AGU期刊一周Research Spotlight
AGU发布最新Editor's Highlight和国外工作学习机会(Jul 5~Jul 12, 2019)
时间:2019年07月12日 09:13来源:www.3522com 点击数:

Solar Properties Rival for Control of Mars's Bow Shock

While most planetary bow shocks are controlled by the solar wind, at Mars the solar EUV flux is equally important.

SOURCE: Journal of Geophysical Research: Space Physics


The EUV flux at Mars (blue curve) along with the median subsolar bow shock location at Mars, filtered by the 27-day solar rotation (red curve) and the 687-day Mars year (green curve). All lines have been plotted on a single normalized scale. Mars years and seasons are marked along the top, with Earth years along the bottom. It is seen that EUV flux and subsolar bow shock distance track each other quite well. Credit: Hall et al. [2019], Figure 2a

Every planet with an atmosphere or magnetic field has a "bow shock," a boundary at which the supersonic solar wind suddenly slows down so it can be diverted around the planet. At Earth, the main controlling factors for the location of this bow shock are properties of the solar wind, especially its speed. Mars has an atmosphere but does not have a strong internal magnetic field, so this boundary is quite close to the planet.

By examining 11 years of bow shock crossings by the Mars Express satellite, Hall et al. [2019] reveal that the solar flux of extreme ultraviolet light, the photons responsible for ionizing the planet’s upper atmosphere, is an equal contributor to the solar wind flow parameters for controlling the location of the bow shock at Mars. Properties of the solar wind are important on short time scales, but this influence is superimposed on a longer-term variation governed by the expansion of the neutral atmosphere from EUV heating and ionization.

Control of the bow shock by the solar EUV flux is completely negligible at Earth, revealing a key difference between the space environments of these two neighboring planets. This finding should to be taken into account when interpreting other observations around Mars, in particular planetary atmospheric loss to deep space.

Citation:Hall, B. E. S., SánchezCano, B., Wild, J. A., Lester, M., & Holmstrom, M. [2019]. The Martian bow shock over solar cycle 23–24 as observed by the Mars Express mission. Journal of Geophysical Research: Space Physics, 124. https://doi.org/10.1029/2018JA026404

—Mike Liemohn, Editor in Chief, JGR: Space Physics



1. Postdoctoral Research Scientist

Palisades, New York

Lamont-Doherty Earth Observatory at Columbia University


2. Postdoctoral Positions in Improving Land-Atmosphere Interactions in the GFDL Climate & Earth System

Princeton, New Jersey

Princeton University


3. Assistant Professor (tenure track) of Interactions Between Atmospheric and Earth Surface Processes

Switzerland (CH)



4. Professor/Associate Professor in Atmospheric and Space Physics

Trondheim (By) (NO)

Norwegian University of Science and Technology




地 址:北京大学廖凯原楼5层 511

邮 编:100871

电 话:010-62752344

传 真:010-62752344

邮 箱:pkuocean@pku.edu.cn

版权所有 strong>www.3522com_葡京集团-[官方网站] Copyright by ocean.pku.edu.cn @2017, All Rights Reserved.

XML 地图 | Sitemap 地图