SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:uu-228812"
 

Search: onr:"swepub:oai:DiVA.org:uu-228812" > Cassini nightside o...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Cassini nightside observations of the oscillatory motion of Saturn's northern auroral oval

Bunce, E. J. (author)
Grodent, D. C. (author)
Jinks, S. L. (author)
show more...
Andrews, David J. (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Badman, S. V. (author)
Coates, A. J. (author)
Cowley, S. W. H. (author)
Dougherty, M. K. (author)
Kurth, W. S. (author)
Mitchell, D. G. (author)
Provan, G. (author)
show less...
 (creator_code:org_t)
2014
2014
English.
In: Journal of Geophysical Research - Space Physics. - 2169-9380. ; 119:5, s. 3528-3543
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • 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.

Subject headings

NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Keyword

Saturn
aurora
field-aligned currrents
auroral hiss

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view