On application of asymmetric Kan-like exact equilibria to the Earth magnetotail modeling

Korovinskiy, Daniil B.; Kubyshkina, Darya I.; Semenov, Vladimir S.; Kubyshkina, Marina V.; Erkaev, Nikolai V.; Kiehas, Stefan A.

doi:10.5194/angeo-36-641-2018

Articles | Volume 36, issue 2

https://doi.org/10.5194/angeo-36-641-2018

© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

https://doi.org/10.5194/angeo-36-641-2018

© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 36, issue 2

Regular paper

|

19 Apr 2018

Regular paper |

| 19 Apr 2018

On application of asymmetric Kan-like exact equilibria to the Earth magnetotail modeling

Daniil B. Korovinskiy, Darya I. Kubyshkina, Vladimir S. Semenov, Marina V. Kubyshkina, Nikolai V. Erkaev, and Stefan A. Kiehas

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Cumulative views and downloads (calculated since 17 Jan 2018)

Month	HTML	PDF	XML	Total
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Feb 2018	88	6	17	111
Mar 2018	44	10	2	56
Apr 2018	99	28	6	133
May 2018	147	18	1	166
Jun 2018	48	8	1	57
Jul 2018	7	5	0	12
Aug 2018	10	3	0	13
Sep 2018	7	7	0	14
Oct 2018	9	8	0	17
Nov 2018	17	5	0	22
Dec 2018	11	5	2	18
Jan 2019	10	9	0	19
Feb 2019	11	11	0	22
Mar 2019	9	10	0	19
Apr 2019	10	16	0	26
May 2019	17	11	0	28
Jun 2019	28	11	0	39
Jul 2019	9	12	0	21
Aug 2019	14	15	2	31
Sep 2019	13	15	0	28
Oct 2019	46	44	1	91
Nov 2019	7	4	0	11
Dec 2019	9	4	0	13
Jan 2020	11	12	1	24
Feb 2020	13	11	0	24
Mar 2020	9	12	1	22
Apr 2020	6	4	0	10
May 2020	10	9	0	19
Jun 2020	25	10	0	35
Jul 2020	22	31	11	64
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Aug 2024	18	12	5	35
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Oct 2024	9	3	2	14
Nov 2024	6	2	1	9
Dec 2024	9	4	1	14
Jan 2025	4	7	0	11
Feb 2025	14	4	1	19
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Apr 2025	5	6	0	11
May 2025	15	8	6	29
Jun 2025	28	6	0	34
Jul 2025	17	19	3	39
Aug 2025	9	11	3	23
Sep 2025	31	21	1	53
Oct 2025	18	26	4	48
Nov 2025	29	17	1	47
Dec 2025	15	16	1	32
Jan 2026	33	14	8	55
Feb 2026	25	12	3	40
Mar 2026	1	12	1	14

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Short summary

The Harris–Fadeev–Kan–Manankova family of exact two-dimensional equilibria is generalized to reproduce the slow decrease of the normal magnetic component in the tailward direction, and the magnetotail current sheet bending and shifting in the vertical plane, arising from the Earth dipole tilting and the solar wind nonradial propagation. The analytical solution is found to fit the empirical T96 model, especially, at distances beyond 10–15 Earth radii at high levels of magnetospheric activity.


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