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Geostationary magnetic field signatures of erosion : Wind-goes observations. / Mühlbachler, S.; Farrugia, C. J.; Biernat, H. K.; Torbert, R. B.; Semenov, V. S.

в: European Space Agency, (Special Publication) ESA SP, № 477, 01.03.2002, стр. 459-462.

Результаты исследований: Научные публикации в периодических изданиях › статья в журнале по материалам конференции › Рецензирование

Harvard

Mühlbachler, S, Farrugia, CJ, Biernat, HK, Torbert, RB & Semenov, VS 2002, 'Geostationary magnetic field signatures of erosion: Wind-goes observations', European Space Agency, (Special Publication) ESA SP, № 477, стр. 459-462.

APA

Mühlbachler, S., Farrugia, C. J., Biernat, H. K., Torbert, R. B., & Semenov, V. S. (2002). Geostationary magnetic field signatures of erosion: Wind-goes observations. European Space Agency, (Special Publication) ESA SP, (477), 459-462.

Vancouver

Mühlbachler S, Farrugia CJ, Biernat HK, Torbert RB, Semenov VS. Geostationary magnetic field signatures of erosion: Wind-goes observations. European Space Agency, (Special Publication) ESA SP. 2002 Март 1;(477):459-462.

Author

Mühlbachler, S. ; Farrugia, C. J. ; Biernat, H. K. ; Torbert, R. B. ; Semenov, V. S. / Geostationary magnetic field signatures of erosion : Wind-goes observations. в: European Space Agency, (Special Publication) ESA SP. 2002 ; № 477. стр. 459-462.

BibTeX

@article{e0a237dc0cf04eb1a5fff6d71dca8c6a,
title = "Geostationary magnetic field signatures of erosion: Wind-goes observations",
abstract = "We present an experimental study of erosion of the dayside magnetosphere, utilizing solar wind measurements from the Wind spacecraft and magnetic field measurements from the Goes spacecraft when located between 11.00-13.00 MLT. We focus on three case studies encompassing 3 levels of solar wind dynamic pressure and 3 levels of moderate, negative IMF Bz. In all cases the variation of Bz and dynamic pressure do not exceed 1 nT and 1 nPa, respectively. The AL index is analyzed to confirm that the day-side observations refer to the substorm growth phase. Particular attention is thus paid to the timing of sub-storms to infer the delay times for onset signatures to reach the dayside.",
author = "S. M{\"u}hlbachler and Farrugia, {C. J.} and Biernat, {H. K.} and Torbert, {R. B.} and Semenov, {V. S.}",
year = "2002",
month = mar,
day = "1",
language = "English",
pages = "459--462",
journal = "European Space Agency, (Special Publication) ESA SP",
issn = "0379-6566",
publisher = "ESA Publication Division",
number = "477",
note = "2nd Solar Cycle and Space Weather Conference ; Conference date: 24-09-2001 Through 29-09-2001",

}

RIS

TY - JOUR

T1 - Geostationary magnetic field signatures of erosion

T2 - 2nd Solar Cycle and Space Weather Conference

AU - Mühlbachler, S.

AU - Farrugia, C. J.

AU - Biernat, H. K.

AU - Torbert, R. B.

AU - Semenov, V. S.

PY - 2002/3/1

Y1 - 2002/3/1

N2 - We present an experimental study of erosion of the dayside magnetosphere, utilizing solar wind measurements from the Wind spacecraft and magnetic field measurements from the Goes spacecraft when located between 11.00-13.00 MLT. We focus on three case studies encompassing 3 levels of solar wind dynamic pressure and 3 levels of moderate, negative IMF Bz. In all cases the variation of Bz and dynamic pressure do not exceed 1 nT and 1 nPa, respectively. The AL index is analyzed to confirm that the day-side observations refer to the substorm growth phase. Particular attention is thus paid to the timing of sub-storms to infer the delay times for onset signatures to reach the dayside.

AB - We present an experimental study of erosion of the dayside magnetosphere, utilizing solar wind measurements from the Wind spacecraft and magnetic field measurements from the Goes spacecraft when located between 11.00-13.00 MLT. We focus on three case studies encompassing 3 levels of solar wind dynamic pressure and 3 levels of moderate, negative IMF Bz. In all cases the variation of Bz and dynamic pressure do not exceed 1 nT and 1 nPa, respectively. The AL index is analyzed to confirm that the day-side observations refer to the substorm growth phase. Particular attention is thus paid to the timing of sub-storms to infer the delay times for onset signatures to reach the dayside.

UR - http://www.scopus.com/inward/record.url?scp=0036506543&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:0036506543

SP - 459

EP - 462

JO - European Space Agency, (Special Publication) ESA SP

JF - European Space Agency, (Special Publication) ESA SP

SN - 0379-6566

IS - 477

Y2 - 24 September 2001 through 29 September 2001

ER -

ID: 53085313