Articles | Volume 38, issue 4
https://doi.org/10.5194/angeo-38-931-2020
https://doi.org/10.5194/angeo-38-931-2020
Regular paper
 | 
28 Aug 2020
Regular paper |  | 28 Aug 2020

Outer Van Allen belt trapped and precipitating electron flux responses to two interplanetary magnetic clouds of opposite polarity

Harriet George, Emilia Kilpua, Adnane Osmane, Timo Asikainen, Milla M. H. Kalliokoski, Craig J. Rodger, Stepan Dubyagin, and Minna Palmroth

Data sets

Index of /data_pub G. Reeves https://www.rbsp-ect.lanl.gov/data_pub

GOES Space Environment Monitor NOAA https://www.ngdc.noaa.gov/stp/satellite/goes/index.html

Public data from current and past space physics missions T. Kovalick https://cdaweb.gsfc.nasa.gov/index.html/

Final Dst index H. Toh http://wdc.kugi.kyoto-u.ac.jp/dst_final/index.html

Near-Earth Interplanetary Coronal Mass Ejections Since January 1996 I. Richardson and H. Cane http://www.srl.caltech.edu/ACE/ASC/DATA/level3/icmetable2.htm

Data Index S. Bounds https://emfisis.physics.uiowa.edu/data/index

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Short summary
We compared trapped outer radiation belt electron fluxes to high-latitude precipitating electron fluxes during two interplanetary coronal mass ejections (ICMEs) with opposite magnetic cloud rotation. The electron response had many similarities and differences between the two events, indicating that different acceleration mechanisms acted. Van Allen Probe data were used for trapped electron flux measurements, and Polar Operational Environmental Satellites were used for precipitating flux data.