Evaluation of the performance of the CCD236 swept charge devices in lunar orbit using in-flight data
India’s Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS) employs 16 CCD236 Swept Charge Devices (SCDs) similar in structure to Charge Coupled Device (CCD) image sensors. The CCD236 permits X-ray detection over a large surface area, intended to improve low flux performance, with simplified co...
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Published in | Journal of instrumentation Vol. 17; no. 7; p. C07013 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Bristol
IOP Publishing
01.07.2022
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Subjects | |
Online Access | Get full text |
ISSN | 1748-0221 1748-0221 |
DOI | 10.1088/1748-0221/17/07/C07013 |
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Abstract | India’s Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS) employs 16 CCD236 Swept Charge Devices (SCDs) similar in structure to Charge Coupled Device (CCD) image sensors. The CCD236 permits X-ray detection over a large surface area, intended to improve low flux performance, with simplified control interfaces and improved warm temperature performance. These devices were the subject of ground testing and performance evaluation before flight. Data that was recently made available by the Indian Space Research Organisation (ISRO) has permitted the analysis of the performance of the CLASS SCDs after over a year of operations around the Moon. Of particular interest is the change in device performance and behaviour during transit and in lunar orbit. Preliminary analysis has indicated that device FWHM, representing the aggregate of different noise sources, has increased in line with predictions based on ground irradiation and testing. |
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AbstractList | India’s Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS) employs 16 CCD236 Swept Charge Devices (SCDs) similar in structure to Charge Coupled Device (CCD) image sensors. The CCD236 permits X-ray detection over a large surface area, intended to improve low flux performance, with simplified control interfaces and improved warm temperature performance. These devices were the subject of ground testing and performance evaluation before flight. Data that was recently made available by the Indian Space Research Organisation (ISRO) has permitted the analysis of the performance of the CLASS SCDs after over a year of operations around the Moon. Of particular interest is the change in device performance and behaviour during transit and in lunar orbit. Preliminary analysis has indicated that device FWHM, representing the aggregate of different noise sources, has increased in line with predictions based on ground irradiation and testing. |
Author | Jones, L.S. Endicott, J. Holland, A.D. Crews, C. |
Author_xml | – sequence: 1 givenname: L.S. surname: Jones fullname: Jones, L.S. organization: The Open University Centre for Electronic Imaging, Walton Hall, Milton Keynes, U.K – sequence: 2 givenname: C. surname: Crews fullname: Crews, C. organization: The Open University Centre for Electronic Imaging, Walton Hall, Milton Keynes, U.K – sequence: 3 givenname: J. surname: Endicott fullname: Endicott, J. organization: The Open University Centre for Electronic Imaging, Walton Hall, Milton Keynes, U.K – sequence: 4 givenname: A.D. surname: Holland fullname: Holland, A.D. organization: The Open University Centre for Electronic Imaging, Walton Hall, Milton Keynes, U.K |
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Cites_doi | 10.18520/cs/v118/i2/219-225 10.1117/12.926213 10.1088/1748-0221/10/03/C03041 10.1016/j.nima.2012.04.013 10.1088/1748-0221/10/01/C01037 10.1016/j.icarus.2021.114436 10.1117/12.826856 |
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SubjectTerms | Charge coupled devices Ground tests Indian space program Indian spacecraft Lunar orbits Lunar probes Moon Performance evaluation Radiation damage to detector materials (solid state) Soft x rays Space instrumentation Space research X ray spectrometers X-ray detectors |
Title | Evaluation of the performance of the CCD236 swept charge devices in lunar orbit using in-flight data |
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