Measurement of Individual H+ and O+ Ion Temperatures in the Topside Ionosphere. Issue 2 (14th February 2018)
- Record Type:
- Journal Article
- Title:
- Measurement of Individual H+ and O+ Ion Temperatures in the Topside Ionosphere. Issue 2 (14th February 2018)
- Main Title:
- Measurement of Individual H+ and O+ Ion Temperatures in the Topside Ionosphere
- Authors:
- Hsu, Chih‐Te
Heelis, Roderick A. - Abstract:
- Abstract: Plasma temperatures in the ionosphere are associated with both the dynamics and spatial distribution of the neutral and charge particles. During the daytime, temperatures are determined by solar energy inputs and energy exchange between charged and neutral particles. Plasma transport parallel to the magnetic field adds another influence on temperatures through adiabatic processes that are most evident during the nighttime. Previous observations suggest that the topside H + temperature ( T H+ ) should reside between the O + temperature ( T O+ ) and the electron temperature ( T e ), and further calculations confirm the preferential heat transfer from the electrons to H + in the topside. In this work we implement a more sophisticated analysis procedure to extract individual mass‐dependent ion temperatures from the retarding potential analyzer measurements on the DMSP F15 satellite. The results show that the daytime T H+ is a few hundred degrees higher than T O+ at all longitudes. The nighttime temperature difference between T H+ and T O+ is indicative of mass‐dependent adiabatic heating and cooling processes across the equatorial region. The ion temperatures and measured plasma flows present clear longitudinal variations that are associated with magnetic declination. Key Points: A more sophisticated analysis procedure to extract O + and H + temperatures ( T O+ and T H+ ) from RPA was implemented When electrons are heated during daytime, T O+ < T H+ When O + isAbstract: Plasma temperatures in the ionosphere are associated with both the dynamics and spatial distribution of the neutral and charge particles. During the daytime, temperatures are determined by solar energy inputs and energy exchange between charged and neutral particles. Plasma transport parallel to the magnetic field adds another influence on temperatures through adiabatic processes that are most evident during the nighttime. Previous observations suggest that the topside H + temperature ( T H+ ) should reside between the O + temperature ( T O+ ) and the electron temperature ( T e ), and further calculations confirm the preferential heat transfer from the electrons to H + in the topside. In this work we implement a more sophisticated analysis procedure to extract individual mass‐dependent ion temperatures from the retarding potential analyzer measurements on the DMSP F15 satellite. The results show that the daytime T H+ is a few hundred degrees higher than T O+ at all longitudes. The nighttime temperature difference between T H+ and T O+ is indicative of mass‐dependent adiabatic heating and cooling processes across the equatorial region. The ion temperatures and measured plasma flows present clear longitudinal variations that are associated with magnetic declination. Key Points: A more sophisticated analysis procedure to extract O + and H + temperatures ( T O+ and T H+ ) from RPA was implemented When electrons are heated during daytime, T O+ < T H+ When O + is adiabatically heated at night, T O+ > T H+ … (more)
- Is Part Of:
- Journal of geophysical research. Volume 123:Issue 2(2018)
- Journal:
- Journal of geophysical research
- Issue:
- Volume 123:Issue 2(2018)
- Issue Display:
- Volume 123, Issue 2 (2018)
- Year:
- 2018
- Volume:
- 123
- Issue:
- 2
- Issue Sort Value:
- 2018-0123-0002-0000
- Page Start:
- 1525
- Page End:
- 1533
- Publication Date:
- 2018-02-14
- Subjects:
- retarding potential analyzer -- topside ionosphere energy budget -- H+ temperature -- interhemispheric transports
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:
- 10.1002/2017JA024932 ↗
- Languages:
- English
- ISSNs:
- 2169-9380
- Deposit Type:
- Legaldeposit
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- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 4995.010000
British Library DSC - BLDSS-3PM
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