X - ray spectrometers on - board Aditya - L1 for  solar flare studies

Sankarasubramanian, K; Sudhakar, M; Sudhakar, M; Nandi, Anuj; Ramadevi, M. C; Adoni, A. A; Kushwaha, A; Agarwal, Anil; Dey, A; Joshi, B; Singh, Brajpal||Girish, V; Tomar, I; Majhi, K. K; Kumar; Olekar, Manjunath; Bug, M; Pala, Manohar; Thakur, Mukund Kumar; Badagandi, Rajeev R; Ravishankar, B. T; Garg, Sarthak; Sitaramamurthy, N; Sridhara, N; Umapathy, C. N; Gupta, Vinod Kumar; Agrawal, Vivek Kumar; Yougandar, B

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dc.contributor.author	Sankarasubramanian, K
dc.contributor.author	Sudhakar, M
dc.contributor.author	Sudhakar, M
dc.contributor.author	Nandi, Anuj
dc.contributor.author	Ramadevi, M. C
dc.contributor.author	Adoni, A. A
dc.contributor.author	Kushwaha, A
dc.contributor.author	Agarwal, Anil
dc.contributor.author	Dey, A
dc.contributor.author	Joshi, B
dc.contributor.author	Singh, Brajpal\|\|Girish, V
dc.contributor.author	Tomar, I
dc.contributor.author	Majhi, K. K
dc.contributor.author	Kumar
dc.contributor.author	Olekar, Manjunath
dc.contributor.author	Bug, M
dc.contributor.author	Pala, Manohar
dc.contributor.author	Thakur, Mukund Kumar
dc.contributor.author	Badagandi, Rajeev R
dc.contributor.author	Ravishankar, B. T
dc.contributor.author	Garg, Sarthak
dc.contributor.author	Sitaramamurthy, N
dc.contributor.author	Sridhara, N
dc.contributor.author	Umapathy, C. N
dc.contributor.author	Gupta, Vinod Kumar
dc.contributor.author	Agrawal, Vivek Kumar
dc.contributor.author	Yougandar, B
dc.date.accessioned	2020-11-10T02:30:03Z
dc.date.available	2020-11-10T02:30:03Z
dc.date.issued	2017-04
dc.identifier.citation	Current Science, Vol. 113, No. 4, pp. 625 - 627	en_US
dc.identifier.issn	0011-3891
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/6730
dc.description	Open access © Current Science Association http://www.currentscience.ac.in/Volumes/113/04/0625.pdf	en_US
dc.description.abstract	Aditya-L1 mission will carry two high-spectral resolution X-ray spectrometers to study solar flares. The soft X-ray spectrometer will cover the energy range from 1 to 30 keV, while the hard X-ray spectrometer will cover from 10 to 150 keV. These two instruments together will provide opportunities to study the plasma parameters during solar flares as well as acceleration mechanisms of energetic particles during the flaring time.	en_US
dc.language.iso	en	en_US
dc.publisher	Current Science Association	en_US
dc.subject	Coronal heating	en_US
dc.subject	Solar flares	en_US
dc.subject	X-ray spectrometers	en_US
dc.title	X - ray spectrometers on - board Aditya - L1 for solar flare studies	en_US
dc.type	Article	en_US