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Autores principales: Prasad, K. Durga, Kumar, Chandan, Mishra, Sanjeev K., Reddy, P. Kalyana S., Kumar, Janmejay, Ladiya, Tinkal, Patel, Arpit, Bhardwaj, Anil
Formato: Preprint
Publicado: 2024
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Acceso en línea:https://arxiv.org/abs/2409.00150
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author Prasad, K. Durga
Kumar, Chandan
Mishra, Sanjeev K.
Reddy, P. Kalyana S.
Kumar, Janmejay
Ladiya, Tinkal
Patel, Arpit
Bhardwaj, Anil
author_facet Prasad, K. Durga
Kumar, Chandan
Mishra, Sanjeev K.
Reddy, P. Kalyana S.
Kumar, Janmejay
Ladiya, Tinkal
Patel, Arpit
Bhardwaj, Anil
contents Chandra Surface Thermophysical Experiment (ChaSTE) is one of the payloads flown onboard the Chandrayaan-3 lander. The objective of the experiment is in-situ investigation of thermal behaviour of outermost 100 mm layer of the lunar surface by deploying a thermal probe. The probe consists of 10 temperature sensors (Platinum RTDs) mounted at different locations along the length of the probe to measure lunar soil temperatures as a function of depth. A heater is also mounted on the probe for thermal conductivity measurements. The onboard electronics of ChaSTE has two parts, Front-End Electronics (FEE) and processing electronics (PE). The front-end electronics (FEE) card is responsible for carrying out necessary sensor signal conditioning,which includes exciting the RTD sensors,acquiring analog voltages and then converting the acquired analog signals to digital signals using an Analog to Digital Converter(ADC). The front-end card is further interfaced with the processing electronics card for digital processing and spacecraft interface.The calibration, characterisation and functional test activities of Front-End Electronics of ChaSTE were carried out with the objective of testing and ensuring proper functionality and performance.A two phase calibration process involving electronic offset correction and temperature calibration were carried out. All these activities were successfully completed and the results from them provided us with a really good understanding of the behaviour of the FEE under different thermal and electrical conditions as well as when subjected to the simulated conditions of the actual ChaSTE experiment. The performance of the ChaSTE front-end electronics was very much within the design margins and its behaviour in simulated lunar environment was as desired. The data from these activities is useful in the interpretation of the actual science data of ChaSTE.
format Preprint
id arxiv_https___arxiv_org_abs_2409_00150
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Characterisation of Front-End Electronics of ChaSTE experiment onboard Chandayaan-3 lander
Prasad, K. Durga
Kumar, Chandan
Mishra, Sanjeev K.
Reddy, P. Kalyana S.
Kumar, Janmejay
Ladiya, Tinkal
Patel, Arpit
Bhardwaj, Anil
Instrumentation and Detectors
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
Chandra Surface Thermophysical Experiment (ChaSTE) is one of the payloads flown onboard the Chandrayaan-3 lander. The objective of the experiment is in-situ investigation of thermal behaviour of outermost 100 mm layer of the lunar surface by deploying a thermal probe. The probe consists of 10 temperature sensors (Platinum RTDs) mounted at different locations along the length of the probe to measure lunar soil temperatures as a function of depth. A heater is also mounted on the probe for thermal conductivity measurements. The onboard electronics of ChaSTE has two parts, Front-End Electronics (FEE) and processing electronics (PE). The front-end electronics (FEE) card is responsible for carrying out necessary sensor signal conditioning,which includes exciting the RTD sensors,acquiring analog voltages and then converting the acquired analog signals to digital signals using an Analog to Digital Converter(ADC). The front-end card is further interfaced with the processing electronics card for digital processing and spacecraft interface.The calibration, characterisation and functional test activities of Front-End Electronics of ChaSTE were carried out with the objective of testing and ensuring proper functionality and performance.A two phase calibration process involving electronic offset correction and temperature calibration were carried out. All these activities were successfully completed and the results from them provided us with a really good understanding of the behaviour of the FEE under different thermal and electrical conditions as well as when subjected to the simulated conditions of the actual ChaSTE experiment. The performance of the ChaSTE front-end electronics was very much within the design margins and its behaviour in simulated lunar environment was as desired. The data from these activities is useful in the interpretation of the actual science data of ChaSTE.
title Characterisation of Front-End Electronics of ChaSTE experiment onboard Chandayaan-3 lander
topic Instrumentation and Detectors
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2409.00150