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C. Beule, G. Wurm, T. Kelling, Marc Koester, M. Kocifaj (2015)
An Insolation Activated Dust Layer on MarsIcarus, 260
S. Vet, J. Merrison, M. Mittelmeijer-Hazeleger, E. Loon, L. Cammeraat (2014)
Effects of rolling on wind-induced detachment thresholds of volcanic glass on MarsPlanetary and Space Science, 103
T. Lopez, R. Antoine, D. Baratoux, M. Rabinowicz, K. Kurita, L. D'Uston (2012)
Thermal anomalies on pit craters and sinuous rilles of Arsia Mons: Possible signatures of atmospheric gas circulation in the volcanoJournal of Geophysical Research, 117
P. Whelley, R. Greeley (2008)
The distribution of dust devil activity on MarsJournal of Geophysical Research, 113
M. Kocifaj, J. Klačka, T. Kelling, G. Wurm (2011)
Radiative cooling within illuminated layers of dust on (pre)-planetary surfaces and its effect on dust ejectionIcarus, 211
B. Cantor (2007)
MOC observations of the 2001 Mars planet-encircling dust stormIcarus, 186
L. Montabone, L. Montabone, L. Montabone, F. Forget, E. Millour, R. Wilson, S. Lewis, B. Cantor, D. Kass, A. Kleinboehl, M. Lemmon, M. Smith, M. Wolff (2014)
Eight-year climatology of dust optical depth on MarsIcarus, 251
E. Muntz, Y. Sone, K. Aoki, S. Vargo, M. Young (2002)
Performance analysis and optimization considerations for a Knudsen compressor in transitional flowJournal of Vacuum Science and Technology, 20
J. Merrison (2012)
Sand transport, erosion and granular electrificationAeolian Research, 4
M. Kahre, S. Vines, R. Haberle, J. Hollingsworth (2013)
The early Martian atmosphere: Investigating the role of the dust cycle in the possible maintenance of two stable climate statesJournal of Geophysical Research: Planets, 118
T. Kelling, G. Wurm, C. Dürmann (2011)
Ice particles trapped by temperature gradients at mbar pressure.The Review of scientific instruments, 82 11
G. Paraskov, G. Wurm, O. Krauss (2006)
Eolian Erosion of Dusty Bodies in Protoplanetary DisksThe Astrophysical Journal, 648
T. Kelling, G. Wurm, M. Kocifaj, J. Klačka, D. Reiss (2011)
Dust ejection from planetary bodies by temperature gradients: Laboratory experimentsIcarus, 212
M. Balme, A. Hagermann (2006)
Particle lifting at the soil‐air interface by atmospheric pressure excursions in dust devilsGeophysical Research Letters, 33
R. Greeley, R. Leach, B. White, J. Iversen, J. Pollack (1980)
Threshold windspeeds for sand on Mars: Wind tunnel simulationsGeophysical Research Letters, 7
J. Merrison, H. Gunnlaugsson, P. Nørnberg, A. Jensen, K. Rasmussen (2007)
Determination of the wind induced detachment threshold for granular material on Mars using wind tunnel simulationsIcarus, 191
G. Peters, W. Abbey, G. Bearman, G. Mungas, J. Smith, R. Anderson, S. Douglas, L. Beegle (2008)
Mojave Mars simulant—Characterization of a new geologic Mars analogIcarus, 197
D. Rader (1990)
Momentum slip correction factor for small particles in nine common gasesJournal of Aerosol Science, 21
G. Wurm, O. Krauss (2006)
Dust eruptions by photophoresis and solid state greenhouse effects.Physical review letters, 96 13
R. Antoine, T. Lopez, D. Baratoux, M. Rabinowicz, K. Kurita (2011)
Thermal analysis of fractures at Cerberus Fossae, Mars: Detection of air convection in the porous debris apronIcarus, 214
A. Fedorova, F. Montmessin, A. Rodin, O. Korablev, A. Määttänen, L. Maltagliati, J. Bertaux (2014)
Evidence for a bimodal size distribution for the suspended aerosol particles on MarsIcarus, 231
C. Beule, G. Wurm, T. Kelling, M. Küpper, T. Jankowski, J. Teiser (2013)
The martian soil as a planetary gas pumpNature Physics, 10
M. Knudsen
Eine Revision der Gleichgewichtsbedingung der Gase. Thermische MolekularströmungAnnalen der Physik, 336
Y. Sone, E. Itakura (1990)
Analysis of Poiseuille and thermal transpiration flows for arbitrary Knudsen numbers by a modified Knudsen number expansion method and their database.Shinku, 33
H. Singh
Dust Eruptions
J. Kok, N. Rennó (2006)
Enhancement of the emission of mineral dust aerosols by electric forcesGeophysical Research Letters, 33
L. Neakrase, R. Greeley (2010)
Dust devil sediment flux on Earth and Mars: Laboratory simulationsIcarus, 206
J. Kok (2010)
Difference in the wind speeds required for initiation versus continuation of sand transport on mars: implications for dunes and dust storms.Physical review letters, 104 7
Nathan Bridges, F. Ayoub, J. Avouac, S. Leprince, Antoine Lucas, Sarah Mattson (2012)
Earth-like sand fluxes on MarsNature, 485
G. Wurm, J. Teiser, D. Reiss (2008)
Greenhouse and thermophoretic effects in dust layers: The missing link for lifting of dust on MarsGeophysical Research Letters, 35
In this work we present laboratory measurements on the reduction of the threshold friction velocity necessary for lifting dust if the dust bed is illuminated. Insolation of a porous soil establishes a temperature gradient. At low ambient pressure this gradient leads to thermal creep gas flow within the soil. This flow leads to a subsurface overpressure which supports lift imposed by wind. The wind tunnel was run with Mojave Mars Simulant and air at 3, 6, and 9mbar, to cover most of the pressure range at Martian surface levels. Our first measurements imply that the insolation of the Martian surface can reduce the entrainment threshold velocity between 4% and 19% for the conditions sampled with our experiments. An insolation activated soil might therefore provide additional support for aeolian particle transport at low wind speeds.
Journal of Geophysical Research: Planets – Wiley
Published: Jul 1, 2015
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