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pro vyhledávání: '"Bhavana Hegde"'
Autor:
Narra, Venkata Suresh, Raja, K. Sasikumar, B, Raghavendra Prasad, Singh, Jagdev, Mishra, Shalabh, U, Sanal Krishnan V, S, Bhavana Hegde, D., Utkarsha, V, Natarajan, S, Pawan Kumar, Priyal V, Muthu, P, Savarimuthu, Gavshinde, Priya, P, Umesh Kamath
The magnetic field strength and its topology play an important role in understanding the formation, evolution, and dynamics of the solar corona. Also, it plays a significant role in addressing long-standing mysteries such as coronal heating problem,
Externí odkaz:
http://arxiv.org/abs/2409.12793
Autor:
Mishra, Shalabh, Raja, K. Sasikumar, U, Sanal Krishnan V, Narra, Venkata Suresh, S, Bhavana Hegde, D., Utkarsha, Priyal V, Muthu, S, Pawan Kumar, V, Natarajan, B, Raghavendra Prasad, Singh, Jagdev, P, Umesh Kamath, S, Kathiravan, T, Vishnu, Suresha, P, Savarimuthu, Desai, Jalshri H, Kumaran, Rajiv, Sagar, Shiv, Kumar, Sumit, Bamrah, Inderjeet Singh, Kumar, Amit
Aditya-L1 is the first Indian space mission to explore the Sun and solar atmosphere with seven multi-wavelength payloads, with Visible Emission Line Coronagraph (VELC) being the prime payload. It is an internally occulted coronagraph with four channe
Externí odkaz:
http://arxiv.org/abs/2403.07373
Autor:
S. Nagabhushana, B. Raghavendra Prasad, Suresh Nagesh, Suresh Venkata Nara, D. S. Sandeep, P. U. Kamath, Shalab Misra, Bhavana Hegde, D. Utkarsha, Mrityunjay Kumar Sinha, S. Kathiravan, V. Natarajan, S. Pawan Kumar, Amit Kumar
Publikováno v:
Journal of Astronomical Instrumentation. 11
One of the major objectives of the optomechanics is to support large optics required for the purpose and also to maintain high dynamic stability in operation. This requirement calls for more number of supports, to support large optics. While addressi