← Назад к работе
Работы, на которые ссылается эта работа
Работ: 54
Работа: Electron radiation belt dynamics during magnetic storms and in quiet time
Why are relativistic electrons persistently quiet at geosynchronous orbit in 2009?
Ryuho Kataoka, Yoshizumi Miyoshi
Статья2010Цитирований: 2ABIMagnetospheric Substorms and the Sources of Inner Magnetosphere Particle Acceleration
Глава2011Цитирований: 2ABIExplaining sudden losses of outer radiation belt electrons during geomagnetic storms
D. L. Turner, Yuri Shprits, Michael D. Hartinger +1
Статья2012Цитирований: 2ABINumerical calculations of relativistic electron drift loss effect
Kyung Chan Kim, D.‐Y. Lee, H.‐J. Kim +4
Статья2008Цитирований: 2ABIThe global response of relativistic radiation belt electrons to the January 1997 magnetic cloud
G. D. Reeves, D. N. Baker, R. D. Belian +7
Статья1998Цитирований: 2ABITimescale for radiation belt electron acceleration by whistler mode chorus waves
R. B. Horne, S. A. Glauert, J. M. Albert +2
Статья2005Цитирований: 2ABIElectron acceleration in the magnetosphere by whistler-mode waves of varying frequency
A. G. Demekhov, V. Yu. Trakhtengerts, M.J. Rycroft +1
Статья2006Цитирований: 2ABIEvolution of relativistic outer belt electrons during an extended quiescent period
A. N. Jaynes, X. Li, Q. Schiller +9
Статья2014Цитирований: 2ABISolar particle dynamics during magnetic storms of July 23–27, 2004
S. N. Kuznetsov, Л. Л. Лазутин, M. I. Panasyuk +5
Статья2008Цитирований: 2ABIOutward radial diffusion driven by losses at magnetopause
Yuri Shprits, R. M. Thorne, R. Friedel +4
Статья2006Цитирований: 2ABI