Journal article
Magnetic signatures of plasma‐depleted flux tubes in the Saturnian inner magnetosphere
Geophysical research letters, Vol.34(14), pp.L14108-n/a
07/21/2007
DOI: 10.1029/2007GL030374
Abstract
Initial Cassini observations have revealed evidence for interchanging magnetic flux tubes in the inner Saturnian magnetosphere. Some of the reported flux tubes differ remarkably by their magnetic signatures, having a depressed or enhanced magnetic pressure relative to their surroundings. The ones with stronger fields have been interpreted previously as either outward moving mass‐loaded or inward moving plasma‐depleted flux tubes based on magnetometer observations only. We use detailed multi‐instrumental observations of small and large density depletions in the inner Saturnian magnetosphere from Cassini Rev. A orbit that enable us to discriminate amongst the two previous and opposite interpretations. Our analysis undoubtedly confirms the similar nature of both types of reported interchanging magnetic flux tubes, which are plasma‐depleted, whatever their magnetic signatures are. Their different magnetic signature is clearly an effect associated with latitude. These Saturnian plasma‐depleted flux tubes ultimately may play a similar role as the Jovian ones.
Details
- Title: Subtitle
- Magnetic signatures of plasma‐depleted flux tubes in the Saturnian inner magnetosphere
- Creators
- N. André - University College LondonA. M. Persoon - University of IowaJ. Goldstein - Southwest Research InstituteJ. L. Burch - Southwest Research InstituteP. Louarn - Centre d'Etude Spatiales des RayonnementsG. R. Lewis - University College LondonA. M. Rymer - Johns Hopkins University Applied Physics LaboratoryA. J. Coates - University College LondonW. S. Kurth - University of IowaE. C. Sittler - Goddard Space Flight CenterM. F. Thomsen - Los Alamos National LaboratoryF. J. Crary - Southwest Research InstituteM. K. Dougherty - Imperial CollegeD. A. Gurnett - University of IowaD. T. Young - Southwest Research Institute
- Resource Type
- Journal article
- Publication Details
- Geophysical research letters, Vol.34(14), pp.L14108-n/a
- DOI
- 10.1029/2007GL030374
- ISSN
- 0094-8276
- eISSN
- 1944-8007
- Number of pages
- 7
- Language
- English
- Date published
- 07/21/2007
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984455657802771
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