Abstract
Optical methods have enabled to detect auroral emissions during daytime conditions, and to identify a narrow latitudinal region of energetic particle precipitation from the Indian station Maitri (11 deg38`E; 70deg45`S; 62.8degS I-lat.) in Antarctica. These observations are new. The energetic particles originate within the closed geomagnetic field lines close to the plasmapause region and maximize {approx} 0830 h MLT (magnetic local time) ({approx}1200 UT). Enhanced proton precipitation activity could also be inferred during a moderate geomagnetic storm, suggesting the enhancement/activation of acceleration mechanisms during this event. (author). 11 refs., 2 figs.
Sridharan, R;
Pallam Raju, D;
Narayanan, R;
Modi, N K;
Subbaraya, B H;
Raghavarao, R
[1]
- Physical Research Lab., Ahmedabad (India)
Citation Formats
Sridharan, R, Pallam Raju, D, Narayanan, R, Modi, N K, Subbaraya, B H, and Raghavarao, R.
Daytime measurements of optical auroral emissions from Antarctica.
India: N. p.,
1995.
Web.
Sridharan, R, Pallam Raju, D, Narayanan, R, Modi, N K, Subbaraya, B H, & Raghavarao, R.
Daytime measurements of optical auroral emissions from Antarctica.
India.
Sridharan, R, Pallam Raju, D, Narayanan, R, Modi, N K, Subbaraya, B H, and Raghavarao, R.
1995.
"Daytime measurements of optical auroral emissions from Antarctica."
India.
@misc{etde_101577,
title = {Daytime measurements of optical auroral emissions from Antarctica}
author = {Sridharan, R, Pallam Raju, D, Narayanan, R, Modi, N K, Subbaraya, B H, and Raghavarao, R}
abstractNote = {Optical methods have enabled to detect auroral emissions during daytime conditions, and to identify a narrow latitudinal region of energetic particle precipitation from the Indian station Maitri (11 deg38`E; 70deg45`S; 62.8degS I-lat.) in Antarctica. These observations are new. The energetic particles originate within the closed geomagnetic field lines close to the plasmapause region and maximize {approx} 0830 h MLT (magnetic local time) ({approx}1200 UT). Enhanced proton precipitation activity could also be inferred during a moderate geomagnetic storm, suggesting the enhancement/activation of acceleration mechanisms during this event. (author). 11 refs., 2 figs.}
journal = []
issue = {8}
volume = {68}
journal type = {AC}
place = {India}
year = {1995}
month = {Apr}
}
title = {Daytime measurements of optical auroral emissions from Antarctica}
author = {Sridharan, R, Pallam Raju, D, Narayanan, R, Modi, N K, Subbaraya, B H, and Raghavarao, R}
abstractNote = {Optical methods have enabled to detect auroral emissions during daytime conditions, and to identify a narrow latitudinal region of energetic particle precipitation from the Indian station Maitri (11 deg38`E; 70deg45`S; 62.8degS I-lat.) in Antarctica. These observations are new. The energetic particles originate within the closed geomagnetic field lines close to the plasmapause region and maximize {approx} 0830 h MLT (magnetic local time) ({approx}1200 UT). Enhanced proton precipitation activity could also be inferred during a moderate geomagnetic storm, suggesting the enhancement/activation of acceleration mechanisms during this event. (author). 11 refs., 2 figs.}
journal = []
issue = {8}
volume = {68}
journal type = {AC}
place = {India}
year = {1995}
month = {Apr}
}