Observations of magnetospheric high‐m poloidal waves by ST‐5 satellites in low Earth orbit during geomagnetically quiet times. Issue 6 (24th June 2015)
- Record Type:
- Journal Article
- Title:
- Observations of magnetospheric high‐m poloidal waves by ST‐5 satellites in low Earth orbit during geomagnetically quiet times. Issue 6 (24th June 2015)
- Main Title:
- Observations of magnetospheric high‐m poloidal waves by ST‐5 satellites in low Earth orbit during geomagnetically quiet times
- Authors:
- Chi, P. J.
Le, G. - Abstract:
- <abstract abstract-type="main" id="jgra51866-abs-0001"> <title>Abstract</title> <p id="jgra51866-para-0001">The poloidal waves with large azimuthal wave numbers (<italic>m</italic>) in the magnetosphere are known to be generated by drift or drift‐bounce resonance with energetic ring current particles, and these waves may play a role in modulating the energetic particles in the inner magnetosphere. When examining the magnetic field data collected by the NASA Space Technology 5 (ST‐5) satellites in the low Earth orbit, Le et al. (2011) discovered many wave events with frequencies of 30–200 mHz (in the Pc2 and Pc3 bands), and they proposed that these waves should, in fact, be Doppler‐shifted high‐<italic>m</italic> poloidal waves in the magnetosphere with frequencies at only a few millihertz (in the Pc5 band). Using a new method that examines the differences in wave phase detected by the three ST‐5 satellites, we confirm that the frequencies in the Earth frame for the poloidal waves observed are mainly between 3 and 5 mHz. Not only were poloidal waves observed frequently by ST‐5 in the dayside magnetosphere but they were also occasionally seen in the nightside when the satellites passed through the same <italic>L</italic> shells. In each wave event, the azimuthal wave number may change with <italic>L</italic>, but the wave frequency in the Earth frame remains the same. We also find that poloidal waves can last more than 9 h during geomagnetically quiet conditions, suggesting<abstract abstract-type="main" id="jgra51866-abs-0001"> <title>Abstract</title> <p id="jgra51866-para-0001">The poloidal waves with large azimuthal wave numbers (<italic>m</italic>) in the magnetosphere are known to be generated by drift or drift‐bounce resonance with energetic ring current particles, and these waves may play a role in modulating the energetic particles in the inner magnetosphere. When examining the magnetic field data collected by the NASA Space Technology 5 (ST‐5) satellites in the low Earth orbit, Le et al. (2011) discovered many wave events with frequencies of 30–200 mHz (in the Pc2 and Pc3 bands), and they proposed that these waves should, in fact, be Doppler‐shifted high‐<italic>m</italic> poloidal waves in the magnetosphere with frequencies at only a few millihertz (in the Pc5 band). Using a new method that examines the differences in wave phase detected by the three ST‐5 satellites, we confirm that the frequencies in the Earth frame for the poloidal waves observed are mainly between 3 and 5 mHz. Not only were poloidal waves observed frequently by ST‐5 in the dayside magnetosphere but they were also occasionally seen in the nightside when the satellites passed through the same <italic>L</italic> shells. In each wave event, the azimuthal wave number may change with <italic>L</italic>, but the wave frequency in the Earth frame remains the same. We also find that poloidal waves can last more than 9 h during geomagnetically quiet conditions, suggesting that even a very weak ring current can supply enough energetic particles to excite poloidal waves.</p> </abstract> … (more)
- Is Part Of:
- Journal of geophysical research. Volume 120:Issue 6(2015:Jun.)
- Journal:
- Journal of geophysical research
- Issue:
- Volume 120:Issue 6(2015:Jun.)
- Issue Display:
- Volume 120, Issue 6 (2015)
- Year:
- 2015
- Volume:
- 120
- Issue:
- 6
- Issue Sort Value:
- 2015-0120-0006-0000
- Page Start:
- 4776
- Page End:
- 4783
- Publication Date:
- 2015-06-24
- Subjects:
- Magnetospheric physics -- Periodicals
Space environment -- Periodicals
Cosmic physics -- Periodicals
Planets -- Atmospheres -- Periodicals
Heliosphere (Astrophysics) -- Periodicals
Geophysics -- Periodicals
523.01 - Journal URLs:
- http://onlinelibrary.wiley.com/journal/10.1002/(ISSN)2169-9402 ↗
http://onlinelibrary.wiley.com/ ↗ - DOI:
- 10.1002/2015JA021145 ↗
- Languages:
- English
- ISSNs:
- 2169-9380
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 4995.010000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 3908.xml