HelioWebMario D'Amore
flowchart
A[Mario D'Amore]
AC["Associated Concepts (19)"]
AW["Authored Works (26)"]
CA["Linked Co-Authors (2)"]
CI["Linked Collaborating Institutions (30)"]
A== dcterms:relation ==>AC
AW== author ==>A
AW== author ==>CA
AW== affil ==>CI
click AC "#associated-concepts"
click AW "#authored-works"
click CA "#co-authors"
click CI "#collaborating-institutions"
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- ORCiD
- https://orcid.org/0000-0001-9325-6889
- OpenAlex ID
- https://openalex.org/A5029165722 (API record)
Associated Concepts [?]
- Biology
- Physics
- Geology
- Chemistry
- Astronomy
- Computer science
- Medicine
- Quantum mechanics
- Geography
- Astrobiology
- Internal medicine
- Optics
- Remote sensing
- Genetics
- Immunology
- Pathology
- Programming language
- Biochemistry
- Mercury (programming language)
Authored Works
sorted by decreasing year, and then by display-name
- Machine Learning Approach to Deconvolution of Mid-Infrared Telescope Spectra of Mercury: Supporting MERTIS onboard ESA/JAXA BepiColombo mission
- Gaining a global perspective on the surface composition of Venus from orbit through near infrared observations - with a little help from machine learning approaches
- Venus surface peeking through the atmosphere - gaining a global perspective on the surface composition through near infrared observations
- Surface mapping via unsupervised classification of remote sensing: application to MESSENGER/MASCS and DAWN/VIRS data.
- Deconvolution of Thermal Emissivity Spectra of Mercury to their Endmember Counterparts measured in Simulated Mercury Surface Conditions
- Reflectance and Emissivity Spectra of Graphite as Potential Darkening Agent for Mercury from the UV to the TIR and its Comparison to Remote Sensing Measurements from MESSENGER and MERTIS on BepiColombo
- Machine Learning Applied to Dawn/VIR data of Vesta in view of MERTIS/BepiColombo.
- Unravelling thermal emissivity spectra of the main minerals on Mercury's surface by comparison with ab initio calculated IR-HT vibrational frequencies
- A Hydrothermally Altered, Mn-incrusted Marine Sediment as an Analogue for Martian Deposits?
- Unsupervised Classification of Mercury's Surface Spectral and Chemical Characteristics
- TIR Spectroscopy: Looking for Igneous Rocks on the Surface of Mercury.
- Emissivity and Reflectance Spectra of Asteroid Analogs: Their Dependence on Emerging Angle
- TIR Emissivity Spectra of Thermally Processed Sulfates, Carbonates and Phyllosilicates as Analog Materials for Asteroid Surfaces
- Simulated MERTIS observation of the Rudaki-Kuiper craters area on Mercury
- Emissivity Spectra of Meteoritic Powders mixed with Liquid Formamide (NH2COH) at Different Temperatures
- Calcium pyroxenes at Mercurian surface temperatures: investigation of in-situ emissivity spectra and thermal expansion
- Surface units on Mercury defined by unsupervised classification analysis of MESSENGER spectral reflectance data from the first year in orbit
- Making Sense of 2.5 Million Surface Reflectance Spectra of Mercury from MESSENGER
- Emissivity and reflectance measurements of 10 meteoritic analogues in the 1 to 100 μm spectral range, from PEL
- Simulating thermal stress features on hot planetary surfaces in vacuum at high temperature facility in the PEL laboratory
- High-temperature laboratory measurements in support of a statistical analysis of spectral data from MESSENGER
- Simulating airless and/or hot planetary surfaces in the Planetary Emissivity Laboratory (PEL)
- Detection of Phyllosilicates on Mars from PFS Observations
- Compositional units on Mercury from principal component and clustering analyses of MESSENGER spectrometer observations
- Turn the heat up - A first look at MESSENGER's near-infrared spectra of Mercury using new high-temperature emissivity measurements
- Emissivity of Phyllosilicates From the Berlin Emissivity Database (BED) in the [3, 50] Micron Spectral Range in Support of Remote Sensed Data Analysis
Linked Co-Authors
Linked Collaborating Institutions
- American Museum of Natural History, New York
- Brown University, Department of Geological Sciences
- Carnegie Institution of Washington
- Carnegie Institution of Washington, Department of Terrestrial Magnetism
- Catholic University, Washington DC
- Columbia University, New York
- Ecole Polytechnique, France
- Free University of Berlin, Germany
- German Aerospace Center, Berlin
- Helmholtz Institute for Planetary Research, Berlin
- Jet Propulsion Laboratory
- Johns Hopkins University, Applied Physics Laboratory
- Lamont-Doherty Earth Observatory
- Mount Holyoke College, Massachusetts
- Planetary Science Institute, Arizona
- SETI Institute, California
- Smithsonian Institution Air and Space Museum
- University of Arizona, Department of Planetary Sciences
- University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics
- University of Hawaii, Manoa
- University of Hawaii, Manoa, School of Earth and Ocean Sciences
- University of Munster, Institute for Planetology
- University of Padua, Department of Geosciences
- University of Padua, Italy
- University of Parma, Italy
- University of Pavia, Department of Earth Sciences
- University of Pavia, Italy
- University of Turin, Italy
- University of Tuscia, Italy
- Wilhelms University of Munster, Germany
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