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Movies for "Hybrid simulations of the cusp and dayside magnetosheath dynamics under quasi-radial interplanetary magnetic fields"

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2022Embargo end date: 03 Feb 2022Publisher:Zenodo
Authors: J. Ng; L.-J. Chen; Y. Omelchenko; Y. Zou; B. Lavraud;

doi: 10.5281/zenodo.6574908 , 10.5281/zenodo.5889582 , 10.5281/zenodo.5889583 , 10.5281/zenodo.6986351

Movies for "Hybrid simulations of the cusp and dayside magnetosheath dynamics under quasi-radial interplanetary magnetic fields"

Abstract

rho0_nw and rho0_sw show the time evolution of the density in the northward and southward IMF simulations used in the article submitted to JGR. A 175x250x250 subset of the simulation domain is shown, and the inner boundary is represented by the grey hemisphere. bz_sw_nw shows the evolution of Bz GSM in the GSM y = 0 plane. panels_sw_jet2 shows the evolution of the density and dynamic pressure in the quasi-radial southward IMF simulation.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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