Njau, E. C. (2004) Natural solar energy amplifiers in planet-atmosphere systems. Il nuovo cimento C, 27 (6). pp. 579-593. ISSN 1826-9885
|
Text
ncc8897.pdf - Published Version Download (193kB) | Preview |
Abstract
Planets and their atmospheres (including the Earth and its atmosphere) continuously receive solar energy which comprises very small variable components and a relatively huge constant component. On the basis of certain conditions, specific physical mechanisms can exist in each planet-atmosphere system under which the tiny variable solar energy components so received apparently undergo large amplifications. In the case of the Earth-Atmosphere system, these energy amplifications continuously exist and involve maximum amplification factors that range from ∼ 2312 to over 6915 for frequencies equal to or less than the 11-year sunspot cycle frequency. Consequently energy and hence temperature variations at the solar (or sunspot) cycle frequencies dominantly exist in the Earth-Atmosphere system. These energy and temperature variations are continuously mapped or translated into corresponding variations in the other weather parameters as verified by pastrecords.
Item Type: | Article |
---|---|
Uncontrolled Keywords: | Planets, their satellites and rings; asteroids ; Climatology ; Solar modulation and geophysical effects |
Subjects: | 500 Scienze naturali e Matematica > 550 Scienze della Terra > 551.6 Climatologia e tempo atmosferico (Classificare qui i lo studio dei Cambiamenti climatici) |
Depositing User: | Marina Spanti |
Date Deposited: | 14 Mar 2020 12:17 |
Last Modified: | 14 Mar 2020 12:17 |
URI: | http://eprints.bice.rm.cnr.it/id/eprint/15269 |
Actions (login required)
View Item |