Statistical modeling of plasmaspheric hiss amplitude using solar wind measurements and geomagnetic indices
Version of Record online: 23 MAR 2012
Copyright 2012 by the American Geophysical Union
Geophysical Research Letters
Volume 39, Issue 6, 28 March 2012
How to Cite
2012), Statistical modeling of plasmaspheric hiss amplitude using solar wind measurements and geomagnetic indices, Geophys. Res. Lett., 39, L06103, doi:10.1029/2012GL051185., , , and (
- Issue online: 23 MAR 2012
- Version of Record online: 23 MAR 2012
- Manuscript Accepted: 24 FEB 2012
- Manuscript Revised: 22 FEB 2012
- Manuscript Received: 31 JAN 2012
- NSF. Grant Numbers: 1043442, 1137411
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|grl29050-sup-0001-readme.txt||plain text document||1K||readme.txt|
|grl29050-sup-0002-ts01.txt||plain text document||15K||Table S1. These are the model coefficients for each L/MLT bin for the model of plasmaspheric hiss amplitude.|
|grl29050-sup-0003-ms01.avi||application/x-troff-msvideo||37216K||Animation S1. An animation showing the modeled evolution of equatorial hiss amplitude in the range 2 < L < 5 from 03 September 2012 to 05 September 2012.|
|grl29050-sup-0004-t01.txt||plain text document||0K||Tab-delimited Table 1.|
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