Issue Date | Title | Author(s) |
1992 | Can HeH(+) molecule be present in solar photosphere | Gaur, V. P; Joshi, G. C; Pande, M. C |
1998 | CCD observations of eruptive prominence of March 19, 1994 | Uddin, W; Gaur, V. P; Pande, M. C |
1998 | CCD observations of eruptive prominence of March 19, 1994 | Uddin, W; Gaur, V. P; Pande, M. C |
1997 | CCD Observations of the Total Solar Eclipse of October 24, 1995 | Verma, V. K; Wahab Uddin; Gaur, V. P; Joshi, G. C; Bondal, K. R |
1980-03 | Centre to Limb Variation of Rotational Temperature of the CH Molecules in the Solar Photosphere | Pande, M. C; Gaur, V. P; Bondal, K. R; Dubey, R. C |
1995 | Evolution of the helical prominence of December 15, 1992 | Uddin, W; Gaur, V. P; Pande, M. C |
1981-09 | Ionized molecules in facula models | Tripathi, B. M; Gaur, V. P; Pande, M. C |
1980-06 | Observations of Total Solar Eclipse of February 16, 1980 | Gaur, V. P; Bondal, K. R; Sinha, K; Joshi, G. C; Pande, M. C |
1986-06 | On some visible and infrared atomic hydrogen lines in three photospheric models | Bondal, K. R; Gaur, V. P |
1986-12 | On the behaviour of some visible and infrared atomic hydrogen lines in facular models | Bondal, K. R; Gaur, V. P; Pande, M. C |
1987 | On the centre-to-limb variation of some visible and infrared atomic hydrogen lines in three facular models | Bondal, K. R; Gaur, V. P |
1987-03 | On the Solar Limb Darkening in the Wings of Some Atomic Hydrogen Lines | Bondal, K. R; Gaur, V. P; Pande, M. C |
1994 | On the unusual surge of 1991 November 16 | Bondal, K. R; Gaur, V. P; Joshi, A; Uddin, W; Pande, M. C |
1998 | Proposed 60-cm multichannel Solar Vacuum Telescope of UPSO, Naini Tal | Verma, V. K; Uddin, W; Gaur, V. P |
1998 | Solar observational programs and facilities at UPSO, Naini Tal | Gaur, V. P; Verma, V. K; Uddin, W |
1995 | Study of a quiescent prominence | Joshi, A; Gaur, V. P; Pande, M. C |
1996 | Total solar eclipse observations of 24 October 1995 from Meja Khas, Allahabad | Verma, V. K; Uddin, W; Gaur, V. P; Joshi, G. C; Bondal, K. R; Pant, P |