The physics of sediment transport initiation, cessation, and entrainment across aeolian and fluvial environments
Predicting the morphodynamics of sedimentary landscapes due to fluvial and aeolian flows
requires answering the following questions: Is the flow strong enough to initiate sediment …
requires answering the following questions: Is the flow strong enough to initiate sediment …
Modern Mars' geomorphological activity, driven by wind, frost, and gravity
Extensive evidence of landform-scale martian geomorphic changes has been acquired in
the last decade, and the number and range of examples of surface activity have increased …
the last decade, and the number and range of examples of surface activity have increased …
[图书][B] Geomorphology of desert dunes
N Lancaster - 2013 - taylorfrancis.com
Untitled Page 1 Page 2 GEOMORPHOLOGY OF DESERT DUNES Sand dunes cover up to a
quarter of many desert regions. Determining the factors that determine their shape, size and …
quarter of many desert regions. Determining the factors that determine their shape, size and …
An expression for the angle of repose of dry cohesive granular materials on Earth and in planetary environments
F Elekes, EJR Parteli - … of the National Academy of Sciences, 2021 - National Acad Sciences
The angle of repose—ie, the angle θ r between the sloping side of a heap of particles and
the horizontal—provides one of the most important observables characterizing the packing …
the horizontal—provides one of the most important observables characterizing the packing …
The Pluto System After New Horizons
SA Stern, WM Grundy, WB McKinnon… - Annual Review of …, 2018 - annualreviews.org
The New Horizons (NH) flyby of the Pluto–Charon binary planet and its system of four small
surrounding satellites in mid-2015 revolutionized our knowledge of this distant planet and its …
surrounding satellites in mid-2015 revolutionized our knowledge of this distant planet and its …
1I/'Oumuamua as an N2 Ice Fragment of an exo‐Pluto Surface: I. Size and Compositional Constraints
AP Jackson, SJ Desch - Journal of Geophysical Research …, 2021 - Wiley Online Library
The origin of the interstellar object 1I/'Oumuamua has defied explanation. We perform
calculations of the non‐gravitational acceleration that would be experienced by bodies …
calculations of the non‐gravitational acceleration that would be experienced by bodies …
Understanding wind-blown sand: Six vexations
DJ Sherman - Geomorphology, 2020 - Elsevier
The study of aeolian geomorphological systems over the last half century has advanced
along several important fronts, supported by developments in technologies and analytic …
along several important fronts, supported by developments in technologies and analytic …
Pluto's haze as a surface material
WM Grundy, T Bertrand, RP Binzel, MW Buie, BJ Buratti… - Icarus, 2018 - Elsevier
Pluto's atmospheric haze settles out rapidly compared with geological timescales. It needs to
be accounted for as a surface material, distinct from Pluto's icy bedrock and from the volatile …
be accounted for as a surface material, distinct from Pluto's icy bedrock and from the volatile …
Out of Order
M Berenbaum - American Entomologist, 2019 - academic.oup.com
4 American Entomologist• Spring 2019 of Streator, and... is so far the only Illinoisan and only
American to ever discover a planet... be it RESOLVED, BY THE SENATE OF THE NINETY …
American to ever discover a planet... be it RESOLVED, BY THE SENATE OF THE NINETY …
Coevolving aerodynamic and impact ripples on Earth
Wind-blown sand creates multiscale bedforms on Earth, Mars and other planetary bodies.
According to conventional wisdom, decametre-scale dunes and decimetre-scale ripples …
According to conventional wisdom, decametre-scale dunes and decimetre-scale ripples …