The Response of Electron Pitch Angle Distributions to the Upper Limit on Stably Trapped Particles

Author:

Walton S. D.1ORCID,Mann I. R.2ORCID,Olifer L.2ORCID,Ozeke L. G.2ORCID,Forsyth C.3ORCID,Rae I. J.4ORCID,Walach M.‐T.5ORCID,Murphy K. R.46ORCID,Claudepierre S. G.7,Spence H. E.8ORCID,Baker D. N.9ORCID

Affiliation:

1. Space Sciences Laboratory University of California Berkeley CA USA

2. Department of Physics University of Alberta Edmonton AB Canada

3. Mullard Space Science Laboratory University College London Dorking UK

4. Department of Maths, Physics and Electrical Engineering Northumbria University Newcastle upon Tyne UK

5. Department of Physics Lancaster University Lancaster UK

6. Self Thunder Bay ON Canada

7. Department of Atmospheric and Oceanic Sciences University of California Los Angeles CA USA

8. Institute for the Study of Earth, Oceans, and Space University of New Hampshire Durham NH USA

9. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA

Abstract

AbstractWe use Van Allen Probes electron data during 70 geomagnetic storms to examine the response of equatorial pitch angle distributions (PADs) at L* = 4.0–4.5 to a theoretical upper limit on stably trapped particle fluxes. Of the energies examined, 54 and 108 keV electron PADs isotropize to a previously assumed level within 6 hr of reaching the limit, near‐identically across all 70 storms, consistent with rapid pitch angle scattering due to chorus wave interactions. In around 30% of events, 54 keV electrons completely exceed the KP limit, before being quickly subdued. 470 and 749 keV PADs show clear indications of an upper limit, though less aligned with the calculated limit used here. The consistency of an absolute upper limit shown across all events demonstrates the importance of this phenomena in both the limiting effect on electron flux and consistently influencing electron PAD evolution during geomagnetic storms. These results also highlight the need for further investigation, particularly related to the limiting of higher energy electrons.

Funder

National Aeronautics and Space Administration

Science and Technology Facilities Council

Natural Environment Research Council

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

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