uu.seUppsala University Publications
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Cassini nightside observations of the oscillatory motion of Saturn's northern auroral oval
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Swedish Institute of Space Physics, Uppsala Division.
Show others and affiliations
2014 (English)In: Journal of Geophysical Research - Space Physics, ISSN 2169-9380, Vol. 119, no 5, 3528-3543 p.Article in journal (Refereed) Published
Abstract [en]

In recent years we have benefitted greatly from the first in-orbit multi-wavelength images of Saturn's polar atmosphere from the Cassini spacecraft. Specifically, images obtained from the Cassini UltraViolet Imaging Spectrograph (UVIS) provide an excellent view of the planet's auroral emissions, which in turn give an account of the large-scale magnetosphere-ionosphere coupling and dynamics within the system. However, obtaining near-simultaneous views of the auroral regions with in situ measurements of magnetic field and plasma populations at high latitudes is more difficult to routinely achieve. Here we present an unusual case, during Revolution 99 in January 2009, where UVIS observes the entire northern UV auroral oval during a 2h interval while Cassini traverses the magnetic flux tubes connecting to the auroral regions near 21 LT, sampling the related magnetic field, particle, and radio and plasma wave signatures. The motion of the auroral oval evident from the UVIS images requires a careful interpretation of the associated latitudinally oscillating magnetic field and auroral field-aligned current signatures, whereas previous interpretations have assumed a static current system. Concurrent observations of the auroral hiss (typically generated in regions of downward directed field-aligned current) support this revised interpretation of an oscillating current system. The nature of the motion of the auroral oval evident in the UVIS image sequence, and the simultaneous measured motion of the field-aligned currents (and related plasma boundary) in this interval, is shown to be related to the northern hemisphere magnetosphere oscillation phase. This is in agreement with previous observations of the auroral oval oscillatory motion.

Place, publisher, year, edition, pages
2014. Vol. 119, no 5, 3528-3543 p.
Keyword [en]
Saturn, aurora, field-aligned currrents, auroral hiss
National Category
Fusion, Plasma and Space Physics
Identifiers
URN: urn:nbn:se:uu:diva-228812DOI: 10.1002/2013JA019527ISI: 000337622100024OAI: oai:DiVA.org:uu-228812DiVA: diva2:735067
Available from: 2014-07-22 Created: 2014-07-22 Last updated: 2014-07-22Bibliographically approved

Open Access in DiVA

fulltext(4071 kB)133 downloads
File information
File name FULLTEXT01.pdfFile size 4071 kBChecksum SHA-512
5badf816315b01c1eb2f1bec6ff02b2cda0c068896a38218117fa239dcc6bbd76dfda735be00f4c32ac7e9ac55b9f74983dc1ad75c19f454f95f677850188f24
Type fulltextMimetype application/pdf

Other links

Publisher's full text

Authority records BETA

Andrews, David J.

Search in DiVA

By author/editor
Andrews, David J.
By organisation
Swedish Institute of Space Physics, Uppsala Division
Fusion, Plasma and Space Physics

Search outside of DiVA

GoogleGoogle Scholar
Total: 133 downloads
The number of downloads is the sum of all downloads of full texts. It may include eg previous versions that are now no longer available

doi
urn-nbn

Altmetric score

doi
urn-nbn
Total: 417 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf