Articles | Volume 36, issue 4
Regular paper
08 Aug 2018
Regular paper |  | 08 Aug 2018

Cavitons and spontaneous hot flow anomalies in a hybrid-Vlasov global magnetospheric simulation

Xochitl Blanco-Cano, Markus Battarbee, Lucile Turc, Andrew P. Dimmock, Emilia K. J. Kilpua, Sanni Hoilijoki, Urs Ganse, David G. Sibeck, Paul A. Cassak, Robert C. Fear, Riku Jarvinen, Liisa Juusola, Yann Pfau-Kempf, Rami Vainio, and Minna Palmroth


Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to revisions (further review by editor and referees) (30 May 2018) by Christopher Owen
AR by Markus Battarbee on behalf of the Authors (29 Jun 2018)  Author's response   Manuscript 
ED: Publish as is (03 Jul 2018) by Christopher Owen
AR by Markus Battarbee on behalf of the Authors (09 Jul 2018)  Manuscript 
Short summary
We use the Vlasiator code to study the characteristics of transient structures that exist in the Earth's foreshock, i.e. upstream of the bow shock. The structures are cavitons and spontaneous hot flow anomalies (SHFAs). These transients can interact with the bow shock. We study the changes the shock suffers via this interaction. We also investigate ion distributions associated with the cavitons and SHFAs. A very important result is that the arrival of multiple SHFAs results in shock erosion.