Zobrazeno 1 - 10
of 135
pro vyhledávání: '"Vittorio Formisano"'
Autor:
Marilena Amoroso, Julia Marin-Yaseli de la Parra, Paulina Wolkenberg, Frank Daerden, Dorothy Z. Oehler, Alejandro Cardesín-Moinelo, Donald Merritt, Marco Giuranna, Giuseppe Etiope, A. Aronica, Sébastien Viscardy, Lori Neary, Vittorio Formisano, Shohei Aoki
Reports of methane detection in the Martian atmosphere have been intensely debated. The presence of methane could enhance habitability and may even be a signature of life. However, no detection has been confirmed with independent measurements. Here,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ff0b18298048c7b37fb612eea210064
http://hdl.handle.net/20.500.12386/30044
http://hdl.handle.net/20.500.12386/30044
Autor:
Diego Scaccabarozzi, Shohei Aoki, Paulina Wolkenberg, A. Aronica, Marco Giuranna, Vittorio Formisano, Davide Grassi, Bortolino Saggin
We used thermal-infrared spectra returned by the Mars Express Planetary Fourier Spectrometer (PFS/MEx) to retrieve atmospheric temperature profiles, surface temperatures, and column-integrated optical depths of dust and water ice. More than 2,500,000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cdee2c12edd331bce29bc93a1bc33235
http://hdl.handle.net/11311/1135680
http://hdl.handle.net/11311/1135680
Autor:
Andrea Longobardo, Paulina Wolkenberg, Marco Giuranna, Giuseppe Sindoni, Vittorio Formisano, Sergio Fonte
We present PFS-MEX limb observations of the CO2 non-local thermodynamic equilibrium (non-LTE) emission at 4.3 μm in the atmosphere of Mars collected in more than six Martian years. With unprecedented spatial and temporal coverage, and relatively hig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e061e0ae85849fcea630b800595403f
http://hdl.handle.net/20.500.12386/27905
http://hdl.handle.net/20.500.12386/27905
Autor:
Yasumasa Kasaba, Vittorio Formisano, A. Geminale, Shohei Aoki, Giuseppe Sindoni, Marco Giuranna, Hiromu Nakagawa
Publikováno v:
Icarus. 245:177-183
We searched for hydrogen peroxide (H2O2) in the Martian atmosphere using data measured by the Planetary Fourier Spectrometer (PFS) onboard Mars Express during five martian years (MY27-31). It is well known that H2O2 plays a key role in the oxidizing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f1a18fb5da10902e10631756a49ab5c7
https://doi.org/10.1016/j.icarus.2014.09.034
https://doi.org/10.1016/j.icarus.2014.09.034
Autor:
Dale P. Cruikshank, Angioletta Coradini, F. Leader, Pierre Drossart, Karl L. Mitchell, P. Cerroni, Robert M. Nelson, Randolph L. Kirk, Dennis L. Matson, Stephen D. Wall, Fabrizio Capaccioni, John C. Pearl, Kevin H. Baines, Vito Mennella, M. Combes, P. D. Nicholson, Gianrico Filacchione, M. D. Boryta, Ralf Jaumann, L. W. Kamp, Yves Langevin, Rosaly M. C. Lopes, Bruno Sicardy, Thomas B. McCord, Jonathan I. Lunine, Vittorio Formisano, Jean-Pierre Bibring, Roger N. Clark, Bruce Hapke, Patrick G. J. Irwin, Christophe Sotin, Giancarlo Bellucci, William D. Smythe
Publikováno v:
Geophysical Research Letters
Geophysical Research Letters, 2009, 36, pp.04202. ⟨10.1029/2008GL036206⟩
Geophysical Research Letters, 2009, 36, pp.04202. ⟨10.1029/2008GL036206⟩
International audience; We report infrared spectrophotometric variability on the surface of Saturn's moon Titan detected in images returned by the Visual and Infrared Mapping Spectrometer (VIMS) onboard the Cassini Saturn Orbiter. The changes were ob
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38d74dde33a1eb6f5a3fc4f48f48795a
https://ora.ox.ac.uk/objects/uuid:6ae22888-2b99-4a6f-99e0-0ee2bed83d1b
https://ora.ox.ac.uk/objects/uuid:6ae22888-2b99-4a6f-99e0-0ee2bed83d1b
Publikováno v:
Icarus. 215:628-638
The interval from Ls = 330° in Mars Year (MY) 26 until Ls = 84° in MY 27 has been used to compare and validate measurements from the Mars Global Surveyor Thermal Emission Spectrometer (TES) and the Mars Express Planetary Fourier Spectrometer (PFS).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f64bf66665db55e04592d43298844058
https://doi.org/10.1016/j.icarus.2011.07.032
https://doi.org/10.1016/j.icarus.2011.07.032
Autor:
Bernd Funke, Pierre Drossart, Vittorio Formisano, Miguel Lopez-Valverde, Giuseppe Piccioni, Manuel López-Puertas, Gabriella Gilli
Publikováno v:
Planetary and Space Science. 59:1010-1018
We report here on CO limb observations in Mars, Venus and Earth and their model simulations. A comparative study of the CO emission, including the most recent spacecraft observations of the three planets’ atmospheres, has been performed. Strong day
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::410d7fd99988058a11a0a701a4525209
https://doi.org/10.1016/j.pss.2010.07.023
https://doi.org/10.1016/j.pss.2010.07.023
Autor:
Maya García-Comas, Vittorio Formisano, Miguel Lopez-Valverde, Manuel López-Puertas, Bernd Funke, Gabriella Gilli, Pierre Drossart, Giuseppe Piccioni
Publikováno v:
Planetary and Space Science
Planetary and Space Science, 2011, 59, pp.988-998. ⟨10.1016/j.pss.2010.02.001⟩
Planetary and Space Science, 2011, 59, pp.988-998. ⟨10.1016/j.pss.2010.02.001⟩
International audience; The MIPAS instrument on board Envisat, in Earth orbit, the PFS and OMEGA instruments on Mars Express, and VIRTIS on board Venus Express are currently providing a dataset of limb measurements of the CO 2 atmospheric fluorescenc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63bfaa95adadce661a3af70aa682825b
https://doi.org/10.1016/j.pss.2010.02.001
https://doi.org/10.1016/j.pss.2010.02.001
Publikováno v:
Planetary and Space Science. 59:149-162
In the history of Mars exploration its atmosphere and planetary climatology aroused particular interest. In the study of the minor gases abundance in the Martian atmosphere, water vapour became especially important, both because it is the most variab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c25a5e5c547c395989d2b61cca3d0af9
https://doi.org/10.1016/j.pss.2010.12.006
https://doi.org/10.1016/j.pss.2010.12.006
Publikováno v:
Planetary and Space Science. 59:137-148
In this study we map the methane gas in the Martian atmosphere. The main goal of this work is to show the methane behaviour across the planet seasonally. To this aim, we analyze the strongest methane band in the short wavelength channel of the Planet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ce5f4cd0144a9ef694bf02422af94b02
https://doi.org/10.1016/j.pss.2010.07.011
https://doi.org/10.1016/j.pss.2010.07.011