Van Allen Probes Bibliography is from August 2012 through September 2021 Notice:
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Found 3 entries in the Bibliography.
Showing entries from 1 through 3
2019 |
Empirical Modeling of the Geomagnetosphere for SIR and CME-Driven Magnetic Storms During geomagnetic disturbances, the solar wind arrives in the form of characteristic sequences lasting from tens of hours to days. The most important magnetic storm drivers are the coronal mass ejections (CMEs) and the slow-fast stream interaction regions (SIRs). Previous data-based magnetic field models did not distinguish between these types of the solar wind driving. In the present work we retained the basic structure of the Tsyganenko and Andreeva (2015) model but fitted it to data samples corresponding to (1) SIR-drive ... Published by: Journal of Geophysical Research: Space Physics Published on: 07/2019 YEAR: 2019   DOI: 10.1029/2018JA026008 Magnetic Storms; Magnetosphere; Modeling; Solar wind; spacecraft data; Van Allen Probes |
2017 |
Empirical modeling of the quiet and storm-time geosynchronous magnetic field A dynamical empirical model of the near-geosynchronous magnetic field has been constructed, based on a recently developed RBF approach and a multi-year set of spacecraft data taken by THEMIS, Polar, Cluster, and Van Allen Probes missions including 133 geomagnetic storms in the time interval between 1996 and 2016. The model describes the field as a function of Cartesian solar-magnetic coordinates, dipole tilt angle, solar wind ram pressure, and of a set of dynamic variables representing the response of the magnetosphere to th ... Published by: Space Weather Published on: 12/2017 YEAR: 2017   DOI: 10.1002/2017SW001684 geomagnetic field; geostationary orbit; Modeling; spacecraft data; Van Allen Probes |
2016 |
Reconstructing the magnetosphere from data using radial basis functions A new method is proposed to derive from data magnetospheric magnetic field configurations without any a priori assumptions on the geometry of electric currents. The approach utilizes large sets of archived satellite data and uses an advanced technique to represent the field as a sum of toroidal and poloidal parts, whose generating potentials Ψ1 and Ψ2 are expanded into series of radial basis functions (RBF) with their nodes regularly distributed over the 3D modeling domain. The method was tested by reconstructing the inner ... Andreeva, Varvara; Tsyganenko, Nikolai; Published by: Journal of Geophysical Research: Space Physics Published on: 02/2016 YEAR: 2016   DOI: 10.1002/2015JA022242 current systems; magnetospheric modeling; polar cusps; Van Allen Probes |
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