Investigation of the temperature gradient instability as the source of midlatitude quiet time decameter‐scale ionospheric irregularities: 1. Observations. Issue 6 (9th June 2014)
- Record Type:
- Journal Article
- Title:
- Investigation of the temperature gradient instability as the source of midlatitude quiet time decameter‐scale ionospheric irregularities: 1. Observations. Issue 6 (9th June 2014)
- Main Title:
- Investigation of the temperature gradient instability as the source of midlatitude quiet time decameter‐scale ionospheric irregularities: 1. Observations
- Authors:
- de Larquier, S.
Eltrass, A.
Mahmoudian, A.
Ruohoniemi, J. M.
Baker, J. B. H.
Scales, W. A.
Erickson, P. J.
Greenwald, R. A. - Abstract:
- <abstract abstract-type="main" id="jgra51032-abs-0001"> <title>Abstract</title> <p>Super Dual Auroral Radar Network (SuperDARN) radars regularly observe decameter‐scale ionospheric irregularities at midlatitudes during quiet geomagnetic conditions. The mechanism responsible for the growth of such irregularities is still unknown. Previous results based on data from the Wallops SuperDARN HF radar and Incoherent Scatter Radar have suggested that the Temperature Gradient Instability (TGI) could be responsible for only part of the observed irregularities. This conclusion was reached based on the relative orientation of horizontal electron temperature and density gradients. However, the TGI theory requires driving gradients to be perpendicular to perpendicular to the geomagnetic field <bold>B</bold>. Since midlatitude field lines are approximately 20° off vertical, we have reexamined the original data and computed gradients along the meridional direction perpendicular to <bold>B</bold>. Distinctions have to be made between the topside and bottomside <italic>F</italic> region due to the strong influence of vertical gradients. We find that the TGI growth is possible in the topside <italic>F</italic> region for the duration of the experiment, even before irregularities were observed. We show that the absence of observed irregularities during favorable TGI growth conditions is not a consequence of HF propagation but of higher <italic>E</italic> region electron irregularity growth. We<abstract abstract-type="main" id="jgra51032-abs-0001"> <title>Abstract</title> <p>Super Dual Auroral Radar Network (SuperDARN) radars regularly observe decameter‐scale ionospheric irregularities at midlatitudes during quiet geomagnetic conditions. The mechanism responsible for the growth of such irregularities is still unknown. Previous results based on data from the Wallops SuperDARN HF radar and Incoherent Scatter Radar have suggested that the Temperature Gradient Instability (TGI) could be responsible for only part of the observed irregularities. This conclusion was reached based on the relative orientation of horizontal electron temperature and density gradients. However, the TGI theory requires driving gradients to be perpendicular to perpendicular to the geomagnetic field <bold>B</bold>. Since midlatitude field lines are approximately 20° off vertical, we have reexamined the original data and computed gradients along the meridional direction perpendicular to <bold>B</bold>. Distinctions have to be made between the topside and bottomside <italic>F</italic> region due to the strong influence of vertical gradients. We find that the TGI growth is possible in the topside <italic>F</italic> region for the duration of the experiment, even before irregularities were observed. We show that the absence of observed irregularities during favorable TGI growth conditions is not a consequence of HF propagation but of higher <italic>E</italic> region electron irregularity growth. We conclude that the TGI is a valid mechanism to explain the generation of all irregularities observed during the experiment.</p> </abstract> … (more)
- Is Part Of:
- Journal of geophysical research. Volume 119:Issue 6(2014:Jun.)
- Journal:
- Journal of geophysical research
- Issue:
- Volume 119:Issue 6(2014:Jun.)
- Issue Display:
- Volume 119, Issue 6 (2014)
- Year:
- 2014
- Volume:
- 119
- Issue:
- 6
- Issue Sort Value:
- 2014-0119-0006-0000
- Page Start:
- 4872
- Page End:
- 4881
- Publication Date:
- 2014-06-09
- 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:
- 10.1002/2013JA019643 ↗
- 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:
- 3828.xml