D Reiss, L Fenton, L Neakrase, M Zimmerman… - Space Science …, 2016 - Springer
Dust devils that leave dark-or light-toned tracks are common on Mars and they can also be found on the Earth's surface. Dust devil tracks (hereinafter DDTs) are ephemeral surface …
Over the past several decades, orbital observations of lofted dust have revealed the importance of mineral aerosols as a climate forcing mechanism on both Earth and Mars …
The impact of dust aerosols on the climate and environment of Earth and Mars is complex and forms a major area of research. A difficulty arises in estimating the contribution of small …
J Bullard, M Baddock - Aeolian geomorphology: A new …, 2019 - Wiley Online Library
This chapter focuses on dust sediments, sources, entrainment, and transport. The particle size of emitted dust depends on both the characteristics of the source area and the …
D Reiss, MI Zimmerman, DC Lewellen - Earth and Planetary Science …, 2013 - Elsevier
Aeolian processes are the most active processes modifying the surface of Mars under present day climatic conditions. Besides wind streak changes and dune and ripple …
During field work at the Ibn Battuta Mars analogue sites, two research questions were analyzed:(1) How do we identify sampling sites using remote and local imaging and (2) what …
Studying dust devils is important to better understand Mars climate and resurfacing phenomena. This paper presents an automated approach to calculate the width of tracks in …
AC Sparavigna - arXiv preprint arXiv:1112.5572, 2011 - arxiv.org
In several desert areas, the slow motion of sand dunes can be a challenge for modern human activities and a threat for the survival of ancient places or archaeological sites …