Paper
18 July 2016 Near UV imager with an MCP-based photon counting detector
S. Ambily, Joice Mathew, Mayuresh Sarpotdar, A. G. Sreejith, K. Nirmal, Ajin Prakash, Margarita Safonova, Jayant Murthy
Author Affiliations +
Abstract
We are developing a compact UV Imager using light weight components, that can be own on a small CubeSat or a balloon platform. The system has a lens-based optics that can provide an aberration-free image over a wide field of view. The backend instrument is a photon counting detector with off-the-shelf MCP, CMOS sensor and electronics. We are using a Z-stack MCP with a compact high voltage power supply and a phosphor screen anode, which is read out by a CMOS sensor and the associated electronics. The instrument can be used to observe solar system objects and detect bright transients from the upper atmosphere with the help of CubeSats or high altitude balloons. We have designed the imager to be capable of working in direct frame transfer mode as well in the photon-counting mode for single photon event detection. The identification and centroiding of each photon event are done using an FPGA-based data acquisition and real-time processing system.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
S. Ambily, Joice Mathew, Mayuresh Sarpotdar, A. G. Sreejith, K. Nirmal, Ajin Prakash, Margarita Safonova, and Jayant Murthy "Near UV imager with an MCP-based photon counting detector", Proc. SPIE 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 990539 (18 July 2016); https://doi.org/10.1117/12.2232435
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KEYWORDS
Ultraviolet radiation

Exoplanets

Planets

Spectroscopy

Homodyne detection

Atmospheric modeling

Space telescopes

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