2020
DOI: 10.26464/epp2020034
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An empirical model of the global distribution of plasmaspheric hiss based on Van Allen Probes EMFISIS measurements

Abstract: Key Points:The empirical model is a third-order polynomial function of L-shell, magnetic local time (MLT), magnetic latitude (MLAT), and AE* q The model can perform the hiss amplitude distribution by L/MLT and L/MLAT q All data are based on Van Allen Probes EMFISIS measurements q Abstract: Using wave measurements from the EMFISIS instrument onboard Van Allen Probes, we investigate statistically the spatial distributions of the intensity of plasmaspheric hiss waves. To reproduce these empirical results, we esta… Show more

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Cited by 3 publications
(2 citation statements)
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References 45 publications
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“…Wang et al. (2020) built a fitting model for the spatial distribution of the hiss intensity. A third‐order polynomial function of L‐shell, magnetic local time (MLT), magnetic latitude, and AE* was adopted in this fitting algorithm.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…Wang et al. (2020) built a fitting model for the spatial distribution of the hiss intensity. A third‐order polynomial function of L‐shell, magnetic local time (MLT), magnetic latitude, and AE* was adopted in this fitting algorithm.…”
Section: Introductionmentioning
confidence: 99%
“…Meanwhile, in the research of Golden et al (2012), they used the sequential feature selection to determine optimal historical time series of relevant geomagnetic parameters. Wang et al (2020) built a fitting model for the spatial distribution of the hiss intensity. A third-order polynomial function of L-shell, magnetic local time (MLT), magnetic latitude, and AE* was adopted in this fitting algorithm.…”
mentioning
confidence: 99%