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Can the Fe-snow regime explain a present-day dynamo in Ganymede's core?

Rückriemen, Tina and Breuer, D. and Spohn, T. (2015) Can the Fe-snow regime explain a present-day dynamo in Ganymede's core? 26th General Assembly of the International Union of Geodesy and Geophysics, 22. Juni - 2. Juli 2015, Prag, Tschechische Republik.

Full text not available from this repository.


Item URL in elib:https://elib.dlr.de/101632/
Document Type:Conference or Workshop Item (Speech)
Title:Can the Fe-snow regime explain a present-day dynamo in Ganymede's core?
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Rückriemen, Tinatina.rueckriemen (at) dlr.deUNSPECIFIED
Breuer, D.doris.breuer (at) dlr.deUNSPECIFIED
Spohn, T.tilman.spohn (at) dlr.deUNSPECIFIED
Date:2015
Refereed publication:No
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:Ganyemde, core crystallization, iron snow regime, magnetic field
Event Title:26th General Assembly of the International Union of Geodesy and Geophysics
Event Location:Prag, Tschechische Republik
Event Type:international Conference
Event Dates:22. Juni - 2. Juli 2015
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Science and Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Erforschung des Weltraums
DLR - Research theme (Project):R - Vorhaben Exploration des Sonnensystems
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research
Institute of Planetary Research > Leitungsbereich PF
Institute of Planetary Research > Planetary Physics
Deposited By: Rückriemen, Tina
Deposited On:06 Jan 2016 10:32
Last Modified:01 Dec 2018 19:51

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