dc.creatorStepanova, M.
dc.creatorAntonova, E. E.
dc.creatorMoya, P. S.
dc.creatorPinto, V. A.
dc.creatorValdivia, J. A.
dc.date.accessioned2019-10-15T12:25:30Z
dc.date.available2019-10-15T12:25:30Z
dc.date.created2019-10-15T12:25:30Z
dc.date.issued2019
dc.identifierJournal of Geophysical Research: Space Physics, Volumen 124, Issue 2, 2019, Pages 1187-1202
dc.identifier21699402
dc.identifier21699380
dc.identifier10.1029/2018JA025965
dc.identifierhttps://repositorio.uchile.cl/handle/2250/171706
dc.description.abstractUsing data from Defense Meteorological Satellite Program 16–18, National Oceanic and Atmospheric Administration 15–19, and METOP 1–2 satellites, we reconstructed for the first time a two-dimensional statistical distribution of plasma pressure in the inner magnetosphere during the 1 June 2013 geomagnetic storm with time resolution of 6 hr. Simultaneously, we used the data from Van Allen Probes and Time History of Events and Macroscale Interactions missions to obtain the in situ plasma pressure in the equatorial plane. This allowed us to corroborate that the dipole mapping works reasonably well during the storm time and that variations of plasma pressure are consistent at low and high altitudes; namely, we observed a drastic increase in plasma pressure a few hours before the storm onset that continued during the storm main phase. Plasma pressure remained elevated during the first 18 hr of the recovery phase and then started to decre
dc.languageen
dc.publisherBlackwell Publishing Ltd
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
dc.sourceJournal of Geophysical Research: Space Physics
dc.subjectdynamic pressure
dc.subjectgeomagnetic storm
dc.subjectinner magnetosphere
dc.subjectplasma pressure
dc.subjectsolar wind
dc.titleMultisatellite Analysis of Plasma Pressure in the Inner Magnetosphere During the 1 June 2013 Geomagnetic Storm
dc.typeArtículo de revista


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