Thin Current Sheet Formation and Reconnection at X ∼ −10 RE During the Main Phase of a Magnetic Storm

Standard

Thin Current Sheet Formation and Reconnection at X ∼ −10 R_E During the Main Phase of a Magnetic Storm. / Runov, A.; Angelopoulos, V.; Weygand, J. M.; Artemyev, A. V.; Beyene, F.; Sergeev, V.; Kubyshkina, M.; Henderson, M. G.

In: journal of geophysical research: Space Physics, Vol. 127, No. 9, e2022JA030669, 01.09.2022.

Research output: Contribution to journal › Article › peer-review

Harvard

Runov, A, Angelopoulos, V, Weygand, JM, Artemyev, AV, Beyene, F, Sergeev, V , Kubyshkina, M & Henderson, MG 2022, 'Thin Current Sheet Formation and Reconnection at X ∼ −10 R_E During the Main Phase of a Magnetic Storm', journal of geophysical research: Space Physics, vol. 127, no. 9, e2022JA030669. https://doi.org/10.1029/2022ja030669

APA

Runov, A., Angelopoulos, V., Weygand, J. M., Artemyev, A. V., Beyene, F., Sergeev, V., Kubyshkina, M., & Henderson, M. G. (2022). Thin Current Sheet Formation and Reconnection at X ∼ −10 R_E During the Main Phase of a Magnetic Storm. journal of geophysical research: Space Physics, 127(9), [e2022JA030669]. https://doi.org/10.1029/2022ja030669

Vancouver

Runov A, Angelopoulos V, Weygand JM, Artemyev AV, Beyene F, Sergeev V et al. Thin Current Sheet Formation and Reconnection at X ∼ −10 R_E During the Main Phase of a Magnetic Storm. journal of geophysical research: Space Physics. 2022 Sep 1;127(9). e2022JA030669. https://doi.org/10.1029/2022ja030669

Author

Runov, A. ; Angelopoulos, V. ; Weygand, J. M. ; Artemyev, A. V. ; Beyene, F. ; Sergeev, V. ; Kubyshkina, M. ; Henderson, M. G. / Thin Current Sheet Formation and Reconnection at X ∼ −10 R_E During the Main Phase of a Magnetic Storm. In: journal of geophysical research: Space Physics. 2022 ; Vol. 127, No. 9.

BibTeX

@article{c8f8129f7e62414d959211eeab005ae7,

title = "Thin Current Sheet Formation and Reconnection at X ∼ −10 RE During the Main Phase of a Magnetic Storm",

abstract = "The main question addressed in this study is whether particles with relativistic energy can be injected directly into the inner magnetosphere by very near-Earth reconnection during magnetic storms. We study a sequence of events observed in the solar wind, in the magnetotail, at geosynchronous orbit (GEO), in the inner magnetosphere, and in the ionosphere during the main phase of a geomagnetic storm on 16 June 2012–17 June 2012. The storm was caused by a magnetic cloud with a high dynamic pressure and a strong southward IMF lasting about 10 hr. These conditions caused an extreme compression of the magnetosphere (SymH reached ∼150 nT) and an enhancement of the lobe magnetic field strength to ∼90 nT at R ∼ 10 Earth radii (RE). We focus on an hour-long interval between 1050 and 1150 UT on 17 June 2012 when the Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellites were at apogee at geocentric distances R ≈ 12 RE near midnight. At that time a thin current sheet formed between cis-GEO distances and THEMIS. This thin current sheet reconnected between GEO and THEMIS. A strong lobe magnetic field enabled ion and electron energization to energies E ≈ 600 keV. Fluxes of high energy (up to relativistic) particles at GEO increased within ≈20 s after reconnection onset detected by THEMIS. Fluxes of relativistic electrons at L ∼ 4 in the morning sector increased within about 600 s after reconnection onset. We interpret these observations as signatures of direct injection of reconnected particles into the inner magnetosphere.",

keywords = "injections, magnetic storm, magnetosphere, plasma sheet, reconnection, ring current",

author = "A. Runov and V. Angelopoulos and Weygand, {J. M.} and Artemyev, {A. V.} and F. Beyene and V. Sergeev and M. Kubyshkina and Henderson, {M. G.}",

year = "2022",

month = sep,

day = "1",

doi = "10.1029/2022ja030669",

language = "English",

volume = "127",

journal = "Journal of Geophysical Research: Space Physics",

issn = "2169-9380",

publisher = "Wiley-Blackwell",

number = "9",

}

RIS

TY - JOUR

T1 - Thin Current Sheet Formation and Reconnection at X ∼ −10 RE During the Main Phase of a Magnetic Storm

AU - Runov, A.

AU - Angelopoulos, V.

AU - Weygand, J. M.

AU - Artemyev, A. V.

AU - Beyene, F.

AU - Sergeev, V.

AU - Kubyshkina, M.

AU - Henderson, M. G.

PY - 2022/9/1

Y1 - 2022/9/1

N2 - The main question addressed in this study is whether particles with relativistic energy can be injected directly into the inner magnetosphere by very near-Earth reconnection during magnetic storms. We study a sequence of events observed in the solar wind, in the magnetotail, at geosynchronous orbit (GEO), in the inner magnetosphere, and in the ionosphere during the main phase of a geomagnetic storm on 16 June 2012–17 June 2012. The storm was caused by a magnetic cloud with a high dynamic pressure and a strong southward IMF lasting about 10 hr. These conditions caused an extreme compression of the magnetosphere (SymH reached ∼150 nT) and an enhancement of the lobe magnetic field strength to ∼90 nT at R ∼ 10 Earth radii (RE). We focus on an hour-long interval between 1050 and 1150 UT on 17 June 2012 when the Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellites were at apogee at geocentric distances R ≈ 12 RE near midnight. At that time a thin current sheet formed between cis-GEO distances and THEMIS. This thin current sheet reconnected between GEO and THEMIS. A strong lobe magnetic field enabled ion and electron energization to energies E ≈ 600 keV. Fluxes of high energy (up to relativistic) particles at GEO increased within ≈20 s after reconnection onset detected by THEMIS. Fluxes of relativistic electrons at L ∼ 4 in the morning sector increased within about 600 s after reconnection onset. We interpret these observations as signatures of direct injection of reconnected particles into the inner magnetosphere.

AB - The main question addressed in this study is whether particles with relativistic energy can be injected directly into the inner magnetosphere by very near-Earth reconnection during magnetic storms. We study a sequence of events observed in the solar wind, in the magnetotail, at geosynchronous orbit (GEO), in the inner magnetosphere, and in the ionosphere during the main phase of a geomagnetic storm on 16 June 2012–17 June 2012. The storm was caused by a magnetic cloud with a high dynamic pressure and a strong southward IMF lasting about 10 hr. These conditions caused an extreme compression of the magnetosphere (SymH reached ∼150 nT) and an enhancement of the lobe magnetic field strength to ∼90 nT at R ∼ 10 Earth radii (RE). We focus on an hour-long interval between 1050 and 1150 UT on 17 June 2012 when the Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellites were at apogee at geocentric distances R ≈ 12 RE near midnight. At that time a thin current sheet formed between cis-GEO distances and THEMIS. This thin current sheet reconnected between GEO and THEMIS. A strong lobe magnetic field enabled ion and electron energization to energies E ≈ 600 keV. Fluxes of high energy (up to relativistic) particles at GEO increased within ≈20 s after reconnection onset detected by THEMIS. Fluxes of relativistic electrons at L ∼ 4 in the morning sector increased within about 600 s after reconnection onset. We interpret these observations as signatures of direct injection of reconnected particles into the inner magnetosphere.

KW - injections

KW - magnetic storm

KW - magnetosphere

KW - plasma sheet

KW - reconnection

KW - ring current

UR - http://www.scopus.com/inward/record.url?scp=85138991820&partnerID=8YFLogxK

U2 - 10.1029/2022ja030669

DO - 10.1029/2022ja030669

M3 - Article

AN - SCOPUS:85138991820

VL - 127

JO - Journal of Geophysical Research: Space Physics

JF - Journal of Geophysical Research: Space Physics

SN - 2169-9380

IS - 9

M1 - e2022JA030669

ER -

ID: 100066818