Dust devil height and spacing with relation to the martian planetary boundary layer thickness

Author:

Fenton Lori K.,Lorenz Ralph

Funder

MFRP

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference72 articles.

1. Vertical profiling of convective dust plumes in southern Morocco during SAMUM;Ansmann;Tellus B,2009

2. Bell, F., 1969. Dust Devils and Aviation, Report. Meteorol. Note 27. Aust. Bur. of Meteorol., Melbourne, Victoria.

3. Martian dynamical phenomena during June–November 1976: Viking Orbiter imaging results;Briggs;J. Geophys. Res.,1977

4. Mars Orbiter Camera observations of Martian dust devils and their tracks (September 1997 to January 2006) and evaluation of theoretical vortex models;Cantor;J. Geophys. Res.,2006

5. Atmospheric vorticity and dust devil rotation;Carroll;J. Geophys. Res.,1970

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