火星快车-ExoMars 痕量气体轨道器相互射电掩星的首批结果

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Radio Science Pub Date : 2024-07-01 DOI:10.1029/2023RS007873
Jacob Parrott;Håkan Svedhem;Olivier Witasse;Colin Wilson;Ingo Müller-Wodarg;Alejandro Cardesín-Moinelo;Peter Schmitz;James Godfrey;Olivier Reboud;Bernhard Geiger;Beatriz Sánchez-Cano;Bruno Nava;Yenca Migoya-Orué
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引用次数: 0

摘要

火星快车(MEX)和痕量气体轨道器(TGO)之间正在火星上进行航天器对航天器的无线电掩星实验,这是首次在地球以外的行星上进行广泛的航天器间掩星实验。我们在此介绍 2020 年 11 月 2 日至 2023 年 7 月 5 日期间进行的首批 83 次此类掩星观测的结果。迄今为止,其中 44 次观测提取了垂直电子密度剖面图。这些观测是欧洲航天局进行的一项重要可行性研究的成功结果,该研究旨在利用已有的中继通信设备进行无线电科学研究。与传统的航天器对地面站掩星相比,无线电相互掩星具有许多优势。在这项工作中,我们展示了如何将原始数据转化为电子密度值,并通过模型和其他仪器进行验证。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
First results of Mars Express—ExoMars trace gas orbiter mutual radio occultation
Spacecraft-to-spacecraft radio occultations experiments are being conducted at Mars between Mars Express (MEX) and Trace Gas Orbiter (TGO), the first ever extensive inter-spacecraft occultations at a planet other than Earth. Here we present results from the first 83 such occultations, conducted between 2 Nov 2020 and 5th of July 2023. Of these, 44 observations have to-date resulted in the extraction of vertical electron density profiles. These observations are the successful results of a major feasibility study conducted by the European Space Agency to use pre-existing relay communication equipment for radio science purposes. Mutual radio occultations have numerous advantages over traditional spacecraft-to-ground station occultations. In this work, we demonstrate how raw data are transformed into electron density values and validated with models and other instruments.
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来源期刊
Radio Science
Radio Science 工程技术-地球化学与地球物理
CiteScore
3.30
自引率
12.50%
发文量
112
审稿时长
1 months
期刊介绍: Radio Science (RDS) publishes original scientific contributions on radio-frequency electromagnetic-propagation and its applications. Contributions covering measurement, modelling, prediction and forecasting techniques pertinent to fields and waves - including antennas, signals and systems, the terrestrial and space environment and radio propagation problems in radio astronomy - are welcome. Contributions may address propagation through, interaction with, and remote sensing of structures, geophysical media, plasmas, and materials, as well as the application of radio frequency electromagnetic techniques to remote sensing of the Earth and other bodies in the solar system.
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