HelioWebG. Bellucci
flowchart
A[G. Bellucci]
AC["Associated Concepts (22)"]
AW["Authored Works (24)"]
CA["Linked Co-Authors (4)"]
CI["Linked Collaborating Institutions (54)"]
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click AW "#authored-works"
click CA "#co-authors"
click CI "#collaborating-institutions"
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- ORCiD
- https://orcid.org/0000-0003-0867-8679
- OpenAlex ID
- https://openalex.org/A5019815694 (API record)
Associated Concepts [?]
- Physics
- Astronomy
- Biology
- Geology
- Astrobiology
- Geography
- Remote sensing
- Quantum mechanics
- Astrophysics
- Engineering
- Computer science
- Optics
- Aerospace engineering
- Environmental science
- Chemistry
- Mars Exploration Program
- Meteorology
- Planet
- Organic chemistry
- Saturn
- Atmospheric sciences
- Martian
Authored Works
sorted by decreasing year, and then by display-name
- Martian Atmospheric H<SUB>2</SUB>O Vapor with Trace Gas Orbiter's NOMAD/LNO
- Mars Atmospheric Loss is Enhanced by Lower Atmospheric Dynamics, Including Regional Dust Storms
- Climatology of Carbon Monoxide on Mars as Observed by NOMAD
- Impact of the 2018 global dust storm on Mars atmosphere composition as observed by NOMAD on ExoMars Trace Gas Orbiter
- The ExoMars 2016 Trace Gas Orbiter NOMAD Spectrometer Suite for Nadir, Limb and Solar Occultation Measurements of Mars' Atmosphere
- VIS-NIR Spectrophotometric Study of the Saturnian icy Satellites by Cassini-VIMS
- Surface-Atmospheric Separation Models for Titan: Plane Parallel vs. Spherical Shell Radiative Transfer Solutions for Cassini VIMS Data
- OMEGA Mars Express: Water Vapour Daily Variability on the South Pole
- Spectral affinities in the icy moons of Saturn investigated through the G-mode multivariate classification method
- Saturn's Titan: Evidence for Surface Reflectance Change: Implications for Atmospheric and Volcanic Activity
- Full-disk observations of the saturnian moons in the VIS-NIR spectral range by Cassini- VIMS
- The Depths of Saturn Revealed: Discrete Cloud Systems and Winds at the 2-Bar Level as Imaged by Cassini/VIMS
- The Cassini VIMS Titan Photometric Control Network: Relevance to Understanding Titan's Surface and Atmosphere
- Spring Sublimation of the Seasonal Condensates on Mars from Omega/Mars Express
- Physical Properties of the Saturnian Ring System Inferred from Cassini VIMS Opposition Observations
- Ice Grain Size Distribution: Differences Between Jovian and Saturnian Icy Satellites From Galileo and Cassini Measurements
- Evidence for Enhanced Hydration and Water Ice Stability at Tropical Latitudes on Mars
- Coordinated Analysis of Mars Express OMEGA Hyperspectral Imaging and Mars Exploration Rover Traverse Data for Meridiani Planum
- Compositional Units on the Mars Surface From the Mars Express HRSC Color Imagery
- Compositional Mapping of Surfaces in the Saturn System with Cassini VIMS: the Role of Water, Cyanide Compounds and Carbon Dioxide
- Titan's Surface Seen by VIMS/Cassini
- The Surface Composition of Saturn's Moon Phoebe As seen by the Cassini Visual and Infrared Mapping Spectrometer
- Spectral Imaging of Saturn by Cassini/VIMS: Early Science Results
- Galilean Satellite Surface Composition: New Cassini VIMS Observations and Comparison With Galileo NIMS Measurements
Linked Co-Authors
Linked Collaborating Institutions
- American University, Washington DC
- Arizona State University, Department of Geological Sciences
- Belgian Institute for Space Aeronomy
- Boston University, Massachusetts
- California Institute of Technology, Division of Geological and Planetary Sciences
- Centre National de la Recherche Scientifique, Toulouse
- Cornell University, Department of Astronomy/Center for Radiophysics and Space Research
- Cornell University, New York
- Free University of Berlin, Department of Geosciences
- German Aerospace Center, Berlin
- Hampton University, Department of Atmospheric and Planetary Science
- Helmholtz Institute for Planetary Research, Berlin
- Institut d'Astrophysique Spatiale
- Institute of Astrophysics of Andalusia
- Italian National Institute of Astrophysics
- Jet Propulsion Laboratory
- Johns Hopkins University, Applied Physics Laboratory
- MIT, Department of Earth and Planetary Science
- Max-Planck-Institute for Solar System Research, Lindau
- Mount San Antonio College, California
- NASA Ames Research Center
- NASA Goddard Space Flight Center, Maryland
- NASA Johnson Space Center
- Observatoire de Paris, Departement de Recherche Spatiale
- Observatoire de Paris, France
- Open University Milton Keynes, UK
- Open University, Department of Physical Sciences
- Parthenope University of Naples, Italy
- Paul Scherrer Institute, Switzerland
- Planetary Science Institute, Arizona
- RAS, Space Research Institute, Moscow
- Royal Observatory of Belgium
- Space Science Institute, Colorado
- U.S. Geological Survey, Colorado
- U.S. Geological Survey, Flagstaff
- Universite Paris Sud (Paris XI), France
- Universite de Nantes, France
- Universite de Nantes, Laboratoire de Planetologie et de Geodynamique
- University of Arizona
- University of Arizona, Department of Astronomy and Steward Observatory
- University of Arizona, Department of Planetary Sciences
- University of Colorado, Boulder
- University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics
- University of Hawaii, Manoa, School of Earth and Ocean Sciences
- University of Lisbon, Astrophysical Institute
- University of Mainz, Faculty of Chemistry
- University of Oulu, Department of Physics
- University of Oxford, Department of Physics
- University of Oxford, UK
- University of Pittsburgh, Department of Geology and Planetary Sciences
- University of Pittsburgh, Pennsylvania
- University of Washington, Department of Earth and Space Sciences
- University of Washington, Seattle
- Washington University in Saint Louis, Department of Earth and Planetary Science
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