Articles | Volume 36, issue 5
https://doi.org/10.5194/angeo-36-1335-2018
https://doi.org/10.5194/angeo-36-1335-2018
Regular paper
 | 
08 Oct 2018
Regular paper |  | 08 Oct 2018

Statistical study of ULF waves in the magnetotail by THEMIS observations

Shuai Zhang, Anmin Tian, Quanqi Shi, Hanlin Li, Alexander W. Degeling, I. Jonathan Rae, Colin Forsyth, Mengmeng Wang, Xiaochen Shen, Weijie Sun, Shichen Bai, Ruilong Guo, Huizi Wang, Andrew Fazakerley, Suiyan Fu, and Zuyin Pu

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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to revisions (further review by editor and referees) (25 Jul 2018) by Minna Palmroth
AR by Anmin Tian on behalf of the Authors (28 Jul 2018)  Author's response   Manuscript 
ED: Referee Nomination & Report Request started (08 Aug 2018) by Minna Palmroth
RR by Anonymous Referee #2 (15 Aug 2018)
RR by Anonymous Referee #1 (14 Sep 2018)
ED: Publish as is (14 Sep 2018) by Minna Palmroth
AR by Anmin Tian on behalf of the Authors (18 Sep 2018)  Manuscript 
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Short summary
The features of ULF waves are statistically studied on the magnetotail stretched magnetic field lines (8 RE < R < 32 RE) by using 8 years of THEMIS data. The occurrence rates of ULF waves are higher in the post-midnight region than pre-midnight region. The frequency decreases with increasing radial distance of 8–16 RE and could be explained by much more standing waves in this region than in the region of 16–32 RE. The wave frequency is higher after the substorm onset than before it.