2. 您的位置
3. 首页
4. 会议论文
5. The Mars Upper Atmosphere from MAVEN

The Mars Upper Atmosphere from MAVEN

来源 :第二届北京月球与深空探测国际论坛 | 被引量 : 0次 | 上传用户：shuijing0328

【摘 要】

：

The MAVEN spacecraft achieved orbit around Mars on 21 September 2014 and has been gather data in the primary science mission since 18 November 2014.It elliptical orbit takes MAVEN through the Mars atm

【作 者】

：

Roger Yelle 

【机 构】

：

University of Arizona, and the MAVEN Team

【出 处】

：

第二届北京月球与深空探测国际论坛

【发表日期】

：

2015年3期

下载到本地 , 更方便阅读

下载此文 赞助VIP

声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架

论文部分内容阅读

　　The MAVEN spacecraft achieved orbit around Mars on 21 September 2014 and has been gather data in the primary science mission since 18 November 2014.It elliptical orbit takes MAVEN through the Mars atmosphere at altitudes as low as 135 km.

其他文献

Lunar-based Ultraviolet Telescope Study of the Well-known Algol-type Binary TW Dra

By using the Lunar-based Ultraviolet Telescope (LUT) from 2 December to 4 December, 2014, the first near-UV light curve of the well-known Algol-type binary TW Dra is reported.We analyze light curve wi

会议

stars:binaries:closestars:binaries:eclipsingstars:individual(TW Draco)

Lunar Magmatism Lasted Longer than Expected

After giant impact, the Moon experienced a stage referred to as Lunar Magma Ocean (LMO), which fractionally crystallized into Mg-Fe-rich mantle and anorthite-predominant highland.

会议

Comprehensive analysis of the Lunar Orientale Basin and research of impact condition

Orientale Basin is the youngest multi-ring basin on the moon crater, so it can provide theoretical reference for the research of more early lunar impact basin.Previously, although there is now a lot o

会议

Lunar Orientale Basinmulti-source dataanalysis by synthesisoblique impact

Analytic relation between total solar irradiation and the temperature of sub-surface lunar regolith

The total solar irradiation (TSI) will cause the change of the temperature of lunar sub-surface regolith (TLSR).Therefore, TLSR contains the information of TSI.In this paper, a simple model dealing wi

会议

Mars orbit optical remote sensor: high and medium resolution integration stereo camera

The high and medium resolution integration stereo camera (HiMERISC) is a two-component system (one high-resolution and one medium-resolution camera), designed to take synoptic stereo mapping of the su

会议

Mapping FeO and TiO2 Abundances of Lunar Regolith with CELMS Data using BPNN Method

Accurate knowledge of the diversity and distribution of the FeO and TiO2 abundances (FTAs) on the lunar surface is of essential importance to investigate the origin and geologic evolution of the Moon.

会议

BPNNCELMS datasurface roughnessslopeFeO and TiO2abundances

Retrieve and validate the geocentric position from extreme ultraviolet images of the Chang'E-3

388 Extreme ultraviolet (EUV) images, which were obtained from December 24, 2013 to May 20, 2014 by the EUV Camera (EUVC) on board the Chinese ChangE-3 lander mission, have been calibrated and release

会议

Chang'E-3Extreme ultravioletgeocentric position

Lunar Radio Ranging and Preliminary Result from CE-3 Mission

Radio science experiments have been involved in all of the Chinese lunar missions with different research objectives.In ChangE-3 landing mission, a 2-and 3-way lunar radio total-count-phase ranging an

会议

Lunar RangingRadio PhaseChang'E-3lander

First View of Close Binaries from Our Moon

The lander of Chinas Change 3 spacecraft was equipped with a 15-cm telescope that is used to monitor celestial objects in the near-UV band (245nm-340nm).The Lunar-based Ultraviolet Telescope (LUT) is

会议

Space vehicles:Lunar-based Ultraviolet Telescopebinaries:closebinaries:eclipsi

Impact Metamorphism And Breakup Events Of Asteroids: Clues From H and L Chondrites

Shock features and noble gas signatures in ordinary chondrites (OCs) provide essential clues to decipher impact and thermal histories of their parent bodies.

会议

Asteroidschondritesshock effectsmetamorphismnoblegasgas retension agescosm