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The Location of Magnetic Reconnection at Earth's Magnetopause
DOI: 10.1007/s11214-021-00817-8 Bibcode: 2021SSRv..217...41T

Fuselier, S. A.; Trattner, K. J.; Petrinec, S. M.

One of the major questions about magnetic reconnection is how specific solar wind and interplanetary magnetic field conditions influence where reconnection occurs at the Earth's magnetopause. There are two reconnection scenarios discussed in the literature: a) anti-parallel reconnection and b) component reconnection. Early spacecraft observations …

2021 Space Science Reviews
Cluster DoubleStar 42
Shock Induced Strong Substorms and Super Substorms: Preconditions and Associated Oxygen Ion Dynamics
DOI: 10.1007/s11214-021-00806-x Bibcode: 2021SSRv..217...33Z

Zong, Q. -G.; Fu, S. -Y.; Yue, C.

It is well known that the interaction between interplanetary (IP) shocks and the Earth's magnetosphere would generate/excite various types of geomagnetic phenomena. Progresses have been made on the Earth's magnetospheric response to solar wind forcing in recent years in the aspects associated with magnetospheric substorms. Strong substorms and sup…

2021 Space Science Reviews
Cluster DoubleStar 30
Current Sheets, Plasmoids and Flux Ropes in the Heliosphere. Part II: Theoretical Aspects
DOI: 10.1007/s11214-021-00799-7 Bibcode: 2021SSRv..217...39P

Malova, H. V.; Zelenyi, L. M.; Bruno, R. +13 more

Our understanding of processes occurring in the heliosphere historically began with reduced dimensionality - one-dimensional (1D) and two-dimensional (2D) sketches and models, which aimed to illustrate views on large-scale structures in the solar wind. However, any reduced dimensionality vision of the heliosphere limits the possible interpretation…

2021 Space Science Reviews
Cluster 27