DIAMAGNETIC PLASMOIDS AS PART OF DIAMAGNETIC STRUCTURES OF THE SLOW SOLAR WIND AND THEIR IMPACT ON EARTH’S MAGNETOSPHERE-Reference-Cited by-同舟云学术

DIAMAGNETIC PLASMOIDS AS PART OF DIAMAGNETIC STRUCTURES OF THE SLOW SOLAR WIND AND THEIR IMPACT ON EARTH’S MAGNETOSPHERE

Published:2019-12-17 Issue:4 Volume:5 Page:34-45
ISSN:2500-0535
Container-title:Solar-Terrestrial Physics
language:en
Short-container-title:

Author:

Parhomov Vladimir¹,Eselevich Viktor²,Eselevich Maxim²,Dmitriev Aleksey³,Vedernikova Tatyana¹

Affiliation:

1. Baikal State University

2. Institute of Solar Terrestrial Physics SB RAS

3. Skobeltsyn Institute of Nuclear Physics, Moscow State University

Abstract

We have shown that diamagnetic structures (DSs), which form the basis of the slow quasi-stationary solar wind (SW), are observed in Earth’s orbit as a sequence of DSs of various scales. The analysis of this phenomenon indicates that diamagnetic plasmoids in SW, whose concept was introduced by Karlsson in 2015, are identical to small-scale DSs. We have found that the impact of a sequence of DSs in the slow SW on Earth’s magnetosphere causes an increase in geomagnetic activity. Isolated DSs generate short-term magnetic disturbances whose duration is approximately equal to the DS duration. Hence, a sequence of DSs can cause sawtooth substorms. We emphasize that the interaction of DS in the slow SW under northward interplanetary magnetic field can be associated with penetration of DS high-density plasma into the magnetosphere.

Publisher

Infra-M Academic Publishing House

Subject

Space and Planetary Science,Atmospheric Science,Geophysics

Reference30 articles.

1. Borrini G., Wilcox J.M., Gosling J.T., Bame S.J., Feldman W.C. Solar wind helium and hydrogen structure near the helio-spheric current sheet; a signal of coronal streamer at 1 AU. J. Geophys. Res. 1981, vol. 86, p. 4565., Borrini G., Wilcox J.M., Gosling J.T., Bame S.J., Feldman W.C. Solar wind helium and hydrogen structure near the helio-spheric current sheet; a signal of coronal streamer at 1 AU. J. Geophys. Res. 1981, vol. 86, p. 4565.

2. Bostick, W.H. Experimental study of ionized matter projected across a magnetic field. Phys. Rev. 1956, vol. 104, pp. 292–299., Bostick, W.H. Experimental study of ionized matter projected across a magnetic field. Phys. Rev. 1956, vol. 104, pp. 292–299.

3. Eselevich M.V., Eselevich V.G. Fractal structure of the heliospheric plasma sheet in the Earth’s orbit. Geomagnetism and Aeronomy. 2005, vol. 45, no. 3, pp. 326–336., Eselevich M.V., Eselevich V.G. Fractal structure of the heliospheric plasma sheet in the Earth’s orbit. Geomagnetism and Aeronomy. 2005, vol. 45, no. 3, pp. 326–336.

4. Eselevich, M.V., Eselevich V.G. Manifestations of the ray structure of the coronal streamer belt in the form of sharp peaks of the solar wind plasma density in the Earth’s orbit. Geomagnetism and Aeronomy. 2006, vol. 46, iss. 6, pp. 770–782., Eselevich, M.V., Eselevich V.G. Manifestations of the ray structure of the coronal streamer belt in the form of sharp peaks of the solar wind plasma density in the Earth’s orbit. Geomagnetism and Aeronomy. 2006, vol. 46, iss. 6, pp. 770–782.

5. Eselevich V.G., Fainshtein V.G. The heliospheric current sheet (HCS) and high-speed solar wind: interaction effects. Planetary Space Sci. 1991. V. 39. P. 737–744., Eselevich V.G., Fainshtein V.G. The heliospheric current sheet (HCS) and high-speed solar wind: interaction effects. Planetary Space Sci. 1991. V. 39. P. 737–744.

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