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01/28/2009 - Surface modifications by winds on Earth, Mars, Venus, and Titan
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Manage episode 121133716 series 103556
Ron Greeley, Regent's Professor, Arizona State University
Windblown dunes, ripples, and erosional features are seen on Earth, Venus, and Titan, while on Mars these features are ubiquitous and reflect the dominant agent of surface modification. Although the fundamental process is similar, the environments on these planetary objects are substantially different. Simulations conducted in the Planetary Aeolian Laboratory at NASA-Ames, coupled with field work and modeling, enable analyses of wind-related features and processes on planetary surfaces.
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17 эпизодов
Архивные серии ("Канал не активен" status)
When? This feed was archived on September 13, 2022 18:20 (). Last successful fetch was on June 10, 2022 09:10 ()
Why? Канал не активен status. Нашим серверам не удалось получить доступ к каналу подкаста в течении длительного периода времени.
What now? You might be able to find a more up-to-date version using the search function. This series will no longer be checked for updates. If you believe this to be in error, please check if the publisher's feed link below is valid and contact support to request the feed be restored or if you have any other concerns about this.
Manage episode 121133716 series 103556
Ron Greeley, Regent's Professor, Arizona State University
Windblown dunes, ripples, and erosional features are seen on Earth, Venus, and Titan, while on Mars these features are ubiquitous and reflect the dominant agent of surface modification. Although the fundamental process is similar, the environments on these planetary objects are substantially different. Simulations conducted in the Planetary Aeolian Laboratory at NASA-Ames, coupled with field work and modeling, enable analyses of wind-related features and processes on planetary surfaces.
play video
17 эпизодов
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