2952. <br>https://doi.org/10.3390/rs16162952
[34]  Biswas, S., Bhaskar, A., Abitha, S.G., <i>et al</i>. (2026) Unprecedented Multipoint Observation of Spatially Varying ICME Turbulence of Different Ages during October 2024 Extreme Solar Storm at 1 AU.
[35]  Davies, E.E., Weiler, E., M&#246;stl, C., <i>et al</i>. (2025) Real-Time Prediction of Geomagnetic Storms Using Solar Orbiter as a Far Upstream Solar Wind Monitor. <i>ESS Open Archive</i>. <br>https://doi.org/10.22541/essoar.175580321.18096327/v1
[36]  European Space Agency (ESA) (2021) ACE (Advanced Composition Explorer)&#8212;Mission Status. ESA eoPortal Directory. <br>https://directory.eoportal.org/web/eoportal/satellite-missions/a/ace
[37]  Strickland, A. (2025) Voyager 1 Will Reach One Light-Day from Earth in 2026. Here&#8217;s What That Means. <br>https://www.cnn.com/2025/12/09/science/voyager-1-light-day-earth#:~:text=By-Ashley%20Strickland,-DEC%209%2C%202025
[38]  Smith, P.H. and Bewtra, N.K. (1976) Dependence of the Charge Exchange Lifetimes on Mirror Latitude. <i>Geophysical Research Letters</i>, 3, 689-692. <br>https://doi.org/10.1029/gl003i011p00689
[39]  Cornwall, J.M., Coroniti, F.V. and Thorne, R.M. (1970) Turbulent Loss of Ring Current Protons. <i>Journal of Geophysical Research</i>, 75, 4699-4709. <br>https://doi.org/10.1029/ja075i025p04699
[40]  Williams, D.J., Hernandez, G. and Lyons, L.R. (1976) Simultaneous Observations of the Proton Ring Current and Stable Auroral Red Arcs. <i>Journal of Geophysical Research</i>, 81, 608-616. <br>https://doi.org/10.1029/ja081i004p00608
[41]  Mizera, P.F. and Blake, J.B. (1973) Observations of Ring Current Protons at Low Altitudes. <i>Journal of Geophysical Research</i>, 78, 1058-1062. <br>https://doi.org/10.1029/ja078i007p01058
[42]  Hovestadt, D., H&#228;usler, B. and Scholer, M. (1972) Observation of Energetic Particles at Very Low Altitudes near the Geomagnetic Equator. <i>Physical Review Letters</i>, 28, 1340-1344. <br>https://doi.org/10.1103/physrevlett.28.1340
[43]  Moritz, J. (1972) Energetic Protons at Low Equatorial Altitudes: A Newly Discovered Radiation Belt Phenomenon and Its Explanation. <i>Zeitschrift</i><i> f&#252;r </i><i>Geophysik</i>, 38, 701-717.
[44]  Scholer, M., Hovestadt, D. and Morfill, G. (1975) Energetic He<sup>+</sup> Ions from the Radiation Belt at Low Altitudes near the Geomagnetic Equator. <i>Journal of Geophysical Research</i>, 80, 80-85. <br>https://doi.org/10.1029/ja080i001p00080
[45]  Fischer, H.M., Auschrat, V.W. and Wibberenz, G. (1977) Angular Distribution and Energy Spectra of Protons of Energy 5 &#8804; <i>e</i> &#8804; 50 Mev at the Lower Edge of the Radiation Belt in Equatorial Latitudes. <i>Journal</i> <i>of</i> <i>Geophysical</i> <i>Research</i>, 82, 537-547. <br>https://doi.org/10.1029/ja082i004p00537
[46]  Claflin, E.S. and White, R.S. (1974) A Study of Equatorial Inner Belt Protons from 2 to 200 Mev. <i>Journal of Geophysical Research</i>, 79, 959-965. <br>https://doi.org/10.1029/ja079i007p00959
[47]  Parsignault, D.R., Holeman, E. and Filz, R.C. (1981) Long-Term Intensity Decrease in the 8-to 25-MeV Proton Fluxes at Low <i>L</i> Values. <i>Journal of Geophysical Research</i>:<i> Space Physics</i>, 86, 11447-11450. <br>https://doi.org/10.1029/ja086ia13p11447
[48]  Miah, M.A. (1989) Observation of Low Energy Particle Precipitation at Low Altitude in the Equatorial Zone. <i>Journal of Atmospheric and Terrestrial Physics</i>, 51, 541-549. <br>https://doi.org/10.1016/0021-9169(89)90094-9
[49]  Miah, M.A. (1991) Global Proton Peak Flux Profile in the Equatorial Zone. <i>Indian Journal of Radio and Space Science</i>, 20, 12-24.
[50]  Miah, M.A. (1991) The ONR-602 Experiment and Investigation of Particle Precipitation near the Equator. <i>Journal of Geomagnetism and </i><i>Geoelectricity</i>, 43, 445-460. <br>https://doi.org/10.5636/jgg.43.445
[51]  Miah, M.A., Nagata, K., Kohno, T., Murakami, H., Nakamoto, A., Hasebe, N., <i>et al</i>. (1992) Spatial and Temporal Features of 0.64-35 MeV Protons in the Space Station Environment: EXOS-C Observations. <i>Journal of Geomagnetism and </i><i>Geoelectricity</i>, 44, 591-610. <br>https://doi.org/10.5636/jgg.44.591
[52]  Miah, M.A. (1991) Observation of Z &#8805; 1 Particles Below 300 km near the Geomagnetic Equator. <i>Journal of Geomagnetism and </i><i>Geoelectricity</i>, 43, 461-475. <br>https://doi.org/10.5636/jgg.43.461
[53]  Coffey, H. (1992) NOAA, Boulder, Colorado, Private Communication.
[54]  Fahr, H.J. and Shizgal, B. (1983) Modern Exospheric Theories and Their Observational Relevance. <i>Reviews of Geophysics</i>, 21, 75-124. <br>https://doi.org/10.1029/rg021i001p00075
[55]  Jacchia, L.G. (1977) Thermospheric Temperature, Density, and Composition: New Models. Smithsonian Astrophysical Observatory, Special Report No. 375.

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