MEX-M-MRS-1-2-3-PRM-0275
收藏esdcdoi.esac.esa.int2025-01-22 收录
下载链接:
http://esdcdoi.esac.esa.int/doi/html/data/planetary/MARS-EXPRESS/MEX-M-MRS-1-2-3-PRM-0275.html
下载链接
链接失效反馈官方服务:
资源简介:
Data Set Overview The Mars Express (MEX) Radio Science (MaRS) Data Archive is a timeordered collection of raw and partially processed data collected during the MEX Mission to Mars. For more information on the investigations proposed see the MaRS User Manual MARSUSERMANUAL2004 in the MaRS DOCUMENT/MRS_DOC folder. This is a Target Gravity measurement covering the time 20050118T05:20:31.000 to 20050118T23:42:43.000. This data set was collected during the MEX Mission Prime Mission Phase (PRM) 20042005. This is a Target Gravity on Mars. These kind of measurements were typically conducted during Mars Express pericenter over interesting geophysical structures like Tempe Fossae or Olympus Mons. This particular measurement was conducted over Tempe Fossae. There were three types of scientific measurements conducted during PRM: Occultation, Bistatic Radar and Gravity where one has to distinguish between global gravity measurements which were conducted around apocenter and target gravity measurements which were conducted around pericenter over interesting geophysical structures. For more information see INST.CAT or the MaRS User Manual MARSUSERMANUAL2004. For all measurements if not indicated otherwise Transponder 1 onboard the s/c was used. Transponder 2 is designed to be a backup. Mission Phase Definition It should be noted that the Mars Express (MEX) Radio Science (MaRS) group uses mission phases which deviate from the ones defined in the MISSION.CAT files given by ESA in order to keep the keywords and abbreviations consistent for Mars Express, Venus Express and Rosetta. Those mission phase abbreviations are also used in the data description field of the dataset_id. MaRS mission name | abbreviation | time span Near Earth Verification | NEV | 20030602 20030731 truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]
数据集概览:火星快车号(MEX)无线电科学(MaRS)数据档案系按照时间顺序排列的原始及部分处理数据集合,这些数据是在火星快车号任务期间收集的。有关拟进行的调查信息,请参阅MaRS用户手册MARSUSERMANUAL2004,位于MaRS文档/MRS_DOC文件夹中。本数据集为针对目标重力测量,覆盖时间范围20050118T05:20:31.000至20050118T23:42:43.000。该数据集是在火星快车号任务初级阶段(PRM)20042005期间收集的。这是对火星上的目标重力进行的测量。此类测量通常在火星快车号经过有趣的地貌结构(如提梅斯峡谷或奥林帕斯山)的近地点时进行。这次特定测量是在提梅斯峡谷进行的。在PRM期间进行了三种类型的科学测量:掩星、双站雷达和重力测量。其中,需区分全球重力测量(在远地点附近进行)和针对有趣的地貌结构的近地点目标重力测量。更多信息请参阅INST.CAT或MaRS用户手册MARSUSERMANUAL2004。除非另有说明,否则所有测量均使用搭载于卫星上的应答器1进行。应答器2设计为备用。任务阶段定义:值得注意的是,火星快车号(MEX)无线电科学(MaRS)小组使用的任务阶段与ESA提供的MISSION.CAT文件中定义的任务阶段不同,以保持火星快车号、金星快车号和罗塞塔号的术语和缩写的一致性。这些任务阶段缩写也用于dataset_id的数据描述字段中。MaRS任务名称 | 缩写 | 时间范围
近地验证 | NEV | 20030602 20030731 截断!请参阅实际数据以获取全文 [截断!请参阅实际数据以获取全文]
提供机构:
European Space Agency



