The determination of ionospheric plasma drifts by a rocket-borne electrostatic flux meter

1974 ◽  
Vol 22 (7) ◽  
pp. 1131-1138 ◽  
Author(s):  
K. Gueth ◽  
H.V. Hoerner ◽  
G. Brommundt
1971 ◽  
Vol 19 (3) ◽  
pp. 345-355 ◽  
Author(s):  
K. Knott ◽  
G. Brommundt ◽  
G. Schumann

2004 ◽  
Vol 10 (2-3) ◽  
pp. 36-44 ◽  
Author(s):  
A.S. Mazmanishvili ◽  
◽  
V.A. Puliaiev ◽  
E.V. Rogozkin ◽  
◽  
...  

BIBECHANA ◽  
2016 ◽  
Vol 14 ◽  
pp. 1-8 ◽  
Author(s):  
Narayan P Chapagain

This study presents the experimental results of the equatorial ionospheric plasma drift zonal velocity obtained from Incoherent Scatter Radar (ISR) observations for 6 selective days in 2011 from Jicamarca, Peru. Our results indicate that the daytime drifts are westward with peak values mostly below ~50 m/s, while the night time drifts velocities are eastward, with a maximum value up to 120 m/s at around local midnight hours. The drift velocity decreases during post-midnight hours and starts to reverse westward in early morning hours. Our plasma drifts results are in good agreement with results from previous radar studies and other measurement techniques.  BIBECHANA 14 (2017)1-8  


2016 ◽  
Vol 121 (8) ◽  
pp. 7961-7973 ◽  
Author(s):  
Chao‐Song Huang ◽  
Gordon R. Wilson ◽  
Marc R. Hairston ◽  
Yongliang Zhang ◽  
Wenbin Wang ◽  
...  

2004 ◽  
Vol 22 (9) ◽  
pp. 3099-3107 ◽  
Author(s):  
T. J. Immel ◽  
H. U. Frey ◽  
S. B. Mende ◽  
E. Sagawa

Abstract. Space-based measurements from an imager aboard the high-apogee NASA-IMAGE satellite allows for global-scale observations of nightside ionospheric densities and structure. Such a view cannot be provided by imagers in near-Earth orbit or based on the ground. The IMAGE Spectroscopic Imager (SI) isolates the Far-ultraviolet (FUV) O I 135.6nm emission which is produced through radiative recombination of O+. These observations clearly show the distribution of FUV emissions of the equatorial airglow bands over the range of local times between the evening terminator to points well after midnight. Determination of plasma drift speeds in these local time sectors is performed by identification and subsequent tracking of localized depressions in the FUV emissions. This determination is made for nearly 200 plasma bubbles in the March-May period of 2002. Important findings of this study include (1) an unambiguous association between Dst and zonal plasma drift speeds, and (2) a longitudinal dependence of the zonal plasma drift speeds, with a peak around the Indian sector. The first effect is attributed to penetrating ring current electric fields, while the second is apparently due to a longitudinal variability in the vertical polarization electric fields that directly affects the zonal plasma drift speeds.


Sign in / Sign up

Export Citation Format

Share Document