The objective of this paper is to explore the performance of a miniature 3D spherical wind sensor for Mars atmosphere, working under extreme wind speeds, up to the Dust Devil scale. The experimental campaign has been made for winds in the range Reynolds 1000-2000, which for typical Mars conditions and the dimensions of the sensor, represent 65-130m/s wind velocities. The experimental results further confirm high-fidelity numerical simulations of the fluid dynamics and heat transfer from a sphere for Reynolds 1000-104 and Prandtl 0.7, recently published in, which indicate that it is possible to measure in this regime.Peer Reviewe
The Optical Particle Counter 'MicroMED' will be part of the ExoMars 2022 mission and aims to provide...
Direct and large-eddy numerical simulations have been performed for a heated sphere at Reynolds numb...
International audienceDust devils - convective vortices made visible by the dust and debris they ent...
The objective of this paper is to explore the performance of a miniature 3D spherical wind sensor fo...
This paper analyzes the behavior of a miniature 3D wind sensor designed for Mars atmosphere. The sen...
A novel wind speed and direction sensor designed for the atmosphere of Mars is described. It is base...
The purpose of this paper is to present the experimental results obtained with a prototype of a 4-se...
The Martian atmosphere is of great scientific interest, both because of its similarity to Earth’s at...
A major limitation in the development of wind sensors for use on Mars is the lack of suitable testin...
In this paper the most important constraints of the wind sensors for the Martian atmosphere are desc...
A wind tunnel test campaign has been conducted prior to the landing of the Exomars2016 EDM module on...
There is a need for wind sensors with high accuracy and measurement frequency for deployment on the ...
The Optical Particle Counter 'MicroMED' will be part of the ExoMars 2022 mission and aims to provide...
Direct and large-eddy numerical simulations have been performed for a heated sphere at Reynolds numb...
International audienceDust devils - convective vortices made visible by the dust and debris they ent...
The objective of this paper is to explore the performance of a miniature 3D spherical wind sensor fo...
This paper analyzes the behavior of a miniature 3D wind sensor designed for Mars atmosphere. The sen...
A novel wind speed and direction sensor designed for the atmosphere of Mars is described. It is base...
The purpose of this paper is to present the experimental results obtained with a prototype of a 4-se...
The Martian atmosphere is of great scientific interest, both because of its similarity to Earth’s at...
A major limitation in the development of wind sensors for use on Mars is the lack of suitable testin...
In this paper the most important constraints of the wind sensors for the Martian atmosphere are desc...
A wind tunnel test campaign has been conducted prior to the landing of the Exomars2016 EDM module on...
There is a need for wind sensors with high accuracy and measurement frequency for deployment on the ...
The Optical Particle Counter 'MicroMED' will be part of the ExoMars 2022 mission and aims to provide...
Direct and large-eddy numerical simulations have been performed for a heated sphere at Reynolds numb...
International audienceDust devils - convective vortices made visible by the dust and debris they ent...