Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8691
Title: The solar ultraviolet imaging telescope on board Aditya-L1
Authors: Tripathi, Durgesh
Ramaprakash, A. N
Padinhatteeri, Sreejith
Sarkar, Janmejoy
Burse, Mahesh
Tyagi, Anurag
Kesharwani, Ravi
Sinha, Sakya
Joshi, Bhushan
Deogaonkar, Rushikesh
Roy, Soumya
Nived, V. N
Gopalakrishnan, Rahul
Kulkarni, Akshay
Khan, Aafaque
Ghosh, Avyarthana
Rajarshi, Chaitanya
Modi, Deepa
Kumar, Ghanshyam
Yadav, Reena
Varma, Manoj
Bayanna, A. R
Chordia, Pravin
Karmakar, Mintu
Abraham, Linn
Adithya, H. N
Adoni, A. A
Ahmed, Gazi A
Banerjee, D
Bhargava Ram, B. S
Bhandare, Rani
Chatterjee, Subhamoy
Chillal, Kalpesh
Dey, A
Gandorfer, Achim
Gowda, Girish
Haridas, T. R
Jain, Anand
James, Melvin K
Jayakumar, R. P
Justin, Evangeline Leeja
Nagaraju, K
Kathait, Deepak
Khodade, Pravin
Kiran, Mandeep
Kohok, A
Krivova, Natalie A
Kumar, Nishank
Mehandiratta, Nidhi
Mestry, V. B
Motamarri, Srikanth
Mustafa, Sajjade F
Nandy, D
Narendranath, S
Navle, Sonal
Parate, Nashiket
Pillai, Anju M
Punnadi, Sujit
Rajendra, A
Ravi, A
Raha, Bijoy
Sankarasubramanian, K
Sarvar, Ghulam
Shaji, Nigar
Sharma, Nidhi
Singh, Aditya
Singh, Shivam
Solanki, S. K
Subramanian, Vivek
Rethika, T
Srikanth, T
Thatimattala, Satyannarayana
Tota, Hari Krishna
Vishnu, T. S
Unnikrishnan, Amrita
Vadodariya, Kaushal
Veeresha, D. R
Venkateswaran, R
Keywords: Photosphere
Chromosphere
Flares
Dynamics
Heating
Magnetic fields
Prominences
Solar Cycle
Solar Irradiance
Instrumentation and Data Management
Issue Date: Mar-2025
Publisher: Springer Nature
Citation: Solar Physics, Vol. 300, No. 3, 30
Abstract: The Solar Ultraviolet Imaging Telescope (SUIT) is an instrument on the Aditya-L1 mission of the Indian Space Research Organization (ISRO) launched on 2 September 2023. SUIT continuously provides near-simultaneous full-disk and region-of-interest images of the Sun, slicing through the photosphere and chromosphere and covering a field of view up to 1.5 solar radii. For this purpose, SUIT uses 11 filters tuned at different wavelengths in the 200 – 400 nm range, including the Mg II h and k and Ca II H spectral lines. The observations made by SUIT help us understand the magnetic coupling of the lower and middle solar atmosphere. In addition, for the first time, this allows for the measurements of spatially resolved solar broad-band radiation in the near- and mid-ultraviolet, which will help constrain the variability of the solar ultraviolet irradiance in a wavelength range that is central for the chemistry of ozone and oxygen the Earth’s stratosphere. This paper discusses the details of the instrument and data products.
Description: Restricted Access
URI: http://hdl.handle.net/2248/8691
ISSN: 0038-0938
Appears in Collections:IIAP Publications

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