SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:uu-517519"
 

Search: onr:"swepub:oai:DiVA.org:uu-517519" > Statistical Mapping...

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

Statistical Mapping of Magnetic Topology at Venus

Xu, Shaosui (author)
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
Frahm, Rudy A. (author)
Southwest Res Inst, San Antonio, TX USA.
Ma, Yingjuan (author)
Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA USA.
show more...
Luhmann, Janet G. (author)
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
Mitchell, David L. (author)
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
Persson, Moa (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
show less...
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA Southwest Res Inst, San Antonio, TX USA. (creator_code:org_t)
American Geophysical Union (AGU), 2023
2023
English.
In: Journal of Geophysical Research - Space Physics. - : American Geophysical Union (AGU). - 2169-9380 .- 2169-9402. ; 128:12
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Despite Venus having insignificant intrinsic magnetic fields, the magnetic connectivity between the solar wind and the Venus ionosphere, or magnetic topology, is not as simple as expected and is also important for characterizing the Venus space environment. This study provides a technique combining superthermal electron energy and pitch angle distributions to infer up to 6 subtypes of magnetic topology at Venus. This enables us to determine magnetic topology with automated procedures using the Venus Express (VEx) observations from May 2006 to November 2014. We find that the draped topology (both ends of a field line not connected to the collisional ionosphere) is the dominant topology in the near-Venus space environment, >70%, except at low altitudes close to the ionosphere. The open (a field line connected to both the solar wind and the collisional ionosphere) and closed (a field line connected only to the collisional ionosphere) topologies make up 20%-30% on average of the magnetotail and up to 50% at low altitudes. This study provides the first characterization of the statistical distributions of different magnetic topologies at Venus.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Den kondenserade materiens fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Condensed Matter Physics (hsv//eng)
NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Geofysik (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Geophysics (hsv//eng)

Keyword

Venus
induced magnetosphere
magnetic topology
solar wind interaction
superthermal electrons
Venus Express

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

Search outside SwePub

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