Old tail lobes effect on the solar-wind – Magnetosphere energy transport for the 27 August 2001 substorm
The magnetic flux of tail lobes Ψ is divided in two parts of comparable values Ψ1 and Ψ02, with the first that appears during substorm and the second, observed before substorm start. The first was named “new magnetic flux”, the second – “old magnetic flux”. The first, Ψ1, is known to play a definiti...
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| Veröffentlicht in: | Advances in space research 2014-12, Vol.54 (12), p.2540-2548 |
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| container_title | Advances in space research |
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| creator | Mishin, V.V. Mishin, V.M. Pu, Z. Lunyushkin, S.B. Sapronova, L.A. Sukhbaatar, U. Baishev, D.G. |
| description | The magnetic flux of tail lobes Ψ is divided in two parts of comparable values Ψ1 and Ψ02, with the first that appears during substorm and the second, observed before substorm start. The first was named “new magnetic flux”, the second – “old magnetic flux”. The first, Ψ1, is known to play a definitive role in the energy transport from the solar wind into the magnetosphere-ionosphere-atmosphere system, but the role of Ψ02 in this transport is not well known. From the 27 August 2001 substorm data we study the involvement in the above transport process of the old flux Ψ02. This involvement is observed in the polar cap (PC) area, which existed prior to the substorm and is called respectively “the old PC”. In this study, as distinct from earlier works, we use the balance equation of the energy stored in magnetosphere and energy consumed. Activation of the old PC magnetic flux Ψ02 was found to increase the energy input by ∼85% in the event under consideration. |
| doi_str_mv | 10.1016/j.asr.2014.09.013 |
| format | Article |
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| ispartof | Advances in space research, 2014-12, Vol.54 (12), p.2540-2548 |
| issn | 0273-1177 1879-1948 |
| language | eng |
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| source | Elsevier ScienceDirect Journals |
| subjects | Energy consumption Energy flux Energy use Lobes Magnetic flux Magnetospheres Magnetospheric convection Mathematical analysis Polar cap Polycarbonates Solar wind Tail lobes Transport |
| title | Old tail lobes effect on the solar-wind – Magnetosphere energy transport for the 27 August 2001 substorm |
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