Abstract
This report describes the guideline for using weather data in R and D on solar energy system. Solar radiation is defined as direct, scattered and reflected radiation in a range of near UV-near IR radiation. Direct solar radiation is observed by silver disk pyrheliometer, while global solar radiation by thermostat or bimetal pyranometer. Accuracy standards of such meters are indispensable to keep the accuracy uniformly. To keep the uniformity and accuracy of observation data all over the world, the international comparative observation is held every 5 years. Solar radiation observation in Japan started in 1932 by installing silver disk pyrheliometers all over the country. In 1938 the observation stations were increased to 79 sites, however, in 1953 those were integrated into 13 long-term weather observation stations. Sunshine duration is defined as the time direct sunbeam aims at the ground, and observed generally by Jordan's heliograph which observes sunshine durations with burned holes on photosensitive recording paper by direct sunbeam through 2 small holes on both sides of a cylinder. The history of statistical processing of solar radiation and sunshine duration data in Meteorological Agency is also presented. (NEDO)
Citation Formats
None.
Fiscal 1974 Sunshine Project result report. R and D on solar energy system (weather survey). Part 2. Guideline for using weather data; 1974 nendo kisho data ni saishite no shishin. 2. Taiyo energy system no kenkyu kaihatsu.
Japan: N. p.,
1975.
Web.
None.
Fiscal 1974 Sunshine Project result report. R and D on solar energy system (weather survey). Part 2. Guideline for using weather data; 1974 nendo kisho data ni saishite no shishin. 2. Taiyo energy system no kenkyu kaihatsu.
Japan.
None.
1975.
"Fiscal 1974 Sunshine Project result report. R and D on solar energy system (weather survey). Part 2. Guideline for using weather data; 1974 nendo kisho data ni saishite no shishin. 2. Taiyo energy system no kenkyu kaihatsu."
Japan.
@misc{etde_20093230,
title = {Fiscal 1974 Sunshine Project result report. R and D on solar energy system (weather survey). Part 2. Guideline for using weather data; 1974 nendo kisho data ni saishite no shishin. 2. Taiyo energy system no kenkyu kaihatsu}
author = {None}
abstractNote = {This report describes the guideline for using weather data in R and D on solar energy system. Solar radiation is defined as direct, scattered and reflected radiation in a range of near UV-near IR radiation. Direct solar radiation is observed by silver disk pyrheliometer, while global solar radiation by thermostat or bimetal pyranometer. Accuracy standards of such meters are indispensable to keep the accuracy uniformly. To keep the uniformity and accuracy of observation data all over the world, the international comparative observation is held every 5 years. Solar radiation observation in Japan started in 1932 by installing silver disk pyrheliometers all over the country. In 1938 the observation stations were increased to 79 sites, however, in 1953 those were integrated into 13 long-term weather observation stations. Sunshine duration is defined as the time direct sunbeam aims at the ground, and observed generally by Jordan's heliograph which observes sunshine durations with burned holes on photosensitive recording paper by direct sunbeam through 2 small holes on both sides of a cylinder. The history of statistical processing of solar radiation and sunshine duration data in Meteorological Agency is also presented. (NEDO)}
place = {Japan}
year = {1975}
month = {Mar}
}
title = {Fiscal 1974 Sunshine Project result report. R and D on solar energy system (weather survey). Part 2. Guideline for using weather data; 1974 nendo kisho data ni saishite no shishin. 2. Taiyo energy system no kenkyu kaihatsu}
author = {None}
abstractNote = {This report describes the guideline for using weather data in R and D on solar energy system. Solar radiation is defined as direct, scattered and reflected radiation in a range of near UV-near IR radiation. Direct solar radiation is observed by silver disk pyrheliometer, while global solar radiation by thermostat or bimetal pyranometer. Accuracy standards of such meters are indispensable to keep the accuracy uniformly. To keep the uniformity and accuracy of observation data all over the world, the international comparative observation is held every 5 years. Solar radiation observation in Japan started in 1932 by installing silver disk pyrheliometers all over the country. In 1938 the observation stations were increased to 79 sites, however, in 1953 those were integrated into 13 long-term weather observation stations. Sunshine duration is defined as the time direct sunbeam aims at the ground, and observed generally by Jordan's heliograph which observes sunshine durations with burned holes on photosensitive recording paper by direct sunbeam through 2 small holes on both sides of a cylinder. The history of statistical processing of solar radiation and sunshine duration data in Meteorological Agency is also presented. (NEDO)}
place = {Japan}
year = {1975}
month = {Mar}
}