967 citations
- J. Bertaux2 profiles15 · h 80
- B. Davidsson2 profiles14 · h 49
- G. Naletto2 profiles13 · h 58
- R. Rodrigo2 profiles13 · h 59
- C. Tubiana2 profiles12 · h 43
- D. Koschny2 profiles12 · h 53
- F. Marzari2 profiles12 · h 60
- M. Fulle2 profiles12 · h 52
- O. Groussin2 profiles12 · h 61
- S. Debei2 profiles12 · h 47
- G. Cremonese2 profiles11 · h 55
- H. Sierks2 profiles11 · h 60
- Centre National de la Recherche ScientifiqueFR91 papers
- Sorbonne UniversitéFR74 papers
- Laboratoire atmosphères, milieux, observations spatialesFR71 papers
- Université de Versailles Saint-Quentin-en-YvelinesFR61 papers
- Université Paris CitéFR51 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR38 papers
- Observatoire de ParisFR35 papers
- Université Paris-SaclayFR32 papers
- Université Paris Sciences et LettresFR26 papers
- Délégation Paris 7FR24 papers
- Laboratoire de Météorologie DynamiqueFR24 papers
- Laboratoire Interuniversitaire des Systèmes AtmosphériquesFR19 papers
12 papers · 1 filter
Dynamics of the Great Oxidation Event from a 3D photochemical-climate model
Adam Yassin Jaziri, Benjamin Charnay, Franck Selsis +2
From the Archean toward the Proterozoic, the Earth's atmosphere underwent a major shift from anoxic to oxic conditions, around 2.4 to 2.1 Gyr, known as the Great Oxidation Event (G…
Neural Fields for Fast and Scalable Interpolation of Geophysical Ocean Variables
J. Emmanuel Johnson, Redouane Lguensat, Ronan Fablet +2
Optimal Interpolation (OI) is a widely used, highly trusted algorithm for interpolation and reconstruction problems in geosciences. With the influx of more satellite missions, we h…
Saturn's atmospheric response to the large influx of ring material inferred from Cassini INMS measurements
Julianne I. Moses, Zarah L. Brown, Tommi T. Koskinen +12
During the Grand Finale stage of the Cassini mission, organic-rich ring material was discovered to be flowing into Saturn's equatorial upper atmosphere at a surprisingly large rate…
The Impact of Turbulent Vertical Mixing in the Venus Clouds on Chemical Tracers
Maxence Lefèvre, Emmanuel Marcq, Franck Lefèvre
Venus clouds host a convective layer between roughly 50 and 60 km that mixes heat, momentum, and chemical species. Observations and numerical modelling have helped to understand th…
InSight Pressure Data Recalibration, and Its Application to the Study of Long-Term Pressure Changes on Mars
L. Lange, F. Forget, D. Banfield +9
Observations of the South Polar Residual Cap suggest a possible erosion of the cap, leading to an increase of the global mass of the atmosphere. We test this assumption by making t…
Impact of the coagulation of dust particles on Mars during the 2018 global dust storm
Tanguy Bertrand, Melinda Kahre, Richard Urata +4
Coagulation of particles occurs when two particles collide and stick together. In the Martian atmosphere, dust coagulation would increase the effective particle size, as small part…