Statistical and Solar Cycle Distribution of Daily Flux $\ge 10^{9}\mbox{ cm}^{-2}$ d−1 sr−1 for $E>2$ MeV Electrons Observed by GOES During 1987

Statistical and Solar Cycle Distribution of Daily Flux $\ge 10^{9}\mbox{ cm}^{-2}$ d−1 sr−1 for $E>2$ MeV Electrons Observed by GOES During 1987 – 2019

Published:2021-01 Issue:1 Volume:296 Page:
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Le Gui-Ming^ORCID,Zhang Yi-Ning,Zhao Ming-Xian

Funder

National Natural Science Foundation of China

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-020-01758-1.pdf

Reference27 articles.

1. Baker, D.N., Kanekal, S.G.: 2008, Solar cycle changes, geomagnetic variations, and energetic particle properties in the inner magnetosphere. J. Atmos. Solar-Terr. Phys. 70, 195. DOI.

2. Baker, D.N., Kanekal, S.G., Blake, J.B.: 2004, Characterizing the Earth’s outer Van Allen zone using a radiation belt content index. Space Weather 2, S02003. DOI.

3. Baker, D.N., Belian, R.D., Higbie, P.R., Klebesadel, R.W., Blake, J.B.: 1987, Deep dielectric charging effects due to high-energy electrons in Earth’s outer magnetosphere. J. Electrost. 20, 3. DOI.

4. Baker, D.N., Kanekal, S., Blake, J.B., Klecker, B., Rostoker, G.: 1994, Satellite anomalies linked to electron increase in the magnetosphere. Eos Trans. AGU 75, 401. DOI.

5. Baker, D.N., Li, X., Turner, N., Allen, J.H., Bargatze, L.F., Blake, J.B., et al.: 1997, Recurrent geomagnetic storms and relativistic electron enhancements in the outer magnetosphere: ISTP coordinated measurements. J. Geophys. Res. 102(A7), 14141. DOI.

Cited by 5 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Solar cycle and seasonal distribution of geomagnetic activities based on Ap indices from 1932 to 2018;CHINESE J GEOPHYS-CH;2022

2. Properties of the Geomagnetic Storm Main Phase and the Corresponding Solar Wind Parameters on 21–22 October 1999;Universe;2022-06-23

3. Can We Estimate the Intensities of Great Geomagnetic Storms (ΔSYM-H ≤ −200 nT) with the Burton Equation or the O’Brien and McPherron Equation?;The Astrophysical Journal;2022-03-01

4. Source Locations and Solar-Cycle Distribution of the Major Geomagnetic Storms ($\mathrm{Dst} \le -100$ nT) from 1932 to 2018;Solar Physics;2021-12

5. Characteristics of source location and solar cycle distribution of the strong solar proton events (≥ 1000 pfu) from 1976 to 2018;Monthly Notices of the Royal Astronomical Society;2021-01-22