Publications of Astronomical Society of India: Recent submissions

  • Muthumariappan, C; Anandarao, B. G; Banerjee, D. P. K (Astronomical Society of India, 1996)
  • Singh, M; Sanwal, B (Astronomical Society of India, 1996)
    Using EG & G spectrograph coupled with reticon array detector and Optical Multichannel Analyser (OMA) at the Cassegrain focus of the 104 cm telescope of the U.P. State Observatory, Naini Tal, several well known bright Be ...
  • Chaubey, U. S (Astronomical Society of India, 1996)
    Spectrum scans of the eclipsing binary star RZ Cas at different phases in the wavelength range λλ 3300 - 7600 Amstrong taken through Hilger and Watts monochromator equipped with 104-cm telescope of Uttar Pradesh State ...
  • Kamath, U. S; Ashok, N. M; Chandrasekhar, T (Astronomical Society of India, 1996)
    JHK photometry of the slow, Fe-II type nova- Nova Aquilae 1995- obtained at the 1.2m Gurushikhar Infrared Telescope (GIRT) is presented here. Evidence for the presence of dust in the nova ejected based on these observations ...
  • Chandra, S (Astronomical Society of India, 1996)
  • Anupama, G. C (Astronomical Society of India, 1996)
    The observational properties of the subclasses of the Cataclysmic Variables; classical and recurrent novae, dwarf novae, intermediate polars and the polars are described here. An interclass connection based on the properties ...
  • Shrivastava, P. K; Shukla, R. P (Astronomical Society of India, 1996)
    Various solar controlled disturbances in interplanetary medium represented by solar flares, coronal holes, solar wind streams, generally produced significant decreases in cosmic ray intensity as well as enhancement in ...
  • Maity, S; Paul, S. N; Bondyopadhaya, R (Astronomical Society of India, 1996)
    The dispersion relation for the MHD waves in a homogeneous medium having differential rotaion has been derived by using spherical polar coordinates. It is found that, for equatorial flow the instability of waves is influenced ...
  • Verma, V. K; Uddin, W; Gaur, V. P; Joshi, G. C; Bondal, K. R; Pant, P (Astronomical Society of India, 1996)
    Monochromatic coronal images during the total solar eclipse of 24 October 1995 were successfully obtained in 6374 Amstrong [Fe X]line. The experiment carried out a Meja Khas, Allahabad during the eclipse and the preliminary ...
  • Goraya, P. S; Rautela, B. S; Sanwal, B. B; Pandey, A. K; Duggal, H. K (Astronomical Society of India, 1996)
    Spectral scans of the head of periodic comet Halley (1982i)covering the wavelength range λλ 320 - 700 nm, are presented for five nights during the months of April an May, 1986. These observations were made when the ...
  • Janardhan, P; Balasubramanian, V; Ananthakrishnan, S; Srivatsan, R (Astronomical Society of India, 1996)
    Extensive IPS observations at 327 MHz using the Ooty Radio Telescope (ORT) are presented. The observations spanning two and a half years starting in September 1992 covered two important periods during the Ulysses south ...
  • Tej, A; Chandrasekhar, T; Ashok, N. M; Ragland, S; Mathur, S. N; Jain, J (Astronomical Society of India, 1996)
    CCD imaging observations of Jupiter were carried out, from the desert location of Jaisalmer in Rajasthan, during the period of its collision with the comet Shoemaker-Levy 9. A Celestron 8 telescope was used with a Lynx PC ...
  • Singh, J (Astronomical Society of India, 1996)
  • Christensen-Dalsgaard, J (Astronomical Society of India, 1996)
    An eminent solar physicist has been quoted as saying that " despite exquisite images we have of the Sun's surface, we know almost nothing about its interior" (Browne 1995). The conference offered an excellent opportunity ...
  • Schou, J; Tomczyk, S; Thompson, M. J (Astronomical Society of India, 1996)
    We present various results from one year of observations with the LOWL instrument, which is designed to observe oscillations with degrees l from 0 to about 100. Among the results shown is an inversion for the solar rotaion ...
  • Satya Narayanan, A (Astronomical Society of India, 1996)
    We consider a simple two layer fluid model to investigate surface waves arising due to the interaction between two fluids of different densities. The interface separates the convection zone and the atmosphere of the Sun. ...
  • Narasimha, D (Astronomical Society of India, 1996)
    The solar p-mode frequencies and eigenfunctions are modified by four processes operative in the atmosphere and the subphotospheric layers which can be, to a good approximation, treated as surface phenomena; they are the ...
  • Martinez, Peter (Astronomical Society of India, 1996)
    This paper discusses the general properties of the p-mode spectra of roAp stars and provides a table of these properties for the 28 currently known roAp stars.
  • Kosovichev, A. G (Astronomical Society of India, 1996)
    The method of 'secondary' helioseismic inversion, in which the equations of state and the thermal balance are used in addition to the hydrostatic equations, have been applied to determine the helium abundance in the Sun's ...
  • Javaraiah, J (Astronomical Society of India, 1996)
    Recently, we studied the rotaion of sunspot gruoups during 1879-1976 and detected ~ 22-yr and a few more other periods 'even' and 'odd' parity torsional oscillations of the Sun (Javaraiah & Gokhale 1995a, b). In the present ...

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