Reply to 'The dynamics of Van Allen belts revisited'
Reply to 'The dynamics of Van Allen belts revisited'
复制标题
回复“重新审视范艾伦皮带的动态”
DOI:
10.1038/nphys4351
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发表时间:
2018
期刊:
影响因子:
19.6
通讯作者:
Mann I
中科院分区:
文献类型:
--
作者:
Mann I
Mann et al. reply—We are pleased to address the comment on our paper1 from Shprits et al. 2 since we believe it supports our conclusion that magnetopause shadowing and ultralow-frequency (ULF) wave outward transport can drive fast losses into the heart of the ultra-relativistic electron radiation belt and produce a remnant belt. As reported by Baker et al. 3, the September 2012 geomagnetic storm produced this phenomena, and we showed1 how such losses could explain it. However, Shprits et al. claim that for this single specific storm that electromagnetic ion cyclotron (EMIC) wave losses are essential for explaining the observed third belt. We dispute this interpretation. Contrary to the claims of Shprits et al., outward ULF wave radial diffusion can act on sufficiently short timescales4 to generate the observed remnant belt. For example, Supplementary Fig. 1 displays additional magnetopause shadowing simulation runs using the same approach described in ref. 1 showing an erosion of the outer belt and the generation of both monotonic and non-monotonic PSD profiles without invoking EMIC wave effects. Our ULF wave-driven radiation belt simulations not only reproduce the third belt morphology but also produce a narrower remnant belt at higher energies just as observed (Supplementary Fig. 2).The principal argument for the action of EMIC wave loss in the Shprits et al. Correspondence is based on analysis of electron phase space density (PSD) profiles. However, we disagree with their analysis and the derived PSD profiles since they do not appear to take into account uncertainties in measurements at the lowest REPT instrument energy channels,