Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model
We determine the field-aligned mapping of Saturn's auroras into the magnetosphere by combining UV images of the southern dayside oval obtained by the Hubble Space Telescope (HST) with a global model of the magnetospheric magnetic field. The model is tailored to simulate prevailing condition...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
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Copernicus Publications
2011-07-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/29/1233/2011/angeo-29-1233-2011.pdf |
| _version_ | 1818020974829764608 |
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| author | E. S. Belenkaya S. W. H. Cowley J. D. Nichols M. S. Blokhina V. V. Kalegaev |
| author_facet | E. S. Belenkaya S. W. H. Cowley J. D. Nichols M. S. Blokhina V. V. Kalegaev |
| author_sort | E. S. Belenkaya |
| collection | DOAJ |
| description | We determine the field-aligned mapping of Saturn's
auroras into the magnetosphere by combining UV images of the southern
dayside oval obtained by the Hubble Space Telescope (HST) with a global
model of the magnetospheric magnetic field. The model is tailored to
simulate prevailing conditions in the interplanetary medium, corresponding
to high solar wind dynamic pressure and variable interplanetary magnetic
field (IMF) strength and direction determined from suitably lagged field
data observed just upstream of Saturn's dayside bow shock by the Cassini
spacecraft. Two out of four images obtained in February 2008 when such
simultaneous data are available are examined in detail, exemplifying
conditions for northward and southward IMF. The model field structure in the
outer magnetosphere and tail is found to be very different in these cases.
Nevertheless, the dayside UV oval is found to have a consistent location
relative to the field structure in each case. The poleward boundary of the
oval is located close to the open-closed field boundary and thus maps to the
vicinity of the magnetopause, consistent with previous results. The
equatorward boundary of the oval then maps typically near the outer boundary
of the equatorial ring current appropriate to the compressed conditions
prevailing. Similar results are also found for related images from the
January 2004 HST data set. These new results thus show that the mapped
dayside UV oval typically spans the outer magnetosphere between the outer
part of the ring current and the magnetopause. It does not encompass the
region of primary corotation flow breakdown within the inner Enceladus
torus. |
| first_indexed | 2024-04-14T08:12:47Z |
| format | Article |
| id | doaj.art-5f7b0af2b869494e838301438707c18a |
| institution | Directory Open Access Journal |
| issn | 0992-7689 1432-0576 |
| language | English |
| last_indexed | 2024-04-14T08:12:47Z |
| publishDate | 2011-07-01 |
| publisher | Copernicus Publications |
| record_format | Article |
| series | Annales Geophysicae |
| spelling | doaj.art-5f7b0af2b869494e838301438707c18a2022-12-22T02:04:30ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762011-07-01291233124610.5194/angeo-29-1233-2011Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field modelE. S. Belenkaya0S. W. H. Cowley1J. D. Nichols2M. S. Blokhina3V. V. Kalegaev4Institute of Nuclear Physics, Moscow State University, Vorob'evy Gory, 119992 Moscow, RussiaDepartment of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UKDepartment of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UKInstitute of Nuclear Physics, Moscow State University, Vorob'evy Gory, 119992 Moscow, RussiaInstitute of Nuclear Physics, Moscow State University, Vorob'evy Gory, 119992 Moscow, RussiaWe determine the field-aligned mapping of Saturn's auroras into the magnetosphere by combining UV images of the southern dayside oval obtained by the Hubble Space Telescope (HST) with a global model of the magnetospheric magnetic field. The model is tailored to simulate prevailing conditions in the interplanetary medium, corresponding to high solar wind dynamic pressure and variable interplanetary magnetic field (IMF) strength and direction determined from suitably lagged field data observed just upstream of Saturn's dayside bow shock by the Cassini spacecraft. Two out of four images obtained in February 2008 when such simultaneous data are available are examined in detail, exemplifying conditions for northward and southward IMF. The model field structure in the outer magnetosphere and tail is found to be very different in these cases. Nevertheless, the dayside UV oval is found to have a consistent location relative to the field structure in each case. The poleward boundary of the oval is located close to the open-closed field boundary and thus maps to the vicinity of the magnetopause, consistent with previous results. The equatorward boundary of the oval then maps typically near the outer boundary of the equatorial ring current appropriate to the compressed conditions prevailing. Similar results are also found for related images from the January 2004 HST data set. These new results thus show that the mapped dayside UV oval typically spans the outer magnetosphere between the outer part of the ring current and the magnetopause. It does not encompass the region of primary corotation flow breakdown within the inner Enceladus torus.https://www.ann-geophys.net/29/1233/2011/angeo-29-1233-2011.pdf |
| spellingShingle | E. S. Belenkaya S. W. H. Cowley J. D. Nichols M. S. Blokhina V. V. Kalegaev Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model Annales Geophysicae |
| title | Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model |
| title_full | Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model |
| title_fullStr | Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model |
| title_full_unstemmed | Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model |
| title_short | Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model |
| title_sort | magnetospheric mapping of the dayside uv auroral oval at saturn using simultaneous hst images cassini imf data and a global magnetic field model |
| url | https://www.ann-geophys.net/29/1233/2011/angeo-29-1233-2011.pdf |
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