Nirmalsinh A. Parmar, Jitendra Adwani, Vaibhav Surana, F. M. Pathan, Hiren K. Mewada
{"title":"基于LabVIEW的高精度温度记录仪项目PARAS","authors":"Nirmalsinh A. Parmar, Jitendra Adwani, Vaibhav Surana, F. M. Pathan, Hiren K. Mewada","doi":"10.1109/ICCSP.2015.7322832","DOIUrl":null,"url":null,"abstract":"The “High Precision Temperature Logger” is designed for the project PARAS (PRL Advance Radial velocity Abu sky Search) to achieve a maximum temperature stability (like 0.01°C rms) throughout the period of observation of thermally insulated chamber where PARAS spectrograph is installed. The scientific aspect of the temperature controlled environment is to bring down the error in radial velocity measurement to 1m/s. Radial velocity (RV) technique is used to determine various orbital parameters in exo-planet search. It has been found that temperature variation of 1°C at the spectrograph environment can increase the error in radial velocity measurement by few thousands of m/s. Mechanical flexures (in the scale of micrometers) in the optical components can increase the error by a significant percentage due to temperature and pressure variations. So the temperature stability is very important for the PARAS project. So high precision temperature logger with a high stability is designed for PARAS project with the help of LabVIEW.","PeriodicalId":174192,"journal":{"name":"2015 International Conference on Communications and Signal Processing (ICCSP)","volume":"7 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2015-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"LabVIEW based High Precision Temperature Logger for the project PARAS\",\"authors\":\"Nirmalsinh A. Parmar, Jitendra Adwani, Vaibhav Surana, F. M. Pathan, Hiren K. Mewada\",\"doi\":\"10.1109/ICCSP.2015.7322832\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The “High Precision Temperature Logger” is designed for the project PARAS (PRL Advance Radial velocity Abu sky Search) to achieve a maximum temperature stability (like 0.01°C rms) throughout the period of observation of thermally insulated chamber where PARAS spectrograph is installed. The scientific aspect of the temperature controlled environment is to bring down the error in radial velocity measurement to 1m/s. Radial velocity (RV) technique is used to determine various orbital parameters in exo-planet search. It has been found that temperature variation of 1°C at the spectrograph environment can increase the error in radial velocity measurement by few thousands of m/s. Mechanical flexures (in the scale of micrometers) in the optical components can increase the error by a significant percentage due to temperature and pressure variations. So the temperature stability is very important for the PARAS project. So high precision temperature logger with a high stability is designed for PARAS project with the help of LabVIEW.\",\"PeriodicalId\":174192,\"journal\":{\"name\":\"2015 International Conference on Communications and Signal Processing (ICCSP)\",\"volume\":\"7 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2015-04-02\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2015 International Conference on Communications and Signal Processing (ICCSP)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/ICCSP.2015.7322832\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2015 International Conference on Communications and Signal Processing (ICCSP)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/ICCSP.2015.7322832","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
摘要
“高精度温度记录仪”是为PARAS (PRL Advance Radial velocity Abu sky Search)项目设计的,用于在安装PARAS光谱仪的隔热室的整个观测期间实现最大温度稳定性(如0.01°C rms)。温度控制环境的科学方面是将径向速度测量误差降低到1m/s。在系外行星搜索中,视向速度(RV)技术用于确定各种轨道参数。研究发现,在摄谱仪环境下,温度每变化1℃,径向速度测量误差就会增加几千m/s。由于温度和压力的变化,光学元件中的机械弯曲(以微米为尺度)会增加误差的显着百分比。因此,温度稳定性对PARAS项目来说是非常重要的。为此,利用LabVIEW软件为PARAS项目设计了高精度、高稳定性的温度记录仪。
LabVIEW based High Precision Temperature Logger for the project PARAS
The “High Precision Temperature Logger” is designed for the project PARAS (PRL Advance Radial velocity Abu sky Search) to achieve a maximum temperature stability (like 0.01°C rms) throughout the period of observation of thermally insulated chamber where PARAS spectrograph is installed. The scientific aspect of the temperature controlled environment is to bring down the error in radial velocity measurement to 1m/s. Radial velocity (RV) technique is used to determine various orbital parameters in exo-planet search. It has been found that temperature variation of 1°C at the spectrograph environment can increase the error in radial velocity measurement by few thousands of m/s. Mechanical flexures (in the scale of micrometers) in the optical components can increase the error by a significant percentage due to temperature and pressure variations. So the temperature stability is very important for the PARAS project. So high precision temperature logger with a high stability is designed for PARAS project with the help of LabVIEW.