Source and seed populations for relativistic electrons: Their roles in radiation belt changes
Journal Article
·
· Journal of Geophysical Research. Space Physics
- Univ. of Colorado, Boulder, CO (United States)
- NOAA Space Weather Prediction Center, Boulder, CO (United States)
- Univ. of Colorado, Boulder, CO (United States); NOAA National Centers for Environmental Information, Boulder, CO (United States)
- NASA Goddard Space Flight Center, Greenbelt, MD (United States)
- Aerospace Corporation, Los Angeles, CA (United States)
- Univ. of California, Los Angeles, CA (United States)
- Univ. of Iowa, Iowa City, IA (United States)
- Univ. of New Hampshire, Durham, NH (United States)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Strong enhancements of outer Van Allen belt electrons have been shown to have a clear dependence on solar wind speed and on the duration of southward interplanetary magnetic field. However, individual case study analyses also have demonstrated that many geomagnetic storms produce little in the way of outer belt enhancements and, in fact, may produce substantial losses of relativistic electrons. In this study, focused upon a key period in August–September 2014, we use GOES geostationary orbit electron flux data and Van Allen Probes particle and fields data to study the process of radiation belt electron acceleration. One particular interval, 13–22 September, initiated by a short-lived geomagnetic storm and characterized by a long period of primarily northward interplanetary magnetic field (IMF), showed strong depletion of relativistic electrons (including an unprecedented observation of long-lasting depletion at geostationary orbit) while an immediately preceding, and another immediately subsequent, storm showed strong radiation belt enhancement. We demonstrate with these data that two distinct electron populations resulting from magnetospheric substorm activity are crucial elements in the ultimate acceleration of highly relativistic electrons in the outer belt: the source population (tens of keV) that give rise to VLF wave growth and the seed population (hundreds of keV) that are, in turn, accelerated through VLF wave interactions to much higher energies. ULF waves may also play a role by either inhibiting or enhancing this process through radial diffusion effects. Furthermore, if any components of the inner magnetospheric accelerator happen to be absent, the relativistic radiation belt enhancement fails to materialize.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC52-06NA25396
- OSTI ID:
- 1236779
- Report Number(s):
- LA-UR--15-27789
- Journal Information:
- Journal of Geophysical Research. Space Physics, Journal Name: Journal of Geophysical Research. Space Physics Journal Issue: 9 Vol. 120; ISSN 2169-9380
- Publisher:
- American Geophysical UnionCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Similar Records
Ultra-low-frequency wave-driven diffusion of radiation belt relativistic electrons
Prompt acceleration of magnetospheric electrons to ultrarelativistic energies by the 17 March 2015 interplanetary shock
Rapid Enhancements of the Seed Populations in the Heart of the Earth's Outer Radiation Belt: A Multicase Study
Journal Article
·
Mon Dec 21 19:00:00 EST 2015
· Nature Communications
·
OSTI ID:1236062
Prompt acceleration of magnetospheric electrons to ultrarelativistic energies by the 17 March 2015 interplanetary shock
Journal Article
·
Sun Aug 14 20:00:00 EDT 2016
· Journal of Geophysical Research. Space Physics
·
OSTI ID:1499330
Rapid Enhancements of the Seed Populations in the Heart of the Earth's Outer Radiation Belt: A Multicase Study
Journal Article
·
Mon Jun 11 20:00:00 EDT 2018
· Journal of Geophysical Research. Space Physics
·
OSTI ID:1558215