Calibration of Spectropolarimetry Package for Visible Emission Line Coronagraph (VELC) on Board Aditya-L1 Mission

Author:

Narra Venkata Suresh1ORCID,Hegde Bhavana1,Dasamantarao Utkarsha1,Venkatasubramanian Natarajan1,Somasundaram Pawan Kumar1,Padhavu Umesh Kamath1,Budihal Raghavendra Prasad1

Affiliation:

1. Indian Institute of Astrophysics, II Block Koramangala, Bangalore 560034, India

Abstract

Visible Emission Line Coronagraph (VELC) is the prime payload on board Aditya-L1 mission. One of the unique capabilities of VELC is the coronal magnetic field measurements from space. To achieve this, VELC performs dual beam spectropolarimetric observations in coronal emission line centered at 10747[Formula: see text]Å. Spectropolarimetric channel of VELC consists of different polarimetric components such as quarter waveplate (QWP), polarising beam displacer (PBD) and half waveplate (HWP). Calibration of individual components is essential to ensure that they meet the performance requirements of the payload. This work discusses the details of the calibration tests carried out to evaluate the performance of different polarimetric components of VELC and the results obtained.

Funder

Indian Space Research Organisation

Publisher

World Scientific Pub Co Pte Ltd

Subject

Astronomy and Astrophysics,Instrumentation

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Ground calibration of visible emission line coronagraph on board Aditya-L1 mission;Journal of Astronomical Telescopes, Instruments, and Systems;2023-10-17

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