Over the years, wavelet-based analyses have been responsible for remarkable
achievements in physics and related sciences. Nevertheless, a deep inspection on wavelet …

This review describes the principles and summarizes the challenges of analytical methods
based on optical emission spectroscopy (OES) in space applications, with a particular focus …

Perseverance's Mastcam-Z instrument provides high-resolution stereo and multispectral
images with a unique combination of spatial resolution, spatial coverage, and wavelength …

Rovers and landers on Mars have experienced local, regional, and planetary‐scale dust
storms. However, in situ documentation of active lifting within storms has remained elusive …

Abstract The Mars Environmental Dynamics Analyzer instrument on Mars 2020 has five
Atmospheric Temperature Sensors at two altitudes (0.84 and 1.45 m) plus a Thermal …

As the largest basin on Mars, Utopia Planitia has both experienced and recorded variations
of the Martian palaeoclimate. Layered subsurface structures have been identified by ground …

The number density of impact craters on a planetary surface is used to determine its age,
which requires a model for the production rate of craters of different sizes. On Mars …

Dust devils (convective vortices loaded with dust) are common at the surface of Mars,
particularly at Jezero crater, the landing site of the Perseverance rover. They are indicators …

Barometers floating on high‐altitude balloons in the relatively clement cloud layer on Venus
could detect and characterize acoustic waves generated by seismic activity, avoiding the …

Acoustics is new on Mars: it allows the characterization of turbulence at smaller scales than
previously possible within the lowest part of the Planetary Boundary Layer. Sound speed …