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Low-frequency oscil...
Low-frequency oscillatory flow signatures and high-speed flows in the Earth's magnetotail
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- De Spiegeleer, Alexandre (author)
- Umeå universitet,Institutionen för fysik
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- Hamrin, Maria (author)
- Umeå universitet,Institutionen för fysik
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- Pitkänen, Timo (author)
- Umeå universitet,Institutionen för fysik
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Volwerk, M. (author)
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- Mann, Ingrid (author)
- Umeå universitet,Institutionen för fysik,Department of Physics and Technology, The Arctic University of Norway, Tromsø, Norway
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Nilsson, H. (author)
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- Norqvist, Patrik (author)
- Umeå universitet,Institutionen för fysik
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Andersson, L. (author)
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- Vaverka, Jakub (author)
- Umeå universitet,Institutionen för fysik
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(creator_code:org_t)
- Washington : American Geophysical Union (AGU), 2017
- 2017
- English.
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In: Journal of Geophysical Research - Space Physics. - Washington : American Geophysical Union (AGU). - 2169-9380 .- 2169-9402. ; 122:7, s. 7042-7056
- Related links:
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https://urn.kb.se/re...
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https://doi.org/10.1...
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Abstract
Subject headings
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- 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)
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