Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/6730
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DC Field | Value | Language |
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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 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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X - ray spectrometers on - board Aditya - L1 for solar flare studies.pdf | 2.5 MB | Adobe PDF | View/Open |
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