Browsing by Author Pande, M. C

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Issue DateTitleAuthor(s)
Dec-1984Association of Coronal holes with large scale Solar Magnetic fieldsShelke, R. N; Pande, M. C
Jun-1986Association of solar flares with twisting of magnetic neutral linesUddin, W; Pande, M. C; Shelke, R. N
Dec-1982Behaviour of some neutral molecular absorption lines in facula modelsTripathi, B. M; Sinha, K; Pande, M. C
Dec-1981Brackett-gamma line and facula modelsTripathi, B. M; Pande, M. C
1992Can HeH(+) molecule be present in solar photosphereGaur, V. P; Joshi, G. C; Pande, M. C
Jun-1982Carbon monoxide and facula modelsTripathi, B. M; Pande, M. C; Sinha, K
1998CCD observations of eruptive prominence of March 19, 1994Uddin, W; Gaur, V. P; Pande, M. C
1998CCD observations of eruptive prominence of March 19, 1994Uddin, W; Gaur, V. P; Pande, M. C
Mar-1980Centre to Limb Variation of Rotational Temperature of the CH Molecules in the Solar PhotospherePande, M. C; Gaur, V. P; Bondal, K. R; Dubey, R. C
Dec-1984Coronal holes and long-lived unipolar magnetic regionsShelke, R. N; Pande, M. C
Mar-1983Double ribbon flare of 1981 October 19Verma, V. K; Pande, M. C
1990Eclipsing binary research at Uttar Pradesh State ObservatorySrivastava, J. B; Chaubey, U. S; Pande, M. C
1995Evolution of the helical prominence of December 15, 1992Uddin, W; Gaur, V. P; Pande, M. C
Jun-1982Franck-Condon factors for some abundant umbral moleculesJoshi, G. C; Joshi, U. C; Punetha, L. M; Pande, M. C
Sep-1981Ionized molecules in facula modelsTripathi, B. M; Gaur, V. P; Pande, M. C
1995A note on the rotational motion in quiescent prominencesPande, M. C; Bondal, K. R
Jun-1980Observations of Total Solar Eclipse of February 16, 1980Gaur, V. P; Bondal, K. R; Sinha, K; Joshi, G. C; Pande, M. C
Dec-1986On the behaviour of some visible and infrared atomic hydrogen lines in facular modelsBondal, K. R; Gaur, V. P; Pande, M. C
Sep-1984On the recurrence of sudden ionospheric disturbancesShelke, R. N; Pande, M. C
Dec-1983On the relation between large scale solar magnetic fields and filament positionsShelke, R. N; Pande, M. C