Home » Spasojevic and Shprits 2013

Chorus functional dependencies derived from CRRES data

Spasojevic M., Y. Y. Shprits, (2013), Chorus functional dependencies derived from CRRES data, Geophysical Research Letters, 40, 3793-3797, doi:10.1002/grl.50755

Abstract

Using data from the Combined Release and Radiation Effects Satellite (CRRES) plasma wave experiment, we present quadratic fits to the mean of the wave amplitude squared, , for lower and upper band chorus as a function of geomagnetic activity (Kp) and magnetic latitude (λ) for the midnight (21 MLT≤3), dawn (3 MLT≤9), and postnoon (12 MLT≤15) sectors and present an ad hoc model for the prenoon (9 MLT≤12) sector. The empirical models are valid for 4≤L≤7, |λ| 15° and Kp≤6 and quantify the dramatic difference in the latitudinal dependence of chorus as a function of local time and how that dependence varies with geomagnetic condition, critical parameters for calculating wave-induced electron scattering rates. Our results are generally consistent with previous studies, and our key contribution is the quantification of wave properties in a manner that is easily incorporated into global quasi-linear diffusion models.

Authors (sorted by name)

Shprits Spasojevic

Journal / Conference

Geophysical Research Letters

Acknowledgments

This work was supported by NASA award NNX09AF51G and NSF award 0902846.

Grants

0902846 NNX09AF51G

Bibtex

@article{doi:10.1002/grl.50755,
author = {Spasojevic, M. and Shprits, Y. Y.},
title = {Chorus functional dependencies derived from CRRES data},
journal = {Geophysical Research Letters},
year = {2013},
volume = {40},
number = {15},
pages = {3793-3797},
keywords = {chorus waves, wave-particle interactions, electron scattering},
doi = {10.1002/grl.50755},
url = {https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1002/grl.50755},
eprint = {https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/grl.50755},
abstract = {Using data from the Combined Release and Radiation Effects Satellite (CRRES) plasma wave experiment, we present quadratic fits to the mean of the wave amplitude squared, , for lower and upper band chorus as a function of geomagnetic activity (Kp) and magnetic latitude (λ) for the midnight (21 MLT≤3), dawn (3 MLT≤9), and postnoon (12 MLT≤15) sectors and present an ad hoc model for the prenoon (9 MLT≤12) sector. The empirical models are valid for 4≤L≤7, |λ| 15° and Kp≤6 and quantify the dramatic difference in the latitudinal dependence of chorus as a function of local time and how that dependence varies with geomagnetic condition, critical parameters for calculating wave-induced electron scattering rates. Our results are generally consistent with previous studies, and our key contribution is the quantification of wave properties in a manner that is easily incorporated into global quasi-linear diffusion models.}
}