Ionospheric Plasma Flows Associated with the Formation of the Distorted Nightside End of A Transpolar Arc-Reference-Cited by-同舟云学术

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Ionospheric Plasma Flows Associated with the Formation of the Distorted Nightside End of A Transpolar Arc

Published:2022-03-31 Issue: Volume: Page:
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Author:

Nowada Motoharu¹^ORCID,Grocott Adrian²^ORCID,Shi Quanqi¹^ORCID

Affiliation:

1. Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University, Weihai, Shandong, People’s Republic of China.

2. Space and Planetary Physics Group, Department of Physics, Lancaster University, Lancaster, UK.

Funder

National Natural Science Foundation of China

Science and Technology Facilities Council

Natural Environment Research Council

Publisher

Wiley

Reference12 articles.

1. Carter J. A. Milan S. E. Fear R. C. Kullen A. and Hairston M. R.: Dayside reconnection under interplanetary magnetic

2. field By-dominated conditions: The formation and movement of bending arcs J. Geophys. Res. : Space Physics 120 2967-

3. 2978 doi:10.1002/2014JA020809 2015.

4. Cowley, S. W. H.: Magnetospheric asymmetries associated with the y-component of the IMF;Chisham G.;Planet. Space Sci.,2007

5. Cowley, S. W. H. and Lockwood, M.: Excitation and decay of solar wind-driven flows in the magnetosphere-ionosphere system;Ann. Geophysicae,1981

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