Sep 14 – 16, 2022
IIA Bangalore
Asia/Kolkata timezone
Poster Size for META 2022 : A0 Size Poster is preferred as fixing board size at IIA is 56 inches x 46 inches (landscape orientation)

Electronics subsystem development of SING spectrograph payload

Not scheduled
20m
IIA Bangalore

IIA Bangalore

Speaker

Mr Bharat Chandra P

Description

SING is a near ultraviolet (NUV) spectrograph which operates in the wavelength range from 1400 Å to 2700 Å, with a spectral resolution of about 3 Å at 2000 Å. The spectrograph is intended to operate in low Earth orbit (LEO), with the primary goal to generate spectral maps of the regions of the sky covered within the field of view (FOV) of the instrument, constrained by the orbital inclination of the spacecraft. As the event rate in the UV is low, the spectrograph employs a photon-counting detector because of its low noise performance. SING on-board electronics consists of 4 subsystems- a photon counting detector based on Raspberry Pi 3, an on-board computer (OBC) based on an STM32 microcontroller, a power supply and a 1553B communication module. Here we will present the low-cost development of the four subsystems using COTS (commercial-off-the-shelf) components.

Presentation type Oral

Primary authors

Mr Bharat Chandra P Shubham Ghatul (Indian Institute of Astrophysics) Ms Shubhangi Jain (Indian Institute of Astrophysics) Binukumar Gopalakrishnan (Indian Institute of Astrophysics) Rekhesh Mohan (Indian Institute of Astrophysics) Jayant Murthy (Indian Institute of Astrophysics) Margarita Safonova (Indian Institute of Astrophysics)

Presentation materials

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