Zobrazeno 1 - 10
of 11
pro vyhledávání: '"G. D. Vyas"'
Publikováno v:
Proceedings of Indian National Science Academy, Vol 47, Iss 1A (2015)
Ionospheric Effects of the Total Solar Eclipse of 16 February 1980
Publikováno v:
Radio Science. 30:475-478
Here we present the study of daytime scintillation due to E region irregularities at low latitudes from a set of simultaneous observations on June 3, 1993. The effects of these irregularities are clearly seen on (1) the 103 MHz signal of the radio st
Publikováno v:
Astrophysics and Space Science. 218:249-265
This article describes in detail a burst from PSR 0950+08 on July 29, 1992. This event was observed by two radio telescopes (separated by ~ 200 km) operating at 103 MHz. There exists a very convincing indirect evidence that at the same time the pulsa
Publikováno v:
ChemInform. 32
Publikováno v:
Indian journal of experimental biology. 36(12)
Several [2-phenyl-4(3H)-oxo-3-quinazolinylamino]-N-substituted- arylacetamides (1a-j) have been synthesized and tested at the National Cancer Institute, Bethesda, Maryland, USA, for their anti-HIV activity against susceptible human host cells (CEM ce
Publikováno v:
International Astronomical Union Colloquium. 160:477-478
Interplanetary Scintillation (IPS) is a diffraction phenomenon in which coherent electro-magnetic radiation, from a distant radio source, passes through the solar wind, which is a turbulent refracting medium, and suffers scattering. This results in r
Publikováno v:
Journal of Earth System Science. 95:83-89
Ionospheric drift records obtained by the closely spaced receiver technique at Udaipur are subjected to low and high pass filtering with varying cutoff frequencies and the effects of filtering on various drift and anisotropy parameters as determined
Publikováno v:
Journal of Earth System Science. 87:215-224
Daily variations of the E-W and N-S components of ionospheric drifts, measured using closely spaced receiver method over Tiruchirapalli near magnetic equator, are described for the periods 1973–75 forE region and 1974–75 forF region. N-S componen
Autor:
R G Rastogi, G D Vyas
Publikováno v:
Proceedings of the Indian Academy of Sciences - Section A. 86:417-421
The mean occurrence of frequency type of spreadF at Huancayo has been shown to have practically no solar cycle dependence. The occurrence of range type of spreadF is shown to be inversely related to sunspot number. The range spread occurs mostly arou
Publikováno v:
Proceedings / Indian Academy of Sciences. 87:109-113
Geomagnetic disturbance effects on the occurrence of range and frequency spread at Huancayo are studied for the period 1957–74. The occurrence of frequency spread is decreased on disturbed days forD-months andE-months while duringJ-months an increa