HIGHLIGHTS
SUMMARY
Acoustic signals of grain impacts recorded during the vortex encounter provide quantitative information about the number density of pArticles in the vortex. This chance dust devil encounter demonstrates the potential of acoustic data for resolving the rapid wind structure of the Martian atmosphere and for directly quantifying wind-blown grain fluxes on Mars. The PBL plays an important role in the mixing of heat, momentum, dust, and chemical species10. Nature Communications | 13:7505 Infrared Sensor (TIRS), e the wind direction and f the wind speed as measured by the MEDA wind sensors, g the . . .
If you want to have access to all the content you need to log in!
Thanks :)
If you don't have an account, you can create one here.