Zobrazeno 1 - 10
of 54
pro vyhledávání: '"D.A. Gagliardini"'
Publikováno v:
Solar & Wind Technology. 7:501-509
Incoming solar radiation, insolation, is an important factor in many processes occuring at the earth surface. These include natural processes such as energy and moisture flux, photosynthesis, evapotranspiration, as well as quantities of interest in s
Autor:
D.A. Gagliardini, H. Karszenbaum
Publikováno v:
Journal of Atmospheric and Terrestrial Physics. 44:613-618
In this paper the interaction of precipitated protons with the atmospheric components is analyzed using a new approach. The method described presents a different way of calculating the proton effects yielding the production rate and fluxes of the gen
Autor:
D.A. Gagliardini, H. Karszenbaum
Publikováno v:
Advances in Space Research. 1:35-38
In this paper we analyse from a new point of view the energy deposition due to precipitated protons when they interact with the atmospheric components. The method described presents a different way of calculating the proton interaction and allows us
Autor:
H. Karszenbaum, D.A. Gagliardini
Publikováno v:
Advances in Space Research. 7:7-10
In the present paper some properties of the NOAA-AVHRR system and information are analysed. A description of the main characteristics of the vegetation of the southest region of South America and the surrounding ocean currents are presented. The appl
Publikováno v:
Remote Sensing of Environment. 15:21-36
In this paper the application of Landsat MSS, NOAA/TIROS AVHRR, and NIMBUS CZCS to study the La Plata River is analyzed. To accomplish this objective, some properties of the river are described first and, second, the following characteristics of the
Publikováno v:
Solar Energy. 41:61-69
Daily values of the solar radiant energy incident on earth's surface constitute a quantity of increasing importance, not only in nonconventional energy development but also for agricultural, weather, and climate monitoring and predictions. In Argenti
Autor:
D.A. Gagliardini, H. Karszenbaum
Publikováno v:
Journal of Atmospheric and Terrestrial Physics. 37:845-849
The electron production rates in the lower ionosphere, due to galactic X-rays, are computed. It is shown that the contribution of photons of energies greater than 10 keV is relevant below 80 km. A non constant photoionization yield is introduced in t
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