On aeolian transport: Grain-scale interactions, dynamical mechanisms and scaling laws
By Orencio Durán, P. Claudin, Bruno Andreotti. 2011
301 citations recorded by the source corpus.
Subfields: Earth-Surface Processes, Ocean Engineering, Soil Science
View Paper: https://www.semanticscholar.org/paper/ccaec4011ca1e461b3b434ad8e852a636a5d1795
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Earth-Surface Processes
- Orencio Durán
- Thomas Pahtz
- Abram H. Clark
- Manousos Valyrakis
- J. Kok
- G. Varga
- Eric J. R. Parteli
- G. Újvári
In Ocean Engineering
- Orencio Durán
- J. Kok
- Thomas Pahtz
- Manousos Valyrakis
- Abram H. Clark
- G. Varga
- Eric J. R. Parteli
- G. Újvári
In Soil Science
- Orencio Durán
- Thomas Pahtz
- Abram H. Clark
- Manousos Valyrakis
- J. Kok
- Eric J. R. Parteli
- T. Michaels
- D. Karam
Citations in the corpus
- An improved dust emission model – Part 1: Model description and comparison against measurements (2014, background): “In particular, the soil’s saltation threshold sets the wind speed in the near-surface layer (Bagnold, 1941), which in turn determines the particle speed (Duran et al., 2011; Kok et al., 2012).”
- The Physics of Sediment Transport Initiation, Cessation, and Entrainment Across Aeolian and Fluvial Environments (2020, methodology): “This behavior is a signature of the fact that the transport layer, in general, consists of different species of particles with different characteristic velocities [e.g., Durán et al., 2011, Figure 21].”
- The physics of wind-blown loess: Implications for grain size proxy interpretations in Quaternary paleoclimate studies (2016, methodology): “Impaction dominates for particles in the size range of Dp = ~3–5 to 50 μm (Raupach and Lu, 2004), while above 50 μm gravitational settling is the dominant dry deposition mechanism (Fig.”
- The physics of wind-blown sand and dust (2012, methodology): “This yields L/ v = CDKu∗it /g, such that the mass flux can be approximated by (Kok and Renno 2007, Durán et al 2011a) QDK = CDK ρa g u∗it (u 2 ∗ − u2∗it ).”