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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 02869naa a2200409 4500 | |
| 001 | oai:DiVA.org:umu-107178 | |
| 003 | SwePub | |
| 008 | 150819s2015 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-1071782 URI |
| 024 | 7 | a https://doi.org/10.1002/2015JA0212122 DOI |
| 040 | a (SwePub)umu | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Lindkvist, Jesperu Umeå universitet,Institutionen för fysik,Swedish Institute of Space Physics, Kiruna4 aut0 (Swepub:umu)jeli0142 |
| 245 | 1 0 | a Callisto plasma interactions :b Hybrid modeling including induction by a subsurface ocean |
| 264 | 1 | c 2015 |
| 338 | a electronic2 rdacarrier | |
| 520 | a By using a hybrid plasma solver (ions as particles and electrons as a fluid), we have modeled the interaction between Callisto and Jupiter's magnetosphere for variable ambient plasma parameters. We compared the results with the magnetometer data from flybys (C3, C9, and C10) by the Galileo spacecraft. Modeling the interaction between Callisto and Jupiter's magnetosphere is important to establish the origin of the magnetic field perturbations observed by Galileo and thought to be related to a subsurface ocean. Using typical upstream magnetospheric plasma parameters and a magnetic dipole corresponding to the inductive response inside the moon, we show that the model results agree well with observations for the C3 and C9 flybys, but agrees poorly with the C10 flyby close to Callisto. The study does support the existence of a subsurface ocean at Callisto. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng |
| 653 | a Callisto | |
| 653 | a plasma interaction | |
| 653 | a hybrid model | |
| 653 | a subsurface ocean | |
| 653 | a Galileo flyby | |
| 653 | a magnetosphere | |
| 700 | 1 | a Holmström, Matsu Swedish Institute of Space Physics, Kiruna4 aut0 (Swepub:umu)maho0050 |
| 700 | 1 | a Khurana, Krishan K.u Department of Earth and Space Sciences, University of California, Los Angeles4 aut |
| 700 | 1 | a Fatemi, Shahabu Space Sciences Laboratory, University of California, Berkeley4 aut |
| 700 | 1 | a Barabash, Stasu Swedish Institute of Space Physics, Kiruna4 aut0 (Swepub:umu)stba0032 |
| 710 | 2 | a Umeå universitetb Institutionen för fysik4 org |
| 773 | 0 | t Journal of Geophysical Research - Space Physicsg 120:6, s. 4877-4889q 120:6<4877-4889x 2169-9380x 2169-9402 |
| 856 | 4 | u https://umu.diva-portal.org/smash/get/diva2:850430/FULLTEXT02.pdfx primaryx Raw objecty fulltext:print |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-107178 |
| 856 | 4 8 | u https://doi.org/10.1002/2015JA021212 |
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