WFRF:(Orton G. S.)
Sökning: WFRF:(Orton G. S.) > Jupiter's Aurora Ob...
LIBRIS Formathandbok (Information om MARC21)
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 05235naa a2200613 4500 | |
| 001 | oai:DiVA.org:kth-232275 | |
| 003 | SwePub | |
| 008 | 180719s2018 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2322752 URI |
| 024 | 7 | a https://doi.org/10.1002/2017JA0250462 DOI |
| 040 | a (SwePub)kth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Grodent, Denisu Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium.4 aut |
| 245 | 1 0 | a Jupiter's Aurora Observed With HST During Juno Orbits 3 to 7 |
| 264 | 1 | b AMER GEOPHYSICAL UNION,c 2018 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20180719 | |
| 520 | a A large set of observations of Jupiter's ultraviolet aurora was collected with the Hubble Space Telescope concurrently with the NASA-Juno mission, during an eight-month period, from 30 November 2016 to 18 July 2017. These Hubble observations cover Juno orbits 3 to 7 during which Juno in situ and remote sensing instruments, as well as other observatories, obtained a wealth of unprecedented information on Jupiter's magnetosphere and the connection with its auroral ionosphere. Jupiter's ultraviolet aurora is known to vary rapidly, with timescales ranging from seconds to one Jovian rotation. The main objective of the present study is to provide a simplified description of the global ultraviolet auroral morphology that can be used for comparison with other quantities, such as those obtained with Juno. This represents an entirely new approach from which logical connections between different morphologies may be inferred. For that purpose, we define three auroral subregions in which we evaluate the auroral emitted power as a function of time. In parallel, we define six auroral morphology families that allow us to quantify the variations of the spatial distribution of the auroral emission. These variations are associated with changes in the state of the Jovian magnetosphere, possibly influenced by Io and the Io plasma torus and by the conditions prevailing in the upstream interplanetary medium. This study shows that the auroral morphology evolved differently during the five similar to 2week periods bracketing the times of Juno perijove (PJ03 to PJ07), suggesting that during these periods, the Jovian magnetosphere adopted various states. | |
| 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 Jupiter | |
| 653 | a aurora | |
| 653 | a Hubble | |
| 653 | a Juno | |
| 653 | a magnetosphere | |
| 700 | 1 | a Bonfond, B.u Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium.4 aut |
| 700 | 1 | a Yao, Z.u Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium.4 aut |
| 700 | 1 | a Gerard, J-C4 aut |
| 700 | 1 | a Radioti, A.u Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium.4 aut |
| 700 | 1 | a Dumont, M.u Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium.4 aut |
| 700 | 1 | a Palmaerts, B.u Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium.4 aut |
| 700 | 1 | a Adriani, A.u INAF, Ist Astrofis & Planetol Spaziali, Rome, Italy.4 aut |
| 700 | 1 | a Badman, S. V.u Univ Lancaster, Phys Dept, Lancaster, England.4 aut |
| 700 | 1 | a Bunce, E. J.u Univ Leicester, Dept Phys & Astron, Leicester, Leics, England.4 aut |
| 700 | 1 | a Clarke, J. T.u Boston Univ, Ctr Space Phys, Boston, MA 02215 USA.4 aut |
| 700 | 1 | a Connerney, J. E. P.u NASA, Goddard Space Flight Ctr, Planetary Magnetospheres Lab, Solar Syst Explorat Div, Greenbelt, MD USA.4 aut |
| 700 | 1 | a Gladstone, G. R.u Southwest Res Inst, Dept Space Sci, San Antonio, TX USA.4 aut |
| 700 | 1 | a Greathouse, T.u Southwest Res Inst, Dept Space Sci, San Antonio, TX USA.4 aut |
| 700 | 1 | a Kimura, T.u RIKEN, Wako, Saitama, Japan.4 aut |
| 700 | 1 | a Kurth, W. S.u Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA.4 aut |
| 700 | 1 | a Mauk, B. H.u Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA.4 aut |
| 700 | 1 | a McComas, D. J.u Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA.4 aut |
| 700 | 1 | a Nichols, J. D.u Univ Leicester, Dept Phys & Astron, Leicester, Leics, England.4 aut |
| 700 | 1 | a Orton, G. S.u CALTECH, Jet Prop Lab, Pasadena, CA USA.4 aut |
| 700 | 1 | a Roth, Lorenzu KTH,Rymd- och plasmafysik4 aut0 (Swepub:kth)u1ml3zu9 |
| 700 | 1 | a Saur, J.u Univ Cologne, Inst Geophys & Meteorol, Cologne, Germany.4 aut |
| 700 | 1 | a Valek, P.u Southwest Res Inst, Dept Space Sci, San Antonio, TX USA.;Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX USA.4 aut |
| 710 | 2 | a Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium.b INAF, Ist Astrofis & Planetol Spaziali, Rome, Italy.4 org |
| 773 | 0 | t Journal of Geophysical Research - Space Physicsd : AMER GEOPHYSICAL UNIONg 123:5, s. 3299-3319q 123:5<3299-3319x 2169-9380x 2169-9402 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-232275 |
| 856 | 4 8 | u https://doi.org/10.1002/2017JA025046 |
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