ORCID Profile
0000-0002-5859-1136
Current Organisations
International Space Science Institute
,
University College London
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Publisher: The Royal Society
Date: 29-05-2017
Publisher: Elsevier BV
Date: 05-2012
Publisher: American Geophysical Union (AGU)
Date: 2004
DOI: 10.1029/2004JA010614
Publisher: Elsevier BV
Date: 12-2014
Publisher: Springer Science and Business Media LLC
Date: 05-08-2008
Publisher: Elsevier BV
Date: 10-2020
Publisher: American Geophysical Union (AGU)
Date: 11-2008
DOI: 10.1029/2008JA013592
Publisher: Springer Science and Business Media LLC
Date: 13-05-2008
Publisher: Elsevier BV
Date: 08-2011
Publisher: American Geophysical Union (AGU)
Date: 19-10-2006
DOI: 10.1029/2006JA011676
Publisher: American Association for the Advancement of Science (AAAS)
Date: 13-05-2005
Abstract: The magnetic field signature obtained by Cassini during its first close encounter with Titan on 26 October 2004 is presented and explained in terms of an advanced model. Titan was inside the saturnian magnetosphere. A magnetic field minimum before closest approach marked Cassini's entry into the magnetic ionopause layer. Cassini then left the northern and entered the southern magnetic tail lobe. The magnetic field before and after the encounter was approximately constant for ∼20 Titan radii, but the field orientation changed exactly at the location of Titan's orbit. No evidence of an internal magnetic field at Titan was detected.
Publisher: Springer Science and Business Media LLC
Date: 10-09-2011
Location: United Kingdom of Great Britain and Northern Ireland
Location: United Kingdom of Great Britain and Northern Ireland
No related grants have been discovered for Geraint H. Jones.