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Found 2 entries in the Bibliography.


Showing entries from 1 through 2


2017

Ionosphere VHF scintillations over Vaddeswaram (Geographic Latitude 16.31° N, Geographic Longitude 80.30° E, Dip 18° N), a latitude Indian station--A case study

This research reports the 250\ MHz amplitude ionosphere scintillations recorded at Vaddeswaram (Geographic Latitude 16.31\textdegreeN, Geographic Longitude 80.30\textdegreeE, Dip 18\textdegreeN), a low-latitude station in India. Though amplitude scintillations were recorded for four continuous days (05\textendash08 November 2011), the presence of intense and long-duration scintillations on 06 November 2011 instigated us to verify the ionosphere background conditions. This research, therefore, is also used important databases including, diurnal variations of h F (virtual height of the F-layer) and the vertical drifts as measured by an advanced digital ionosonde radar located at an Indian equatorial station i.e. Trivandrum (Geographic Latitude 8.5\textdegreeN, Geographic Longitude 77\textdegreeE, Dip 0.5\textdegreeN), equatorial Electrojet (EEJ) ground strength measured using magnetometers and the total electron content (TEC) maps provided by the International GPS Service (IGS) to study the background ionosphere conditions. The interesting observations are higher E\ \texttimes\ B drifts, the occurrence of long-duration range-type spread F signatures at Trivandrum and, thereafter, intense scintillations over Vaddeswaram. It was found a secondary peak at around 1600 LT in EEJ strength followed by a higher upward drift velocity (more than 60\ m/s) with a significant raise of the F region up to 470\ km over the magnetic equator on 06 November 2011. The possible physical mechanisms of these important observational results are discussed in the light of available literature.

Brahmanandam, P.S.; Uma, G.; Pant, T.K.;

Published by: Advances in Space Research      Published on: 10/2017

YEAR: 2017     DOI: 10.1016/j.asr.2017.06.051

2016

F2 region response to geomagnetic disturbances across Indian latitudes: O (1S) dayglow emission

during this storm is also examined by using the GUVI column O/N 2 ratio and is depicted in Figure 9. It is to be mentioned here that GUVI provides a global image, which is gathered

Upadhayaya, AK; Gupta, Sumedha; Brahmanandam, PS;

Published by: Journal of Geophysical Research: Space Physics      Published on:

YEAR: 2016     DOI: 10.1002/2015JA021366



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