Excitation of poloidal standing Alfvén waves through drift resonance wave‐particle interaction. Issue 16 (27th August 2013)
- Record Type:
- Journal Article
- Title:
- Excitation of poloidal standing Alfvén waves through drift resonance wave‐particle interaction. Issue 16 (27th August 2013)
- Main Title:
- Excitation of poloidal standing Alfvén waves through drift resonance wave‐particle interaction
- Authors:
- Dai, Lei
Takahashi, Kazue
Wygant, John R.
Chen, Liu
Bonnell, John
Cattell, Cynthia A.
Thaller, Scott
Kletzing, Craig
Smith, Charles W.
MacDowall, Robert J.
Baker, Daniel N.
Blake, J. Bernard
Fennell, Joseph
Claudepierre, Seth
Funsten, Herbert O.
Reeves, Geoffrey D.
Spence, Harlan E. - Abstract:
- <abstract abstract-type="main" id="grl50800-abs-0001"> <title> <x xml:space="preserve">Abstract</x> </title> <p id="grl50800-para-0001">[1] Drift‐resonance wave‐particle interaction is a fundamental collisionless plasma process studied extensively in theory. Using cross‐spectral analysis of electric field, magnetic field, and ion flux data from the Van Allen Probe (Radiation Belt Storm Probes) spacecraft, we present direct evidence identifying the generation of a fundamental mode standing poloidal wave through drift‐resonance interactions in the inner magnetosphere. Intense azimuthal electric field (E<sub><italic>φ</italic></sub>) oscillations as large as 10mV/m are observed, associated with radial magnetic field (B<sub><italic>r</italic></sub>) oscillations in the dawn‐noon sector near but south of the magnetic equator at L∼5. The observed wave period, E<sub><italic>φ</italic></sub>/B<sub><italic>r</italic></sub> ratio and the 90° phase lag between B<sub><italic>r</italic></sub> and E<sub><italic>φ</italic></sub> are all consistent with fundamental mode standing Poloidal waves. Phase shifts between particle fluxes and wave electric fields clearly demonstrate a drift resonance with ∼90 keV ring current ions. The estimated earthward gradient of ion phase space density provides a free energy source for wave generation through the drift‐resonance instability. A similar drift‐resonance process should occur ubiquitously in collisionless plasma systems. One specific example is the<abstract abstract-type="main" id="grl50800-abs-0001"> <title> <x xml:space="preserve">Abstract</x> </title> <p id="grl50800-para-0001">[1] Drift‐resonance wave‐particle interaction is a fundamental collisionless plasma process studied extensively in theory. Using cross‐spectral analysis of electric field, magnetic field, and ion flux data from the Van Allen Probe (Radiation Belt Storm Probes) spacecraft, we present direct evidence identifying the generation of a fundamental mode standing poloidal wave through drift‐resonance interactions in the inner magnetosphere. Intense azimuthal electric field (E<sub><italic>φ</italic></sub>) oscillations as large as 10mV/m are observed, associated with radial magnetic field (B<sub><italic>r</italic></sub>) oscillations in the dawn‐noon sector near but south of the magnetic equator at L∼5. The observed wave period, E<sub><italic>φ</italic></sub>/B<sub><italic>r</italic></sub> ratio and the 90° phase lag between B<sub><italic>r</italic></sub> and E<sub><italic>φ</italic></sub> are all consistent with fundamental mode standing Poloidal waves. Phase shifts between particle fluxes and wave electric fields clearly demonstrate a drift resonance with ∼90 keV ring current ions. The estimated earthward gradient of ion phase space density provides a free energy source for wave generation through the drift‐resonance instability. A similar drift‐resonance process should occur ubiquitously in collisionless plasma systems. One specific example is the "fishbone" instability in fusion plasma devices. In addition, our observations have important implications for the long‐standing mysterious origin of Giant Pulsations.</p> </abstract> … (more)
- Is Part Of:
- Geophysical research letters. Volume 40:Issue 16(2013:Aug.)
- Journal:
- Geophysical research letters
- Issue:
- Volume 40:Issue 16(2013:Aug.)
- Issue Display:
- Volume 40, Issue 16 (2013)
- Year:
- 2013
- Volume:
- 40
- Issue:
- 16
- Issue Sort Value:
- 2013-0040-0016-0000
- Page Start:
- 4127
- Page End:
- 4132
- Publication Date:
- 2013-08-27
- Subjects:
- Geophysics -- Periodicals
Planets -- Periodicals
Lunar geology -- Periodicals
550 - Journal URLs:
- http://www.agu.org/journals/gl/ ↗
http://onlinelibrary.wiley.com/ ↗ - DOI:
- 10.1002/grl.50800 ↗
- Languages:
- English
- ISSNs:
- 0094-8276
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 4156.900000
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