Magnetodisc modelling in Jupiter's magnetosphere using Juno magnetic field data and the paraboloid magnetic field model
<p>One of the main features of Jupiter's magnetosphere is its equatorial magnetodisc, which significantly increases the field strength and size of the magnetosphere. Analysis of Juno measurements of the magnetic field during the first 10 orbits covering the dawn to pre-dawn sector of the...
Main Authors: | I. A. Pensionerov, E. S. Belenkaya, S. W. H. Cowley, I. I. Alexeev, V. V. Kalegaev, D. A. Parunakian |
---|---|
Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2019-02-01
|
Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/37/101/2019/angeo-37-101-2019.pdf |
Similar Items
-
Optimization of Saturn paraboloid magnetospheric field model parameters
using Cassini equatorial magnetic field data
by: E. S. Belenkaya, et al.
Published: (2016-07-01) -
Open and partially closed models of the solar wind interaction with outer planet magnetospheres: the case of Saturn
by: E. S. Belenkaya, et al.
Published: (2017-12-01) -
Magnetospheric magnetic field modelling for the 2011 and 2012 HST Saturn aurora campaigns – implications for auroral source regions
by: E. S. Belenkaya, et al.
Published: (2014-06-01) -
Analysis of Eddy Current Generation on the Juno Spacecraft in Jupiter's Magnetosphere
by: S. Kotsiaros, et al.
Published: (2020-07-01) -
Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model
by: E. S. Belenkaya, et al.
Published: (2011-07-01)