publication . Article . 2017


Giagkiozis, S.; Walker, S.N.; Pope, S.A.; Collinson, G.;
Open Access
  • Published: 01 Aug 2017 Journal: Journal of Geophysical Research: Space Physics, volume 122, pages 8,632-8,641 (issn: 2169-9380, Copyright policy)
  • Publisher: American Geophysical Union (AGU)
  • Country: United Kingdom
The velocity of a collisionless shock (CS) is an important parameter in the determination of the spatial scales of the shock. The spatial scales of the shock determine the processes that guide the energy dissipation, which is related to the nature of the shock. During the pre-ISEE era, estimations of relative shock-spacecraft velocity (VSh) were based on spatial scales of the shock front regions, in particularly the foot. Multispacecraft missions allow more reliable identification of VSh. The main objective of this study is to examine the accuracy of two single spacecraft methods, which use the foot region of quasi-perpendicular shocks in order determine VSh. Th...
arXiv: Astrophysics::High Energy Astrophysical PhenomenaPhysics::Space PhysicsAstrophysics::Galaxy Astrophysics
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