Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Edo Loenen"'
Publikováno v:
Asian Journal of Atmospheric Environment, Vol 13, Iss 1, Pp 39-44 (2019)
AIRBUS presents a global monitoring service on atmospheric composition and emission allocation. Air composition and meteorological data from satellites and local sensors are combined into a chemical transport model to build up or validate trace gas a
Externí odkaz:
https://doaj.org/article/51404a7063f34b93a8acc46ab45da63d
Autor:
Ugo Cortesi, Simone Ceccherini, Samuele Del Bianco, Marco Gai, Cecilia Tirelli, Nicola Zoppetti, Flavio Barbara, Marc Bonazountas, Argyros Argyridis, André Bós, Edo Loenen, Antti Arola, Jukka Kujanpää, Antti Lipponen, William Wandji Nyamsi, Ronald van der A, Jacob van Peet, Olaf Tuinder, Vincenzo Farruggia, Andrea Masini, Emilio Simeone, Rossana Dragani, Arno Keppens, Jean-Christopher Lambert, Michel van Roozendael, Christophe Lerot, Huan Yu, Koen Verberne
Publikováno v:
Atmosphere, Vol 9, Iss 11, p 454 (2018)
With the launch of the Sentinel-5 Precursor (S-5P, lifted-off on 13 October 2017), Sentinel-4 (S-4) and Sentinel-5 (S-5)(from 2021 and 2023 onwards, respectively) operational missions of the ESA/EU Copernicus program, a massive amount of atmospheric
Externí odkaz:
https://doaj.org/article/48a43581242b45fa94b6d69980c1e5e5
Publikováno v:
Asian Journal of Atmospheric Environment, Vol 13, Iss 1, Pp 39-44 (2019)
AIRBUS presents a global monitoring service on atmospheric composition and emission allocation. Air composition and meteorological data from satellites and local sensors are combined into a chemical transport model to build up or validate trace gas a
Publikováno v:
Space and Photonics Innovation Actors (SPIA) Sixth Meeting, Sesto Fiorentino, 04/12/2019
info:cnr-pdr/source/autori:Ugo Cortesi, Emilio Simeone, Edo Loenen, Consorzio AURORA/congresso_nome:Space and Photonics Innovation Actors (SPIA) Sixth Meeting/congresso_luogo:Sesto Fiorentino/congresso_data:04%2F12%2F2019/anno:2019/pagina_da:/pagina_a:/intervallo_pagine
info:cnr-pdr/source/autori:Ugo Cortesi, Emilio Simeone, Edo Loenen, Consorzio AURORA/congresso_nome:Space and Photonics Innovation Actors (SPIA) Sixth Meeting/congresso_luogo:Sesto Fiorentino/congresso_data:04%2F12%2F2019/anno:2019/pagina_da:/pagina_a:/intervallo_pagine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=cnr_________::a7da86b5209da2c2a66371b949d02bb9
https://publications.cnr.it/doc/413390
https://publications.cnr.it/doc/413390
Autor:
Nicola Zoppetti, Rossana Dragani, Michel Van Roozendael, Ugo Cortesi, Argyros Argyridis, Edo Loenen, O. N. E. Tuinder, Arno Keppens, Antti Lipponen, Simone Ceccherini, Cecilia Tirelli, Jukka Kujanpää, Koen Verberne, Andrea Masini, Marco Gai, William Wandji Nyamsi, Jacob C. A. van Peet, Huan Yu, Flavio Barbara, Antti Arola, Christophe Lerot, Samuele Del Bianco, Vincenzo Farruggia, Jean-Christopher Lambert, Marc Bonazountas, Ronald van der A, André Bós, Emilio Simeone
Publikováno v:
Atmosphere, Vol 9, Iss 11, p 454 (2018)
Atmosphere
Volume 9
Issue 11
Atmosphere
Volume 9
Issue 11
With the launch of the Sentinel-5 Precursor (S-5P, lifted-off on 13 October 2017), Sentinel-4 (S-4) and Sentinel-5 (S-5)(from 2021 and 2023 onwards, respectively) operational missions of the ESA/EU Copernicus program, a massive amount of atmospheric
Autor:
Ugo Cortesi, Simone Ceccherini, Samuele Del Bianco, Marco Gai, Cecilia Tirelli, Nicola Zoppetti, Antti Arola, Jukka Kujanpää, Antti Lipponen, Rossana Dragani, Arno Keppens, Michel Van Roozendael, Edo Loenen, Andrea Masini, Emilio Simeone, Marc Bonazountas, Argyros Argyridis, Ronald van derA, Jacob van Peet, Olaf Tuinder, Koen Verberne.
Publikováno v:
EUMETSAT METEOROLOGICAL SATELLITE CONFERENCE 2018, Tallinn, Estonia, 17-21/09/2018
info:cnr-pdr/source/autori:Ugo Cortesi, Simone Ceccherini, Samuele Del Bianco, Marco Gai, Cecilia Tirelli, Nicola Zoppetti, Antti Arola, Jukka Kujanpää, Antti Lipponen, Rossana Dragani, Arno Keppens, Michel Van Roozendael, Edo Loenen, Andrea Masini, Emilio Simeone, Marc Bonazountas, Argyros Argyridis, Ronald van derA, Jacob van Peet, Olaf Tuinder, Koen Verberne./congresso_nome:EUMETSAT METEOROLOGICAL SATELLITE CONFERENCE 2018/congresso_luogo:Tallinn, Estonia/congresso_data:17-21%2F09%2F2018/anno:2018/pagina_da:/pagina_a:/intervallo_pagine
info:cnr-pdr/source/autori:Ugo Cortesi, Simone Ceccherini, Samuele Del Bianco, Marco Gai, Cecilia Tirelli, Nicola Zoppetti, Antti Arola, Jukka Kujanpää, Antti Lipponen, Rossana Dragani, Arno Keppens, Michel Van Roozendael, Edo Loenen, Andrea Masini, Emilio Simeone, Marc Bonazountas, Argyros Argyridis, Ronald van derA, Jacob van Peet, Olaf Tuinder, Koen Verberne./congresso_nome:EUMETSAT METEOROLOGICAL SATELLITE CONFERENCE 2018/congresso_luogo:Tallinn, Estonia/congresso_data:17-21%2F09%2F2018/anno:2018/pagina_da:/pagina_a:/intervallo_pagine
The exploitation of complementary and redundant information on atmospheric targets simultaneously observed by multiple independent data sources, such as the atmospheric Sentinels, has intrinsic potential to extend the quality of geophysical products
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=cnr_________::a6bc769b15e05092c64bbd4f2259edec
http://www.cnr.it/prodotto/i/433901
http://www.cnr.it/prodotto/i/433901
Publikováno v:
Proceedings of the International Astronomical Union. 8:215-218
Line emissions of high- and low-density molecular tracers serve as powerful diagnostic tools for the ISM in both Galactic and extragalactic star formation environments. The emission line strengths and line ratios may be interpreted using detailed mod
Publikováno v:
EAS Publications Series. 31:111-114
The behavior of molecular tracers of the high-density star-forming ISM provides a diagnostics tool for luminous FIR galaxies. All molecules react differently to the physical and chemical environment and their collective behavior is indicative of the
Publikováno v:
Highlights in Astronomy
A report on studies using the observed line ratios of high-density molecular tracers to diagnose the physics and chemistry of the ISM in star-formation environments.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::daa1d80ad05f9a757e13dbcf9d31e239
https://doi.org/10.1017/S1743921310009993
https://doi.org/10.1017/S1743921310009993
Autor:
Alicia Berciano Alba, Fabian Walter, Pierre Cox, Paul van der Werf, Dominik Riechers, Axel Weiss, Edo Loenen, Rowin Meijerink, Marco Spaans
Publikováno v:
Astrophysical Journal Letters, 741(2):L38. IOP PUBLISHING LTD
We present the detection of four rotational emission lines of water vapor, from energy levels Eu/k= 101 - 454 K, in the gravitationally lensed z=3.9 QSO host galaxy APM08279+5255. While the lowest H2O lines are collisionally excited in clumps of warm