Science Filter Characterization of the Solar Ultraviolet Imaging Telescope (SUIT) on board Aditya-L1

Fuente: arXiv
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Autori principali: Sarkar, Janmejoy, Deogaonkar, Rushikesh, Kesharwani, Ravi, Padinhatteeri, Sreejith, Ramaprakash, A. N., Tripathi, Durgesh, Roy, Soumya, Ahmed, Gazi A., Chatterjee, Rwitika, Ghosh, Avyarthana, K., Sankarasubramanian, Khan, Aafaque, Mehandiratta, Nidhi, Pillai, Netra, Singh, Swapnil
Natura: Preprint
Pubblicazione: 2024
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author Sarkar, Janmejoy
Deogaonkar, Rushikesh
Kesharwani, Ravi
Padinhatteeri, Sreejith
Ramaprakash, A. N.
Tripathi, Durgesh
Roy, Soumya
Ahmed, Gazi A.
Chatterjee, Rwitika
Ghosh, Avyarthana
K., Sankarasubramanian
Khan, Aafaque
Mehandiratta, Nidhi
Pillai, Netra
Singh, Swapnil
author_facet Sarkar, Janmejoy
Deogaonkar, Rushikesh
Kesharwani, Ravi
Padinhatteeri, Sreejith
Ramaprakash, A. N.
Tripathi, Durgesh
Roy, Soumya
Ahmed, Gazi A.
Chatterjee, Rwitika
Ghosh, Avyarthana
K., Sankarasubramanian
Khan, Aafaque
Mehandiratta, Nidhi
Pillai, Netra
Singh, Swapnil
contents The Solar Ultraviolet Imaging Telescope (SUIT) on board the Aditya-L1 mission is designed to observe the Sun across 200-400 nm wavelength. The telescope used 16 dichroic filters tuned at specific wavelengths in various combinations to achieve its science goals. For accurate measurements and interpretation, it is important to characterize these filters for spectral variations as a function of spatial location and tilt angle. Moreover, we also measured out-of-band and in-band transmission characteristics with respect to the inband transmissions. In this paper, we present the experimental setup, test methodology, and the analyzed results. Our findings reveal that the transmission properties of all filters meet the expected performance for spatial variation of transmission and the transmission band at a specific tilt angle. The out-of-band transmission for all filters is below 1% with respect to in-band, except for filters BB01 and NB01. These results confirm the capabilities of SUIT to effectively capture critical solar features in the anticipated layer of the solar atmosphere.
format Preprint
id arxiv_https___arxiv_org_abs_2412_11636
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Science Filter Characterization of the Solar Ultraviolet Imaging Telescope (SUIT) on board Aditya-L1
Sarkar, Janmejoy
Deogaonkar, Rushikesh
Kesharwani, Ravi
Padinhatteeri, Sreejith
Ramaprakash, A. N.
Tripathi, Durgesh
Roy, Soumya
Ahmed, Gazi A.
Chatterjee, Rwitika
Ghosh, Avyarthana
K., Sankarasubramanian
Khan, Aafaque
Mehandiratta, Nidhi
Pillai, Netra
Singh, Swapnil
Solar and Stellar Astrophysics
Instrumentation and Methods for Astrophysics
The Solar Ultraviolet Imaging Telescope (SUIT) on board the Aditya-L1 mission is designed to observe the Sun across 200-400 nm wavelength. The telescope used 16 dichroic filters tuned at specific wavelengths in various combinations to achieve its science goals. For accurate measurements and interpretation, it is important to characterize these filters for spectral variations as a function of spatial location and tilt angle. Moreover, we also measured out-of-band and in-band transmission characteristics with respect to the inband transmissions. In this paper, we present the experimental setup, test methodology, and the analyzed results. Our findings reveal that the transmission properties of all filters meet the expected performance for spatial variation of transmission and the transmission band at a specific tilt angle. The out-of-band transmission for all filters is below 1% with respect to in-band, except for filters BB01 and NB01. These results confirm the capabilities of SUIT to effectively capture critical solar features in the anticipated layer of the solar atmosphere.
title Science Filter Characterization of the Solar Ultraviolet Imaging Telescope (SUIT) on board Aditya-L1
topic Solar and Stellar Astrophysics
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2412.11636