SonÄno sevanje - F9

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PRENOS TOPLOTE S SEVANJEMc0 E = hν = hλ Planckov zakon:∂j=∂λ Wienov zakon:λmaxT = C 322πhc5λ exp( hckλT ) −1( ) 1C3 = 2897.8 µmK Stefanov zakonj = σT4j* = εσT4

Nuclear Instruments and Methods in Physics Research A - F9

Study of radiation damage in silicon detectors for high ... - F9

modelling and measurements of laser-skin thermal interaction - F9

ReÅ¡ene naloge iz fizike jedra in osnovnih delcev - F9

Separation of Sr from Ca, Ba and Ra by means of Ca(OH)2 and ... - F9

Excel Add-in Development in C/C++: Applications in ... - F9

PRENOS TOPLOTE S SEVANJEMc0 E = hν = hλ Planckov zakon:∂j=∂λ Wienov zakon:λmaxT = C 322πhc5λ exp( hckλT ) −1( ) 1C3 = 2897.8 µmK Stefanov zakonj = σT4j* = εσT4

SONCE Je rumena pritlikavka Srednja razdalja medSoncem in Zemljo je149.6*10^9 m Kemična sestavaSonca: H (60%), He(35%), 5% - O, Mg,Fe, Si, Na

Page 1 and 2: SONČNO SEVANJEDorina SeverFizika e
Page 3: ZGODOVINA Sončno toploto so izkori
Page 7 and 8: GEOMETRIJSKE RELACIJE MEDSONCEM IN
Page 9 and 10: SPEKTER SONČNEGA SEVANJA Podoben s
Page 11 and 12: DNEVNO IN LETNO OBSEVANJE
Page 13: IZKORIŠČANJE SONČNEGA Za ogrevan
Page 16 and 17: POVPREČNA ENERGIJSKA BILANCAZEMLJE
Page 18 and 19: ENERGIJSKA BILANCA ZEMLJE,ATMOSFERE
Page 20: LITERATURAHsieh, Jui Sheng: Solar E

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SonÄno sevanje - F9