Zobrazeno 1 - 10
of 723
pro vyhledávání: '"ESA Cosmic Vision"'
SPICA (Space Infrared Telescope for Cosmology and Astrophysics) is a JAXA led observatory that will operate in the mid and far infrared wavelength range (5-210 micron) with unprecedented sensitivity, thanks to the 3.5 m (current baseline) cold telesc
Externí odkaz:
http://arxiv.org/abs/1001.0709
Autor:
Barcons, X., Barret, D., Decourchelle, A., Herder, J. -W. den, Dotani, T., Fabian, A. C., Fraga-Encinas, R., Kunieda, H., Lumb, D., Matt, G., Nandra, K., Piro, L., Rando, N., Sciortino, S., Smith, R. K., Strüder, L., Watson, M. G., White, N. E., Willingale, R.
Athena is an X-ray observatory-class mission concept, developed from April to December 2011 as a result of the reformulation exercise for L-class mission proposals in the framework of ESA's Cosmic Vision 2015-2025. Athena's science case is that of th
Externí odkaz:
http://arxiv.org/abs/1207.2745
Autor:
Barcons, X., Barret, D., Bautz, M., Bookbinder, J., Bregman, J., Dotani, T., Flanagan, K., Fraga-Encinas, R, Grady, J., Kunieda, H., Lumb, D. H., Mitsuda, K., Nandra, K., Ohashi, T., Piro, L., Rando, N., Strüder, L., Takahashi, T., Tsuru, T. G., White, N. E.
The International X-Ray Observatory (IXO) will address fundamental questions in astrophysics, including "When did the first SMBH form? How does large scale structure evolve? What happens close to a black hole? What is the connection between these pro
Externí odkaz:
http://arxiv.org/abs/1102.2845
Autor:
Giovanni Santin, J. Sorensen
Publikováno v:
2009 European Conference on Radiation and Its Effects on Components and Systems.
This paper describes some of the radiation environments and their effects encountered by the Cosmic Vision missions, with emphasis on the design specifications and verification tools, including new shielding analysis techniques.
Publikováno v:
SPIE Proceedings.
PLATO is a candidate of the European Space Agency's Science programme Cosmic Vision 2015-2025. "PLAnetary Transits and Oscillations of stars" aims to characterise exoplanetary systems by detecting planetary transits and conducting asteroseismology of
Autor:
Michel, Patrick, Barucci, Antonella, Yoshikawa, Makoto, Koschny, Detlef, Boenhardt, Hermann, Brucato, John Robert, Coradini, Marcello, Dotto, Elisabetta, Franchi, Ian, Green, Simon F., Josset, Jean-Luc, Kawaguchi, Junichiro, Muinonen, Karri, Oberst, Jürgen, Yano, Hajime, Binzel, Rick, Agnolon, David, Romstedt, Jens
Publikováno v:
1st IAA Planetary Defense Conference: Protecting the Earth from Asteroids
Marco Polo is a sample return mission to a Near-Earth Object (NEO) which was originally proposed as a joint European-Japanese mission for the scientific program Cosmic Vision 2015-2025 of the European Space Agency (ESA) in June 2007 and selected for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::54e644a879a1c91604640427761c0485
http://oro.open.ac.uk/24835/1/2009_Michel_et_al_Grenada.pdf
http://oro.open.ac.uk/24835/1/2009_Michel_et_al_Grenada.pdf
Publikováno v:
Proceedings of the 29th International Cosmic Ray Conference
29th International Cosmic Ray Conference-ICRC 2005
29th International Cosmic Ray Conference-ICRC 2005, Aug 2005, Pune, India. pp.121-124
Scopus-Elsevier
29th International Cosmic Ray Conference-ICRC 2005
29th International Cosmic Ray Conference-ICRC 2005, Aug 2005, Pune, India. pp.121-124
Scopus-Elsevier
The astrophysical and physical processes at the very end of the known energy spectrum, in the region of the so-called Ultra High Energies (UHE), have been the subject of an intense debate in the last years. UHE particles are nucleons, nuclei, photons
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::6391ae3cf22c372d898081b497312080
http://hal.in2p3.fr/in2p3-00086022/document
http://hal.in2p3.fr/in2p3-00086022/document
Publikováno v:
SPIE Proceedings.
In order to better understand the properties of exoplanetary systems, the Cosmic Vision mission "PLAnetary Transits and Oscilliations of stars" (PLATO) will detect and characterise exoplanets using their transit signature in front of a large sample o