TY - JOUR
T1 - Power attenuation of Martian rovers and landers solar panels due to dust deposition
AU - Pierron, Thomas
AU - Forget, François
AU - Millour, Ehouarn
AU - Bierjon, Antoine
N1 - Publisher Copyright:
© 2024 The Authors
PY - 2024/11/15
Y1 - 2024/11/15
N2 - Because of the high amount of dust in the Martian atmosphere, solar panels of landers and rovers on Mars get covered by dust in the course of their mission. This accumulation significantly decreases the available power over sols. During some missions, winds were able to blow the dust away. These ”dust cleaning events”, as they are called, were followed by an increase of the electrical current produced by the solar arrays. However, the Insight Lander solar panels were never cleaned and the mission died of dust accumulation. In order to better predict the evolution of available power produced by solar panels in the Martian conditions, this paper proposes a model of dust accumulation in which the solar flux under the accumulated dust layer is computed taking into account a full radiative transfer in the atmosphere and in the dust layer accumulated on the panel. This work uses several missions observation data to validate this model.
AB - Because of the high amount of dust in the Martian atmosphere, solar panels of landers and rovers on Mars get covered by dust in the course of their mission. This accumulation significantly decreases the available power over sols. During some missions, winds were able to blow the dust away. These ”dust cleaning events”, as they are called, were followed by an increase of the electrical current produced by the solar arrays. However, the Insight Lander solar panels were never cleaned and the mission died of dust accumulation. In order to better predict the evolution of available power produced by solar panels in the Martian conditions, this paper proposes a model of dust accumulation in which the solar flux under the accumulated dust layer is computed taking into account a full radiative transfer in the atmosphere and in the dust layer accumulated on the panel. This work uses several missions observation data to validate this model.
U2 - 10.1016/j.pss.2024.105985
DO - 10.1016/j.pss.2024.105985
M3 - Article
AN - SCOPUS:85207596599
SN - 0032-0633
VL - 253
JO - Planetary and Space Science
JF - Planetary and Space Science
M1 - 105985
ER -