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L'Observatoire Midi-Pyrénées (OMP) est un Observatoire des Sciences de l’Univers (OSU) et une école interne de l’Université Toulouse III – Paul Sabatier (UT3). Il fédère les laboratoires des sciences de l’univers, de la planète et de l’environnement midi pyrénéens autour des missions de recherche, d’observation, d’enseignement, de diffusion de la culture scientifique et de coopération internationale communes aux OSU. Il constitue le noyau du Pôle « Univers, Planète, Espace, Environnement » (UPEE) de l’UT3.
Découvrir l'observatoire
Site Web : omp.eu
Dernières publications
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Yutong Zhang, Florence Sevault, Romain Pennel, Melika Baklouti. Analysis of the impact of vertical variation and temporal frequency of the chlorophyll forcing field on modelled temperature in the Mediterranean Sea and potential implications for regional climate projections. Ocean Modelling, 2025, 194, pp.102490. ⟨10.1016/j.ocemod.2024.102490⟩. ⟨hal-04895738⟩
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Gabriel Chesnoiu, Isabelle Chiapello, Nicolas Ferlay, Pierre Nabat, Marc Mallet, et al.. Regional modeling of surface solar radiation, aerosol, and cloud cover spatial variability and projections over northern France and Benelux. Atmospheric Chemistry and Physics, 2025, 25 (2), pp.1307-1331. ⟨10.5194/acp-25-1307-2025⟩. ⟨hal-04920121⟩
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Robert Schoetter, Robin James Hogan, Cyril Caliot, Valéry Masson. Coupling the urban canopy model TEB (SURFEXv9.0) with the radiation model SPARTACUS-Urbanv0.6.1 for more realistic urban radiative exchange calculation. Geoscientific Model Development, 2025, 18 (2), pp.405-431. ⟨10.5194/gmd-18-405-2025⟩. ⟨hal-04909642⟩
Fichiers déposés
15 454
Nombre de notices
10 146
Taux d'open access
71 %
Sujets
Stars rotation
Astrophysics - Astrophysics of Galaxies
Remote sensing
Astrochemistry
Galaxies active
Surveys
Modelling
Mexique
Validation
Modélisation
Trace elements
Hydrology
Radiative transfer
Cosmology observations
Modeling
Calibration
Stars activity
Entomologie
Astrophysics - Earth and Planetary Astrophysics
Classification
Sentinel-1
Changement climatique
Techniques spectroscopic
Galaxies clusters general
Insecte
Galaxies high-redshift
Climate
MISSION SMOS
Evapotranspiration
ENSO
Gale crater
Stars magnetic field
Jezero crater
Astrophysics - Solar and Stellar Astrophysics
Large-scale structure of Universe
Magnetic fields
Pyrenees
Geochemistry
TELEDETECTION
France
Convection
Stars evolution
Satellite
Cosmological parameters
Stars oscillations
ISM abundances
ISM molecules
OHM Pyrenees
Cosmic background radiation
Black hole physics
Methods numerical
SMOS
Catalogs
Irrigation
Télédétection
Climate change
Astrophysics
Hydrodynamics
Precipitation
Altimetry
Mars 2020
X-rays binaries
MODIS
Sentinel-2
Extinction
Soil
Vegetation
Biodiversity
Andes
Stars formation
Mars
Magnetic reconnection
Stars neutron
Techniques polarimetric
Polarization
Snow
Stars interiors
Galaxies ISM
Ozone
ISM clouds
Machine learning
Accretion
Dust
Agriculture
Accretion disks
Turbulence
Radar
Submillimeter ISM
Infrared ISM
Satellite altimetry
Epos-France
Soil moisture
Galaxies evolution
Cosmic rays
Papillon
Data assimilation
Solar wind
SAR
Mediterranean Sea
Methods data analysis
Répartition par domaines