Bale S D, Goetz K, Harvey P R, Turin P, Bonnell J W, de Wit T Dudok, Ergun R E, MacDowall R J, Pulupa M, Andre M, Bolton M, Bougeret J-L, Bowen T A, Burgess D, Cattell C A, Chandran B D G, Chaston C C, Chen C H K, Choi M K, Connerney J E, Cranmer S, Diaz-Aguado M, Donakowski W, Drake J F, Farrell W M, Fergeau P, Fermin J, Fischer J, Fox N, Glaser D, Goldstein M, Gordon D, Hanson E, Harris S E, Hayes L M, Hinze J J, Hollweg J V, Horbury T S, Howard R A, Hoxie V, Jannet G, Karlsson M, Kasper J C, Kellogg P J, Kien M, Klimchuk J A, Krasnoselskikh V V, Krucker S, Lynch J J, Maksimovic M, Malaspina D M, Marker S, Martin P, Martinez-Oliveros J, McCauley J, McComas D J, McDonald T, Meyer-Vernet N, Moncuquet M, Monson S J, Mozer F S, Murphy S D, Odom J, Oliverson R, Olson J, Parker E N, Pankow D, Phan T, Quataert E, Quinn T, Ruplin S W, Salem C, Seitz D, Sheppard D A, Siy A, Stevens K, Summers D, Szabo A, Timofeeva M, Vaivads A, Velli M, Yehle A, Werthimer D, Wygant J R
Space Sciences Laboratory, University of California, Berkeley, CA, USA.
Physics Department, University of California, Berkeley, CA, USA.
Space Sci Rev. 2016 Dec;204(1-4):49-82. doi: 10.1007/s11214-016-0244-5. Epub 2016 Mar 31.
NASA's Solar Probe Plus (SPP) mission will make the first measurements of the solar corona and the birthplace of the solar wind. The FIELDS instrument suite on SPP will make direct measurements of electric and magnetic fields, the properties of plasma waves, electron density and temperature profiles, and interplanetary radio emissions, amongst other things. Here, we describe the scientific objectives targeted by the SPP/FIELDS instrument, the instrument design itself, and the instrument concept of operations and planned data products.
美国国家航空航天局的“帕克太阳探测器”（Solar Probe Plus，简称SPP）任务将首次对太阳日冕和太阳风的发源地进行测量。“帕克太阳探测器”上的“磁场、电场和波探测器”（FIELDS）仪器套件将直接测量电场和磁场、等离子体波的特性、电子密度和温度剖面以及行星际无线电发射等。在此，我们描述了“帕克太阳探测器”/“磁场、电场和波探测器”仪器所针对的科学目标、仪器设计本身以及仪器的操作概念和计划的数据产品。
Zotero 插件
