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Автор Thomas, P.
Автор Veverka, J.
Дата выпуска 1979
dc.description Viking orbiter observations extending over 1 Martian year have been used in conjunction with Mariner 9 data obtained in 1971–1972 to study the seasonal and secular behavior of several kinds of wind streaks. Most bright streaks, inferred to consist of dust storm fallout in the lees of obstacles, have changed very little in form or orientation over a period of 3 Martian years. Some are extremely stable and have experienced no effective eolian action over the 3 years. A few bright streaks changed rapidly during global dust storms; these streaks are located in areas subject to both global and topographic winds. Viking images have shown for the first time that dark, erosional streaks are stable from the time of their formation after major dust storms until the onset of the next episode of major storm activity. Available evidence shows that the large, dark streaks in Oxia Palus consist of material deflated from dune fields within the associated craters. These streaks lengthened secularly since 1972; changes appear to occur episodically during southern summer. The great majority of all streaks reflect winds during the period from late southern spring to early southern fall, although some changes occur throughout the year. The global pattern of wind streaks and the variability of the streaks thus depend strongly upon the current south‐north asymmetry of seasons on Mars.
Формат application.pdf
Копирайт Copyright 1979 by the American Geophysical Union.
Тема Proceedings of the Second International Colloquium on Mars
Тема PLANETARY SCIENCES: SOLID SURFACE PLANETS
Тема Planetology: Atmospheres of planets
Тема Planetology: Surfaces of planets
Название Seasonal and secular variation of wind streaks on Mars: An analysis of Mariner 9 and Viking data
Тип article
DOI 10.1029/JB084iB14p08131
Electronic ISSN 2156-2202
Print ISSN 0148-0227
Журнал Journal of Geophysical Research: Solid Earth
Том 84
Первая страница 8131
Последняя страница 8146
Выпуск B14
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