Giulia Conenna, Andrea Tartari, Giovanni Signorelli, Andrea Passerini, Andrea Limonta, Mario Zannoni, Paolo Dal Bo, Eugenia Di Giorgi, Jean-François Cliche, Stefano Della Torre, Matt Dobbs, Luca Galli, Massimo Gervasi, Maurizio Massa, Andrea Moggi, Joshua Montgomery, Donato Nicolò, Michele Pinchera, Graeme Smecher, Franco Spinella
{"title":"用于 LiteBIRD 太空任务的 SQUID 控制装置:说明、功能测试和早期性能评估","authors":"Giulia Conenna, Andrea Tartari, Giovanni Signorelli, Andrea Passerini, Andrea Limonta, Mario Zannoni, Paolo Dal Bo, Eugenia Di Giorgi, Jean-François Cliche, Stefano Della Torre, Matt Dobbs, Luca Galli, Massimo Gervasi, Maurizio Massa, Andrea Moggi, Joshua Montgomery, Donato Nicolò, Michele Pinchera, Graeme Smecher, Franco Spinella","doi":"10.1007/s10909-024-03124-y","DOIUrl":null,"url":null,"abstract":"<div><p>LiteBIRD is a satellite mission to be launched by JAXA in the early 2030s. It will measure the Cosmic Microwave Background (CMB) primordial B-modes with an unprecedented sensitivity. Microwave radiation will be detected by Transition Edge Sensors (TESs) arrays multiplexed in frequency domain and read by Superconducting QUantum Interference Devices (SQUIDs). The LiteBIRD SQUID Controller Unit (SCU), based on the heritage of the successful design used for the ground-based SPT3G experiment, presents some novel elements that make it suitable for a space-borne application. We compare our first breadboard model with the ground-based, Off-The-Shelf Components (COTS) version, by driving the same SQUID Array Amplifier (SAA) at 4 K, measuring relevant quantities such as noise, gain and bandwidth. We demonstrate that the noise added by our first prototype (including a switching part for redundancy purposes) never exceeds the noise added by the COTS-based electronics board, representing our benchmark. We also present the first noise estimates with the SAA cooled below 1 K, going closer to the conditions expected for LiteBIRD operation.</p></div>","PeriodicalId":641,"journal":{"name":"Journal of Low Temperature Physics","volume":null,"pages":null},"PeriodicalIF":1.1000,"publicationDate":"2024-05-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s10909-024-03124-y.pdf","citationCount":"0","resultStr":"{\"title\":\"The SQUID Controller Unit for the LiteBIRD Space Mission: Description, Functional Tests and Early Performance Assessment\",\"authors\":\"Giulia Conenna, Andrea Tartari, Giovanni Signorelli, Andrea Passerini, Andrea Limonta, Mario Zannoni, Paolo Dal Bo, Eugenia Di Giorgi, Jean-François Cliche, Stefano Della Torre, Matt Dobbs, Luca Galli, Massimo Gervasi, Maurizio Massa, Andrea Moggi, Joshua Montgomery, Donato Nicolò, Michele Pinchera, Graeme Smecher, Franco Spinella\",\"doi\":\"10.1007/s10909-024-03124-y\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>LiteBIRD is a satellite mission to be launched by JAXA in the early 2030s. It will measure the Cosmic Microwave Background (CMB) primordial B-modes with an unprecedented sensitivity. Microwave radiation will be detected by Transition Edge Sensors (TESs) arrays multiplexed in frequency domain and read by Superconducting QUantum Interference Devices (SQUIDs). The LiteBIRD SQUID Controller Unit (SCU), based on the heritage of the successful design used for the ground-based SPT3G experiment, presents some novel elements that make it suitable for a space-borne application. We compare our first breadboard model with the ground-based, Off-The-Shelf Components (COTS) version, by driving the same SQUID Array Amplifier (SAA) at 4 K, measuring relevant quantities such as noise, gain and bandwidth. We demonstrate that the noise added by our first prototype (including a switching part for redundancy purposes) never exceeds the noise added by the COTS-based electronics board, representing our benchmark. We also present the first noise estimates with the SAA cooled below 1 K, going closer to the conditions expected for LiteBIRD operation.</p></div>\",\"PeriodicalId\":641,\"journal\":{\"name\":\"Journal of Low Temperature Physics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":1.1000,\"publicationDate\":\"2024-05-03\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://link.springer.com/content/pdf/10.1007/s10909-024-03124-y.pdf\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Low Temperature Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s10909-024-03124-y\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"PHYSICS, APPLIED\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Low Temperature Physics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10909-024-03124-y","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"PHYSICS, APPLIED","Score":null,"Total":0}
引用次数: 0
摘要
LiteBIRD 是日本宇宙航空研究开发机构将于 2030 年代初发射的一项卫星任务。它将以前所未有的灵敏度测量宇宙微波背景(CMB)的原始 B 模式。微波辐射将由频域多路复用的过渡边缘传感器(TES)阵列探测,并由超导量子干涉装置(SQUID)读取。LiteBIRD SQUID 控制单元(SCU)继承了用于地面 SPT3G 试验的成功设计,并加入了一些新的元素,使其适用于空间应用。我们通过在 4 K 温度下驱动相同的 SQUID 阵列放大器(SAA),测量噪声、增益和带宽等相关参数,将我们的首个面包板模型与地面现成组件(COTS)版本进行了比较。我们证明,我们的第一个原型(包括一个用于冗余目的的开关部件)所增加的噪声从未超过基于 COTS 的电子板(代表我们的基准)所增加的噪声。我们还首次提出了在 SAA 冷却到 1 K 以下时的噪声估计值,更接近 LiteBIRD 运行的预期条件。
The SQUID Controller Unit for the LiteBIRD Space Mission: Description, Functional Tests and Early Performance Assessment
LiteBIRD is a satellite mission to be launched by JAXA in the early 2030s. It will measure the Cosmic Microwave Background (CMB) primordial B-modes with an unprecedented sensitivity. Microwave radiation will be detected by Transition Edge Sensors (TESs) arrays multiplexed in frequency domain and read by Superconducting QUantum Interference Devices (SQUIDs). The LiteBIRD SQUID Controller Unit (SCU), based on the heritage of the successful design used for the ground-based SPT3G experiment, presents some novel elements that make it suitable for a space-borne application. We compare our first breadboard model with the ground-based, Off-The-Shelf Components (COTS) version, by driving the same SQUID Array Amplifier (SAA) at 4 K, measuring relevant quantities such as noise, gain and bandwidth. We demonstrate that the noise added by our first prototype (including a switching part for redundancy purposes) never exceeds the noise added by the COTS-based electronics board, representing our benchmark. We also present the first noise estimates with the SAA cooled below 1 K, going closer to the conditions expected for LiteBIRD operation.
期刊介绍:
The Journal of Low Temperature Physics publishes original papers and review articles on all areas of low temperature physics and cryogenics, including theoretical and experimental contributions. Subject areas include: Quantum solids, liquids and gases; Superfluidity; Superconductivity; Condensed matter physics; Experimental techniques; The Journal encourages the submission of Rapid Communications and Special Issues.