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Browsing Kodaikanal Observatory, Kodaikanal by Title

Browsing Kodaikanal Observatory, Kodaikanal by Title

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  • Peraiah, A; Srinivasa Rao, M (Indian Institute of Astrophysics, Bangalore, 1985-11)
    We have presented a series of P Cygni type profiles of special lines computed by employing different velocity laws of expansion in a spherically atmosphere. A comparison has been made with those of Beals classification. ...
  • Royal Astronomical Society (Royal Astronomical Society, 1925-01-09)
    This includes the announcement made in the journal Monthly Notices of Royal Astronomical Society regarding his election as a fellow of the Royal Astronomical Society, a letter proposing his name for the membership and ...
  • Evershed, John (Taylor and Francis, 1899-07)
  • Vahia, M. N (Indian Institute of Astrophysics, Bangalore, 1988)
    Recent results on various aspects of solar energetic particles are reviewed. A possible grain component of the polar particles is discussed in brief. The plasma component namely the solar wind and the solar energetic ...
  • Vahia, M. N (Indian Institute of Astrophysics, Bangalore, 1988)
    In this paper we attempt to show that currently available data on solar flare particle abundances allows studies of abundance and enchancement patterns. In particular we show that solar particles originate from regions of ...
  • Ramani, M; Cowsik, R; Singh, J; Shukla, A. K (Wg. Cdr.); Ravi Shekar (Sqn. Ldr.); Narayana, P. V. S (Fg. Offr); Shaji, P. K (Fg. Offr.); Paul, S. K (Fg. Offr.); Shelkey, S. N (J.W.O); Babu, K. R (J.W.O); Kamble, V. B (Indian Institute of Astrophysics, Bangalore, 1997)
    The teams of the Indian Air Force participated actively in the programme. They made several supersonic flights to follow shadow zone of the moon on earth along the path of totality, thereby extending thte duration of ...
  • Kumar, S. S; Sharma, P; Devgun, C. B (Indian Institute of Astrophysics, Bangalore, 1997)
    Twenty pictures of solar corona were taken on October 24, 1995 from Bhind on the central line of totality, covering a wide range of exposure times a 500mm telephoto lens captured Images on 35mm film duly calibrated. This ...
  • Chakraborty, P; Sankarasubramanian, K; Majumder, S; Rajesh Nayak, K; Sridharan, R; Jana, A. D; Rajalakshmi, G; Suresh, D; Asgekar, A; Geetha, K. P; Rajesh, C. K (Indian Institute of Astrophysics, Bangalore, 1997)
    White light images of the solar corona were taken on KODAK 2415 films using 3-inch (f/11.5) telescopes fitted with SLR cameras. Observations were made from 4 different sites spread over the totality belt by four different ...
  • Ananda Rao, B. G; Ashok, N. M; Chandrasekhar, T; Desai, J. N; Nanda Kumar, M. S (Indian Institute of Astrophysics, 1997)
    White light pictures and filter grams in three narrow band interference filters centered on the emission lines In Fe X, Fe XIV and Ca XV have been obtained. We have observed a coronal structure towards the north western ...
  • Mohin, S; Raveendran, A. V; Mekkaden, M. V (Indian Institute of Astrophysics, Bangalore, 1980)
    UBV photometry of Zeta Aurigae during the 1977 and 1979-80 eclipses is presented. From an analysis of the available photometry, it is concluded that the long term intrinsic variation in the brightness of the late-type super ...
  • Joshi, U. C; Sen, A. K; Deshpande, M. R; Jain, Rekha (Indian Institute of Astrophysics, 1988)
    Polarimetric measurements of SN1987A in BVR bands were made on March 6 and 7. These observations along with the polarimetric data reported by various other authors within first 30 days of explosion have been discussed. ...
  • Evershed, John (The Observatory, 1918-12)
  • Uddin, W; Pande, M. C; Verma, V. K (Indian Institute of Astrophysics, Bangalore, 1988)
    In the present investigation we have studied the relation between solar proton flares and associated optical, radio and x-ray events. It is found that optical flares are usually associated with large optical flares in ...
  • Narayan, A. L; Ananthasubrahmanyam, C. K (Calcutta University Press, 1940-10)
    The experimental errors inherent in photographic photometry are discussed and a direct reading spectrophotometer for the visible especially adapted to the study of line, contour and absorption and fluorescence spectra is ...
  • Royds, T (Indian Institute of Astrophysics, Bangalore, 1914-04-18)
    The majority of the metallic lines in the solar spectrum are shifted to the red when compared with their positions in the electric are. There are, however, many exceptions. In the tables at the end of this paper I give the ...
  • Rama Rao, P. V. S; Prasad, DSVVD; Sri Ram, P; Jayachandran, P. T (Indian Institute of Astrophysics, Bangalore, 1997)
    The digital ionosonde system at Waltair was operated continuously from 23rd to 27th October 1995. The maximum percentage of obscuration (81%) of the solar disc occurred at 08.44 hrs IST as seen from Waltair on the eclipse ...
  • Evershed, John (Indian Institute of Astrophysics, Bangalore, 1909-08-24)
  • Evershed, John (Taylor and Francis, 1909-06)
  • Evershed, John (Taylor and Francis, 1909-09)

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