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M

M. R. Deshpande

Researcher at Physical Research Laboratory

Publications -  34
Citations -  379

M. R. Deshpande is an academic researcher from Physical Research Laboratory. The author has contributed to research in topics: Total electron content & Scintillation. The author has an hindex of 12, co-authored 34 publications receiving 368 citations.

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Equatorial electrojet control of the low latitude ionosphere.

TL;DR: The role of the equatorial electrojet on the distribution of ionization at low latitudes has been discussed using mult-location Total Electron Content (TEC) data obtained through the radio beacon signals from the geostationary satellite ATS-6 and from ground-based ionosonde data as mentioned in this paper.
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Effect of electrojet on the total electron content of the ionosphere over the Indian subcontinent

TL;DR: The radio beacon method of measuring TEC along a chain of optimally spaced stations near the equatorial anomaly has been used to monitor continuously the latitudinal extent of the anomaly as discussed by the authors.
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Polarimetric observations of the comet Hale-Bopp

TL;DR: In this article, the spectrum properties of the coma region of the comet Hale Bopp were analyzed at different phase angles, varying from 17.1 to 47.4 degrees, and the linear polarization measured through 3650, 4845 and 6840 A bands showed stronger wavelength dependence as compared to what is seen in comet Halley at similar phase angles.
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Rotational Modulation of Microwave Solar Flux

TL;DR: In this paper, time series data of 107 cm solar flux for one solar cycle (1985-1995 years) was processed through autocorrelation modulation with varying persistence and period was quite evident.
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Amplitude scintillations of ATS-6 radio beacon signals within the equatorial electrojet region (Ootacamund, dip 4° N)

TL;DR: In this article, the amplitudes of radio beacon signals on 40, 140 and 360 MHz from ATS-6 (at 34° E longitude) recorded at Ootacamund, India (11.43° N, 76.70°E, dip 4°N, elevation angle 41°) have revealed the largest occurrence of scintillations for about 60% of cases around 2200 hr during the nighttime, and two secondary peaks (25%of cases) around 0900 hr and 1400 hours during the daytime.