Radiation environment for future human exploration on the surface of Mars: the current understanding based on MSL/RAD dose measurements
Potential deleterious health effects to astronauts induced by space radiation is one of the
most important long-term risks for human space missions, especially future planetary …
most important long-term risks for human space missions, especially future planetary …
Observations and impacts of the 10 September 2017 solar events at Mars: An overview and synthesis of the initial results
On 10 September 2017, some of the strongest solar activity occurred in association with
active region 12673 (AR2673), including an X‐class solar flare and a fast coronal mass …
active region 12673 (AR2673), including an X‐class solar flare and a fast coronal mass …
Loss of the Martian atmosphere to space: Present-day loss rates determined from MAVEN observations and integrated loss through time
Observations of the Mars upper atmosphere made from the Mars Atmosphere and Volatile
Evolution (MAVEN) spacecraft have been used to determine the loss rates of gas from the …
Evolution (MAVEN) spacecraft have been used to determine the loss rates of gas from the …
Atmospheric escape processes and planetary atmospheric evolution
The habitability of the surface of any planet is determined by a complex evolution of its
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …
CME evolution in the structured heliosphere and effects at Earth and Mars during solar minimum
The activity of the Sun alternates between a solar minimum and a solar maximum, the former
corresponding to a period of “quieter” status of the heliosphere. During solar minimum, it is …
corresponding to a period of “quieter” status of the heliosphere. During solar minimum, it is …
Statistical properties of solar wind upstream of Mars: MAVEN observations
Using the data sets of Mars Atmosphere and Volatile EvolutioN and OMNI for the period
2014 October 10–2020 February 14 and the heliocentric distance of 1–1.66 au, we …
2014 October 10–2020 February 14 and the heliocentric distance of 1–1.66 au, we …
Generic magnetic field intensity profiles of interplanetary coronal mass ejections at Mercury, Venus, and Earth from superposed epoch analyses
M Janvier, RM Winslow, S Good… - Journal of …, 2019 - Wiley Online Library
We study interplanetary coronal mass ejections (ICMEs) measured by probes at different
heliocentric distances (0.3–1 AU) to investigate the propagation of ICMEs in the inner …
heliocentric distances (0.3–1 AU) to investigate the propagation of ICMEs in the inner …
Characteristic scales of complexity and coherence within interplanetary coronal mass ejections: insights from spacecraft swarms in global heliospheric simulations
Many aspects of the 3D structure and evolution of interplanetary coronal mass ejections
(ICMEs) remain unexplained. Here, we investigate two main topics:(1) the coherence scale …
(ICMEs) remain unexplained. Here, we investigate two main topics:(1) the coherence scale …
Magnetic structure and propagation of two interacting CMEs from the Sun to Saturn
E Palmerio, T Nieves‐Chinchilla… - Journal of …, 2021 - Wiley Online Library
One of the grand challenges in heliophysics is the characterization of coronal mass ejection
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …
ICME evolution in the inner heliosphere: Invited review
ICMEs (interplanetary coronal mass ejections), the heliospheric counterparts of what is
observed with coronagraphs at the Sun as CMEs, have been the subject of intense interest …
observed with coronagraphs at the Sun as CMEs, have been the subject of intense interest …