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DETECTING NEAR-TAIL CURRENT SHEET FORMATION USING ISOTROPIC BOUNDARIES: LESSONS FROM GLOBAL MHD. / Gordeev, E.I. ; Apatenkov, S.V. .

Physics of Auroral Phenomena: Proceedings of the 43 rd Annual Seminar. 2020. p. 11-14.

Research output: Chapter in Book/Report/Conference proceedingConference contributionResearchpeer-review

Harvard

Gordeev, EI & Apatenkov, SV 2020, DETECTING NEAR-TAIL CURRENT SHEET FORMATION USING ISOTROPIC BOUNDARIES: LESSONS FROM GLOBAL MHD. in Physics of Auroral Phenomena: Proceedings of the 43 rd Annual Seminar. pp. 11-14, Physics of Auroral Phenomena, Apatity, Russian Federation, 10/03/20.

APA

Gordeev, E. I., & Apatenkov, S. V. (2020). DETECTING NEAR-TAIL CURRENT SHEET FORMATION USING ISOTROPIC BOUNDARIES: LESSONS FROM GLOBAL MHD. In Physics of Auroral Phenomena: Proceedings of the 43 rd Annual Seminar (pp. 11-14)

Vancouver

Gordeev EI, Apatenkov SV. DETECTING NEAR-TAIL CURRENT SHEET FORMATION USING ISOTROPIC BOUNDARIES: LESSONS FROM GLOBAL MHD. In Physics of Auroral Phenomena: Proceedings of the 43 rd Annual Seminar. 2020. p. 11-14

Author

Gordeev, E.I. ; Apatenkov, S.V. . / DETECTING NEAR-TAIL CURRENT SHEET FORMATION USING ISOTROPIC BOUNDARIES: LESSONS FROM GLOBAL MHD. Physics of Auroral Phenomena: Proceedings of the 43 rd Annual Seminar. 2020. pp. 11-14

BibTeX

@inproceedings{b21eb7a0bcce4a2581fac7fe795a9aba,
title = "DETECTING NEAR-TAIL CURRENT SHEET FORMATION USING ISOTROPIC BOUNDARIES: LESSONS FROM GLOBAL MHD",
abstract = "A number of recent studies suggests an existence of magnetotail current sheet configurations with tailward Bz gradient during the growth phase of the substorm. Such configurations are especially interesting since they are potentially unstable for different types of instabilities and can lead to explosive reconfiguration of the magnetosphere. However, the observations are rare and ability to observe tailward gradients is very limited. Here we use the global MHD configuration with near-tail Bz minimum to investigate the regions with adiabatic and nonadiabatic behavior of energetic particles. Thus we estimate the locations of the isotropic boundaries for the modelled POES-type spacecraft flybys. We expect that the lessons learned from global MHD simulation may become helpful in exploration of non-monotonic tail current sheet configuration using observations on low-orbiting spacecraft.",
author = "E.I. Gordeev and S.V. Apatenkov",
year = "2020",
language = "English",
pages = "11--14",
booktitle = "Physics of Auroral Phenomena",
note = "null ; Conference date: 10-03-2020 Through 13-03-2020",

}

RIS

TY - GEN

T1 - DETECTING NEAR-TAIL CURRENT SHEET FORMATION USING ISOTROPIC BOUNDARIES: LESSONS FROM GLOBAL MHD

AU - Gordeev, E.I.

AU - Apatenkov, S.V.

PY - 2020

Y1 - 2020

N2 - A number of recent studies suggests an existence of magnetotail current sheet configurations with tailward Bz gradient during the growth phase of the substorm. Such configurations are especially interesting since they are potentially unstable for different types of instabilities and can lead to explosive reconfiguration of the magnetosphere. However, the observations are rare and ability to observe tailward gradients is very limited. Here we use the global MHD configuration with near-tail Bz minimum to investigate the regions with adiabatic and nonadiabatic behavior of energetic particles. Thus we estimate the locations of the isotropic boundaries for the modelled POES-type spacecraft flybys. We expect that the lessons learned from global MHD simulation may become helpful in exploration of non-monotonic tail current sheet configuration using observations on low-orbiting spacecraft.

AB - A number of recent studies suggests an existence of magnetotail current sheet configurations with tailward Bz gradient during the growth phase of the substorm. Such configurations are especially interesting since they are potentially unstable for different types of instabilities and can lead to explosive reconfiguration of the magnetosphere. However, the observations are rare and ability to observe tailward gradients is very limited. Here we use the global MHD configuration with near-tail Bz minimum to investigate the regions with adiabatic and nonadiabatic behavior of energetic particles. Thus we estimate the locations of the isotropic boundaries for the modelled POES-type spacecraft flybys. We expect that the lessons learned from global MHD simulation may become helpful in exploration of non-monotonic tail current sheet configuration using observations on low-orbiting spacecraft.

UR - http://pgia.ru:81/seminar/archive/2020/Proceedings_2020.pdf

M3 - Conference contribution

SP - 11

EP - 14

BT - Physics of Auroral Phenomena

Y2 - 10 March 2020 through 13 March 2020

ER -

ID: 77727043