When dust devils or convective vortices form they can be identified by specific meteorological parameters, a ‘signature’. If martian and terrestrial dust devil signatures are compared similarities can be identified
An important and perhaps dominant source of dust in the Martian atmosphere, dust devils play a key r...
Dust devils occur in arid climates on the Earth and ubiquitously on Mars, where they likely dominate...
Dust devils, particle-loaded vertical convective vortices found on both Earth and Mars, are charact...
We report on an extremely well characterised encounter with a terrestrial dust devil, and its compar...
Previous martian studies have provided an understanding of diurnal dust devil behaviour for Viking 2...
Dust devil data from Mars is limited by a lack of data relating to diurnal dust devil behaviour. The...
Surface-based measurements of terrestrial and martian dust devils/convective vortices provided from ...
This paper describes a method for identifying martian dust devils and convective vortices in meteoro...
Dust devils are vortex-generated phenomena which routinely occur in arid regions on both Earth and M...
Dust devils are dust-lofting vortices which routinely occur in arid regions on both Earth and Mars. ...
We present results from the first high-resolution near-surface profiles conducted on dust devil wind...
This work investigates surface dust lifting by Martian dust devils within a global-scale computer mo...
Critical to the future exploration of Mars is having a detailed understanding of the atmospheric env...
[1] Dust devils, particle-loaded vertical convective vortices found on both Earth and Mars, are char...
Over the past several decades, orbital observations of lofted dust have revealed the importance of m...
An important and perhaps dominant source of dust in the Martian atmosphere, dust devils play a key r...
Dust devils occur in arid climates on the Earth and ubiquitously on Mars, where they likely dominate...
Dust devils, particle-loaded vertical convective vortices found on both Earth and Mars, are charact...
We report on an extremely well characterised encounter with a terrestrial dust devil, and its compar...
Previous martian studies have provided an understanding of diurnal dust devil behaviour for Viking 2...
Dust devil data from Mars is limited by a lack of data relating to diurnal dust devil behaviour. The...
Surface-based measurements of terrestrial and martian dust devils/convective vortices provided from ...
This paper describes a method for identifying martian dust devils and convective vortices in meteoro...
Dust devils are vortex-generated phenomena which routinely occur in arid regions on both Earth and M...
Dust devils are dust-lofting vortices which routinely occur in arid regions on both Earth and Mars. ...
We present results from the first high-resolution near-surface profiles conducted on dust devil wind...
This work investigates surface dust lifting by Martian dust devils within a global-scale computer mo...
Critical to the future exploration of Mars is having a detailed understanding of the atmospheric env...
[1] Dust devils, particle-loaded vertical convective vortices found on both Earth and Mars, are char...
Over the past several decades, orbital observations of lofted dust have revealed the importance of m...
An important and perhaps dominant source of dust in the Martian atmosphere, dust devils play a key r...
Dust devils occur in arid climates on the Earth and ubiquitously on Mars, where they likely dominate...
Dust devils, particle-loaded vertical convective vortices found on both Earth and Mars, are charact...