evolution of the plasma sheet electron pitch angle distribution by whistler-mode chorus waves in non-dipole magnetic fields
Clicks: 153
ID: 234356
2012
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This
article has not been analysed, so there is no overall score —
reader engagement is measured and shown alongside.
Reader Engagement
Emerging Content
30.0
/100
153 views
16 readers
AI Quality Assessment
Not analyzed
Readership in this journal
EmergingRanked #140 of 484 articles by views in journal of food measurement and characterization
Most read
Least read
Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 484 in total.
Mint this article as an NFT
Not yet mintedCreate a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.
5
SUSD
one-off · no wallet required
Abstract
We present a detailed numerical study on the effects of a non-dipole magnetic
field on the Earth's plasma sheet electron distribution and its implication
for diffuse auroral precipitation. Use of the modified bounce-averaged
Fokker-Planck equation developed in the companion paper by
Ni et al. (2012) for 2-D non-dipole magnetic fields suggests that we
can adopt a numerical scheme similar to that used for a dipole field, but
should evaluate bounce-averaged diffusion coefficients and bounce period
related terms in non-dipole magnetic fields. Focusing on nightside
whistler-mode chorus waves at L = 6, and using various Dungey magnetic
models, we calculate and compare of the bounce-averaged diffusion
coefficients in each case. Using the Alternative Direction Implicit (ADI)
scheme to numerically solve the 2-D Fokker-Planck diffusion equation, we
demonstrate that chorus driven resonant scattering causes plasma sheet
electrons to be scattered much faster into loss cone in a non-dipole field
than a dipole. The electrons subject to such scattering extends to lower
energies and higher equatorial pitch angles when the southward interplanetary
magnetic field (IMF) increases in the Dungey magnetic model. Furthermore, we
find that changes in the diffusion coefficients are the dominant factor
responsible for variations in the modeled temporal evolution of plasma sheet
electron distribution. Our study demonstrates that the effects of realistic
ambient magnetic fields need to be incorporated into both the evaluation of
resonant diffusion coefficients and the calculation of Fokker-Planck
diffusion equation to understand quantitatively the evolution of plasma sheet
electron distribution and the occurrence of diffuse aurora, in particular at
L > 5 during geomagnetically disturbed periods when the ambient magnetic
field considerably deviates from a magnetic dipole.
| Reference Key |
ma2012annalesevolution
Use this key to autocite in the manuscript while using
SciMatic Manuscript Manager or Thesis Manager
|
|---|---|
| Authors | ;Q. Ma;B. Ni;X. Tao;R. M. Thorne |
| Journal | journal of food measurement and characterization |
| Year | 2012 |
| DOI |
10.5194/angeo-30-751-2012
|
| URL | |
| Keywords |
Citations
No citations found. To add a citation, contact the admin at info@scimatic.org
Comments
No comments yet. Be the first to comment on this article.