Chorus intensity modulation driven by time‐varying field‐aligned low‐energy plasma. Issue 9 (18th September 2015)
- Record Type:
- Journal Article
- Title:
- Chorus intensity modulation driven by time‐varying field‐aligned low‐energy plasma. Issue 9 (18th September 2015)
- Main Title:
- Chorus intensity modulation driven by time‐varying field‐aligned low‐energy plasma
- Authors:
- Nishimura, Y.
Bortnik, J.
Li, W.
Liang, J.
Thorne, R. M.
Angelopoulos, V.
Le Contel, O.
Auster, U.
Bonnell, J. W. - Abstract:
- <abstract abstract-type="main" id="jgra52060-abs-0001"> <title>Abstract</title> <p id="jgra52060-para-0001">Recent studies have shown that chorus waves are responsible for scattering and precipitating the energetic electrons that drive the pulsating aurora. While some of the chorus intensity modulation events are correlated with &lt;~100 eV electron density modulation, most of the chorus intensity modulation events in the postmidnight sector occur without apparent density changes. Although it is generally difficult to measure evolution of low‐energy (&lt;~20 eV) electron fluxes due to constraints imposed by the spacecraft potential and electrostatic analyzer (ESA) energy range limit, we identified using Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellite data that low‐energy ions of ~100 eV show density modulation that is correlated with chorus intensity modulation. Those low‐energy ions and electrons are field‐aligned with major peaks in 0° (for northern hemisphere winter event) and 180° (for northern hemisphere summer event) pitch angle, indicating that outflowing plasma from the sunlit hemisphere is the source of the low‐energy plasma density modulation near the equator. Plasma sheet plasma density, and ambient electric and magnetic fields do not show modulations that are correlated with the chorus intensity modulation. Assuming charge neutrality, the low‐energy ions can be used to represent cold plasma density in wave growth rate<abstract abstract-type="main" id="jgra52060-abs-0001"> <title>Abstract</title> <p id="jgra52060-para-0001">Recent studies have shown that chorus waves are responsible for scattering and precipitating the energetic electrons that drive the pulsating aurora. While some of the chorus intensity modulation events are correlated with &lt;~100 eV electron density modulation, most of the chorus intensity modulation events in the postmidnight sector occur without apparent density changes. Although it is generally difficult to measure evolution of low‐energy (&lt;~20 eV) electron fluxes due to constraints imposed by the spacecraft potential and electrostatic analyzer (ESA) energy range limit, we identified using Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellite data that low‐energy ions of ~100 eV show density modulation that is correlated with chorus intensity modulation. Those low‐energy ions and electrons are field‐aligned with major peaks in 0° (for northern hemisphere winter event) and 180° (for northern hemisphere summer event) pitch angle, indicating that outflowing plasma from the sunlit hemisphere is the source of the low‐energy plasma density modulation near the equator. Plasma sheet plasma density, and ambient electric and magnetic fields do not show modulations that are correlated with the chorus intensity modulation. Assuming charge neutrality, the low‐energy ions can be used to represent cold plasma density in wave growth rate calculations, and the enhancements of the low‐energy plasma density are found to contribute most effectively to chorus linear growth rates. These results suggest that chorus intensity modulation is driven by a feedback process where outflowing plasma due to energetic electron precipitation increases the equatorial density that drives further electron precipitation.</p> </abstract> … (more)
- Is Part Of:
- Journal of geophysical research. Volume 120:Issue 9(2015:Sep.)
- Journal:
- Journal of geophysical research
- Issue:
- Volume 120:Issue 9(2015:Sep.)
- Issue Display:
- Volume 120, Issue 9 (2015)
- Year:
- 2015
- Volume:
- 120
- Issue:
- 9
- Issue Sort Value:
- 2015-0120-0009-0000
- Page Start:
- 7433
- Page End:
- 7446
- Publication Date:
- 2015-09-18
- 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:
- 10.1002/2015JA021330 ↗
- 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:
- 3835.xml