258 citations · 1.3k across the 43 of their papers we have counts for
6 papers · 1 filter
Observations and numerical modelling of a convective disturbance in a large-scale cyclone in Jupiter's South Temperate Belt
P. Iñurrigarro, R. Hueso, J. Legarreta +8
Moist convective storms in Jupiter develop frequently and can trigger atmospheric activity of different scales, from localized storms to planetary-scale disturbances including conv…
Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
J. F. Sanz-Requena, S. Perez-Hoyos, A. Sanchez-Lavega +2
In this paper we present a study of the vertical haze and cloud structure over a triple vortex in Saturn's atmosphere in the planetographic latitude range 55N-69N (del Rio- Gaztelu…
New cloud morphologies discovered on the Venus's night during Akatsuki
J. Peralta, A. Sánchez-Lavega, T. Horinouchi +8
During the years 2016 to 2018, the instruments Akatsuki/IR2 (JAXA) and IRTF/SpeX (NASA) acquired a large set of images at 1.74, 2.26 and 2.32 μm to study the nightside mid-to-lower…
Characterisation of Martian dust aerosol phase function from sky radiance measurements by MSL engineering cameras
H. Chen-Chen, S. Perez-Hoyos, A. Sanchez-Lavega
Dust is the main driver of Mars' atmospheric variability. The determination of Martian dust aerosol properties is of high relevance for radiative modelling and calculating its weat…
Dust particle size and optical depth on Mars retrieved by the MSL Navigation Cameras
H. Chen-Chen, S. Perez-Hoyos, A. Sanchez-Lavega
In this paper we show that Sun-viewing images obtained by the Mars Science Laboratory (MSL) Navigation Cameras (Navcam) can be used for retrieving the dust optical depth and constr…
Morphology and dynamics of Venus's middle clouds with Akatsuki/IR1
J. Peralta, N. Iwagami, Sánchez-Lavega +8
The Venusian atmosphere is covered by clouds with super-rotating winds whose accelerating mechanism is still not well understood. The fastest winds, occurring at the cloud tops ($\…