SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:umu-139015"
 

Search: onr:"swepub:oai:DiVA.org:umu-139015" > Low-frequency oscil...

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

Low-frequency oscillatory flow signatures and high-speed flows in the Earth's magnetotail

De Spiegeleer, Alexandre (author)
Umeå universitet,Institutionen för fysik
Hamrin, Maria (author)
Umeå universitet,Institutionen för fysik
Pitkänen, Timo (author)
Umeå universitet,Institutionen för fysik
show more...
Volwerk, M. (author)
Mann, Ingrid (author)
Umeå universitet,Institutionen för fysik,Department of Physics and Technology, The Arctic University of Norway, Tromsø, Norway
Nilsson, H. (author)
Norqvist, Patrik (author)
Umeå universitet,Institutionen för fysik
Andersson, L. (author)
Vaverka, Jakub (author)
Umeå universitet,Institutionen för fysik
show less...
 (creator_code:org_t)
Washington : American Geophysical Union (AGU), 2017
2017
English.
In: Journal of Geophysical Research - Space Physics. - Washington : American Geophysical Union (AGU). - 2169-9380 .- 2169-9402. ; 122:7, s. 7042-7056
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Using plasma sheet data from Cluster 1 spacecraft from 2001 till 2011, we statistically investigate oscillatory signatures in the plasma bulk flow. These periodic oscillations are compared to high-speed and quiet flows. Periodic oscillations are observed approximately 8% of the time, while high-speed flows and quiet flows are observed around 0.5% and 12% of the time, respectively. We remark that periodic oscillations can roughly occur everywhere for x(gsm) < -10 R-E and |y(gsm)| < 10 RE, while quiet flows mainly occur toward the flanks of this region and toward x = -10 R-E. The relation between the geomagnetic and solar activity and the occurrence of periodic oscillations is investigated and reveal that periodic oscillations occur for most Kp values and solar activity, while quiet flows are more common during low magnetospheric and solar activity. We find that the median oscillation frequency of periodic oscillations is 1.7 mHz and the median duration of the oscillation events is 41 min. We also observe that their associated Poynting vectors show a tendency to be earthward (S-x >= 0). Finally, the distribution of high-speed flows and periodic oscillations as a function of the velocity is investigated and reveals that thresholds lower than 200 km/s should not be used to identify high-speed flows as it could result in misinterpreting a periodic oscillations for a high-speed flow.

Subject headings

TEKNIK OCH TEKNOLOGIER  -- Maskinteknik -- Strömningsmekanik och akustik (hsv//swe)
ENGINEERING AND TECHNOLOGY  -- Mechanical Engineering -- Fluid Mechanics and Acoustics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Subatomär fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Subatomic Physics (hsv//eng)

Keyword

bursty bulk flows
plasma sheet
cluster observations
magnetic field
neutral sheet
magnetosphere
dependence
midtail

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