Zobrazeno 1 - 10
of 58
pro vyhledávání: '"G. Trivellone"'
Autor:
F. Ravegnani, M. Premuda, S. Pagnutti, F. Margelli, I. Kostadinov, D. Bortoli, A. Petritoli, E. Palazzi, G. Giovanelli, G. Trivellone
Publikováno v:
Annals of Geophysics, Vol 49, Iss 1 (2006)
tants, offering numerous advantages over conventional networks of in situ analysers. We propose some innovative solutions in the field of DOAS (Differential Optical Absorption Spectroscopy) remote systems, utilizing diffuse solar light as the radiati
Externí odkaz:
https://doaj.org/article/1d6674ff8eed43449476dcfeffc4c244
Publikováno v:
Meteorological Applications. 24:338-348
A detailed observational study of squall line thunderstorms, a particular form of mesoscale convective systems arranged in a line that repeatedly affected Salento Peninsula (southern Apulia, Italy) throughout 2015, is presented and discussed. Specifi
Autor:
Boyan Petkov, Paolo Bonasoni, Christian Lanconelli, G. Trivellone, Angelo Lupi, Paolo Cristofanelli, U. Bonafè, Vito Vitale, Francescopiero Calzolari
Publikováno v:
Antarctic Science. 20:415-421
Ozone concentration measurements were made during December from 2001–2005 to quantify the contributions of different processes to near-surface ozone concentrations (O3) in Terra Nova Bay, Antarctica. The average O3 concentration was 20.3 ppbv. On d
Autor:
G. Bianchini, S. Argentini, M. Baldi, F. Cairo, F. Calzolari, G. casasanta, A. Conidi, M. del Guasta, G. Di Natale, S. federico, A. Lupi, M. Mazzola, M. De Muro, L. Palchetti, I. Petenko, B. Petkov, M. Snels, G. Trivellone, A.Viola, M. Viterbini
Publikováno v:
EGU General Assembly Conference, pp. 7782, Vienna, maggio 2014
info:cnr-pdr/source/autori:G. Bianchini, S. Argentini, M. Baldi, F. Cairo, F. Calzolari, G. casasanta, A. Conidi, M. del Guasta, G. Di Natale, S. federico, A. Lupi, M. Mazzola, M. De Muro, L. Palchetti, I. Petenko, B. Petkov, M. Snels, G. Trivellone, A.Viola, M. Viterbini/congresso_nome:EGU General Assembly Conference/congresso_luogo:Vienna/congresso_data:maggio 2014/anno:2014/pagina_da:7782/pagina_a:/intervallo_pagine:7782
info:cnr-pdr/source/autori:G. Bianchini, S. Argentini, M. Baldi, F. Cairo, F. Calzolari, G. casasanta, A. Conidi, M. del Guasta, G. Di Natale, S. federico, A. Lupi, M. Mazzola, M. De Muro, L. Palchetti, I. Petenko, B. Petkov, M. Snels, G. Trivellone, A.Viola, M. Viterbini/congresso_nome:EGU General Assembly Conference/congresso_luogo:Vienna/congresso_data:maggio 2014/anno:2014/pagina_da:7782/pagina_a:/intervallo_pagine:7782
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=cnr_________::43a96a8a6f89c9f512781df755c81d9e
https://publications.cnr.it/doc/288278
https://publications.cnr.it/doc/288278
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 61:539-543
The ozone concentration has been measured in the meteor zone using a method of radar echo duration distribution suggested by Jones and Simek (1995) . Data obtained by the forward-scatter system during the Lyrid meteor shower period in five consecutiv
Publikováno v:
Planetary and Space Science. 46:869-880
Forward scatter (FS) continuous wave (CW) meteor radar observations carried out during 1992–96 over the long baseline Bologna–Lecce in Italy, enable us to investigate the structure of the main meteoroid streams and of the sporadic background by t
Publikováno v:
Il Nuovo Cimento C. 19:283-289
Radar observations of the main meteor showers in 1993–1995 carried out by a forward-scatter radiosystem Bologna-Lecce in Italy are analysed and discussed in terms of fragmentation effects even in the orbit of the streams of interplanetary matter. T
Publikováno v:
Il Nuovo Cimento C. 18:343-349
Continuous radio wave monitoring of the Leonid meteoroid stream during November 12–21, 1994, has been carried out by using a forward-scatter bistatic radar operating over the Bologna-Lecce baseline in Italy. An enhanced activity starting from Novem
Publikováno v:
Earth, Moon, and Planets. 68:465-469
Radio observations of the Lyrid meteor shower obtained by a forward scatter radio system (Bologna-Lecce) in 1994 are analysed and discussed. The shower maximum appeared at solar longitude 31.0°(1950.0) and a distinct displacement between the maxima
Autor:
G. Trivellone, Luigi Foschini, G. Cevolani, V. Porubčan, C. Franceschi, A. Hajduk, G. Grassi, G. Bortolotti
Publikováno v:
Earth, Moon, and Planets. 68:247-255
Continuous radio-wave monitoring of the Geminid activity in December 1992 and 1993 by using a forward scatter (FS) bistatic radar over the Bologna-Lecce baseline (700 km) in Italy, reveals peculiar structural aspects of the stream in terms of signal