Open Access Open Access  Restricted Access Subscription Access

Silicon carbide-based functional components in the Visible Emission Line Coronagraph on-board the ADITYA-L1 mission


Affiliations
1 International Advanced Research Centre for Powder Metallurgy and New Materials, Balapur Post, RCI Road, Hyderabad 500 005, India
2 Indian Institute of Astrophysics, 2nd Block, Koramangala, Bengaluru 560 034, India
3 U. R. Rao Satellite Centre, Old Airport Road, Vimanapura Post, Bengaluru 560 017, India
4 Laboratory for Electro-Optics Systems, First Phase, Peenya Industrial Estate, Bengaluru 560 058, India

A state-of-the-art Visible Emission Line Coronagraph (VELC) payload on-board India’s solar mission ADITYA-L1 was designed to study various solar pheno­mena. To maintain the thermal stability of the system, VELC design recommends silicon carbide (SiC)-based components because of their outstanding mechanical, thermal and optical properties. In particular, a SiC-based tertiary mirror (M3) was used for the collection of undesired sunrays and reflecting them out from the system, and a SiC radiator plate (popularly known as a cold finger) for efficient heat dissipation from the mirror and, in turn, from the system. This article describes the processing and evaluation of SiC-based M3 mirror and cold finger for VELC. The substrates for M3 mirror and cold finger were processed through dry pressing of SiC powder with the required formulation, followed by machining and temperature-assisted densification under an inert atmosphere. SiC components developed using powder metallurgical technique exhibited about 98.4% relative density (RD) and achieved the structural and thermal requirements of M3 mirror and cold finger. The optical requirement of M3 mirror was achieved through a coating of SiC substrate with 100% RD employing chemical vapour deposition followed by surface grinding and polishing. The final mirror achieved a surface flatness better than 20 nm, and microroughness data showed less than 5.1 Å root mean square surface roughness in a spatial scale of 0.02 to 0.9 mm

Keywords

Chemical vapour deposition, coronagraph, relative density, silicon carbide, solar mission.
User
Notifications
Font Size

Abstract Views: 141




  • Silicon carbide-based functional components in the Visible Emission Line Coronagraph on-board the ADITYA-L1 mission

Abstract Views: 141  | 

Authors

Bhaskar Prasad Saha
International Advanced Research Centre for Powder Metallurgy and New Materials, Balapur Post, RCI Road, Hyderabad 500 005, India
Dulal Chandra Jana
International Advanced Research Centre for Powder Metallurgy and New Materials, Balapur Post, RCI Road, Hyderabad 500 005, India
Prasenjit Barick
International Advanced Research Centre for Powder Metallurgy and New Materials, Balapur Post, RCI Road, Hyderabad 500 005, India
V. Natarajan
Indian Institute of Astrophysics, 2nd Block, Koramangala, Bengaluru 560 034, India
Suresh Venkata
Indian Institute of Astrophysics, 2nd Block, Koramangala, Bengaluru 560 034, India
Abhijit A. Adoni
U. R. Rao Satellite Centre, Old Airport Road, Vimanapura Post, Bengaluru 560 017, India
D. R. Veeresha
U. R. Rao Satellite Centre, Old Airport Road, Vimanapura Post, Bengaluru 560 017, India
R. Venkateswaran
Laboratory for Electro-Optics Systems, First Phase, Peenya Industrial Estate, Bengaluru 560 058, India
P. U. Kamath
Indian Institute of Astrophysics, 2nd Block, Koramangala, Bengaluru 560 034, India
Roy Johnson
International Advanced Research Centre for Powder Metallurgy and New Materials, Balapur Post, RCI Road, Hyderabad 500 005, India
K. V. Sriram
Laboratory for Electro-Optics Systems, First Phase, Peenya Industrial Estate, Bengaluru 560 058, India
B. Raghavendra Prasad
Indian Institute of Astrophysics, 2nd Block, Koramangala, Bengaluru 560 034, India
G. Padmanabham
International Advanced Research Centre for Powder Metallurgy and New Materials, Balapur Post, RCI Road, Hyderabad 500 005, India

Abstract


A state-of-the-art Visible Emission Line Coronagraph (VELC) payload on-board India’s solar mission ADITYA-L1 was designed to study various solar pheno­mena. To maintain the thermal stability of the system, VELC design recommends silicon carbide (SiC)-based components because of their outstanding mechanical, thermal and optical properties. In particular, a SiC-based tertiary mirror (M3) was used for the collection of undesired sunrays and reflecting them out from the system, and a SiC radiator plate (popularly known as a cold finger) for efficient heat dissipation from the mirror and, in turn, from the system. This article describes the processing and evaluation of SiC-based M3 mirror and cold finger for VELC. The substrates for M3 mirror and cold finger were processed through dry pressing of SiC powder with the required formulation, followed by machining and temperature-assisted densification under an inert atmosphere. SiC components developed using powder metallurgical technique exhibited about 98.4% relative density (RD) and achieved the structural and thermal requirements of M3 mirror and cold finger. The optical requirement of M3 mirror was achieved through a coating of SiC substrate with 100% RD employing chemical vapour deposition followed by surface grinding and polishing. The final mirror achieved a surface flatness better than 20 nm, and microroughness data showed less than 5.1 Å root mean square surface roughness in a spatial scale of 0.02 to 0.9 mm

Keywords


Chemical vapour deposition, coronagraph, relative density, silicon carbide, solar mission.



DOI: https://doi.org/10.18520/cs%2Fv125%2Fi12%2F1323-1327