Hari Vats - Academia.edu (original) (raw)
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Observatoire Midi-Pyrénées, Université de Toulouse III Paul Sabatier
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Papers by Hari Vats
New Astronomy, Jul 1, 2023
arXiv (Cornell University), May 27, 2021
Communications in Asteroseismology, 2009
Bulletin of the Astronomical Society of India, Dec 1, 1991
Solar-Terrestrial Physics, 1984
Bulletin of the Astronomical Society of India, Jun 1, 2000
Bulletin of the Astronomical Society of India, Sep 1, 1993
Bulletin of the Astronomical Society of India, Jun 1, 1994
Bull. Astr. Soc. India (1994) 22, 165-175 A report on PRL's interplanetary scintillation (IP... more Bull. Astr. Soc. India (1994) 22, 165-175 A report on PRL's interplanetary scintillation (IPS) radio telescopes Han Om Vats and MR Deshpande Physical Research Laboratory, Ahmedabad 380 009 Received 1993 May 18; accepted 1993 June 3 Abstract. Physical Research ...
Indian Journal of Radio and Space Physics, Aug 1, 1996
Bulletin of the Astronomical Society of India, Mar 1, 1981
Antennas and Propagation, 1989. ICAP 89., Sixth International Conference on (Conf. Publ. No.301), Apr 4, 1989
Radio Science, May 1, 1981
Using amplitude data of radio beacons at 40, 140, and 360 MHz from ATS 6 (phase II), an attempt h... more Using amplitude data of radio beacons at 40, 140, and 360 MHz from ATS 6 (phase II), an attempt has been made to study scattering of these waves in the equatorial ionosphere. A comparison of observed scintillation index S 4 with the theoretical results of the multiple scattering approach and variation of autocorrelation time with the frequency indicates that this theory explains the results to a large extent. A comparison of power spectra of amplitude records with the ionograms of a nearby equatorial station has led to the following conclusions: The change from a weak scattering regime to a strong scattering regime is gradual and occurs because of the gradual decrease in the scale size of the irregularities (i.e., broadening of the spectra) and the gradual increase in the thickness of the irregular region.
New Astronomy, Jul 1, 2023
arXiv (Cornell University), May 27, 2021
Communications in Asteroseismology, 2009
Bulletin of the Astronomical Society of India, Dec 1, 1991
Solar-Terrestrial Physics, 1984
Bulletin of the Astronomical Society of India, Jun 1, 2000
Bulletin of the Astronomical Society of India, Sep 1, 1993
Bulletin of the Astronomical Society of India, Jun 1, 1994
Bull. Astr. Soc. India (1994) 22, 165-175 A report on PRL's interplanetary scintillation (IP... more Bull. Astr. Soc. India (1994) 22, 165-175 A report on PRL's interplanetary scintillation (IPS) radio telescopes Han Om Vats and MR Deshpande Physical Research Laboratory, Ahmedabad 380 009 Received 1993 May 18; accepted 1993 June 3 Abstract. Physical Research ...
Indian Journal of Radio and Space Physics, Aug 1, 1996
Bulletin of the Astronomical Society of India, Mar 1, 1981
Antennas and Propagation, 1989. ICAP 89., Sixth International Conference on (Conf. Publ. No.301), Apr 4, 1989
Radio Science, May 1, 1981
Using amplitude data of radio beacons at 40, 140, and 360 MHz from ATS 6 (phase II), an attempt h... more Using amplitude data of radio beacons at 40, 140, and 360 MHz from ATS 6 (phase II), an attempt has been made to study scattering of these waves in the equatorial ionosphere. A comparison of observed scintillation index S 4 with the theoretical results of the multiple scattering approach and variation of autocorrelation time with the frequency indicates that this theory explains the results to a large extent. A comparison of power spectra of amplitude records with the ionograms of a nearby equatorial station has led to the following conclusions: The change from a weak scattering regime to a strong scattering regime is gradual and occurs because of the gradual decrease in the scale size of the irregularities (i.e., broadening of the spectra) and the gradual increase in the thickness of the irregular region.