Difference between revisions of "Dust storms"
| Line 4: | Line 4: | ||
==Frequency== | ==Frequency== | ||
| − | Local and global dust storms happen fairly frequently on Mars. | + | Local and global dust storms happen fairly frequently on Mars. Planet wide encircling dust storms have a frequency of about once every three years. Practically all large martian dust storms happen during the latter, warmer part of the martian year<ref>https://oro.open.ac.uk/36468/1/Mulholland-Interannual-2.pdf</ref>. Most storms initiate from the southern part of the planet, mainly from the Hellas basin and the Acidalia/Chryse regions. |
==Opacity== | ==Opacity== | ||
| − | The opacity of the martian atmosphere during a dust storm is an important parameter to evaluate the degradation of performance of solar powered equipment on Mars. The duration of dust storms also affect the required [[energy storage]] and the energy management strategies of the settlement. | + | The opacity of the martian atmosphere during a dust storm is an important parameter to evaluate the degradation of performance of solar powered equipment on Mars. The duration of dust storms also affect the required [[energy storage]] and the energy management strategies of the settlement. Even during the most severe dust storms, illumination does not drop more than 60%.<ref>http://www.marspapers.org/paper/MAR98058.pdf</ref> This means that a settlement operating uniquely on photoelectric Solar energy would be able to maintain itself by shutting down some of its more energy intensive operations during the storm. |
{{stub}} | {{stub}} | ||
Revision as of 13:51, 18 April 2019
Dust storms on Mars cover large areas and can last more than a month.
The low density of the martian atmosphere precludes the spectacular effects described in the film 'The Martian'. However dust storms on Mars are significant events that must be taken into account for planing a functional settlement.
Frequency
Local and global dust storms happen fairly frequently on Mars. Planet wide encircling dust storms have a frequency of about once every three years. Practically all large martian dust storms happen during the latter, warmer part of the martian year[1]. Most storms initiate from the southern part of the planet, mainly from the Hellas basin and the Acidalia/Chryse regions.
Opacity
The opacity of the martian atmosphere during a dust storm is an important parameter to evaluate the degradation of performance of solar powered equipment on Mars. The duration of dust storms also affect the required energy storage and the energy management strategies of the settlement. Even during the most severe dust storms, illumination does not drop more than 60%.[2] This means that a settlement operating uniquely on photoelectric Solar energy would be able to maintain itself by shutting down some of its more energy intensive operations during the storm.
| This article is a stub. You can help Marspedia by expanding it. |
