๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Solar irradiance modulation by active regions during 1980

โœ Scribed by Sabatino Sofia; Ludwig Oster; Kenneth Schatten


Publisher
Springer
Year
1982
Tongue
English
Weight
577 KB
Volume
80
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

โœฆ Synopsis


The solar irradiance modulation due to active regions during 1980 has been investigated in detail. Specifically, we estimate the uncertainties caused by ground-based data used as input in the modeling effort, and by our currently incomplete knowledge of the proper parameters that describe the angular variation of sunspot and facular contrasts. We conclude that the most significant uncertainties are due to errors in area measurements and, possibly, varying spot and facular brightness. A 'standard model' for later use is derived by a best-fit technique of the currently available ACRIM irradiance data and the predictions of our models with appropriately varied parameters. Finally, we compute the expected irradiance for the entire year of 1980.


๐Ÿ“œ SIMILAR VOLUMES


Modulation of Solar Constant by Active R
โœ J. Pap ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 516 KB

## Abstract Irradiance records of the Nimbusโ€7 and SMM satellites indicate a systematic downward trend of the solar constant of the order of a few hundredths of a percent and a slow variation of the solar constant on a time scale from days to weeks. The reason for the downward trend is not known as

Solar irradiance variations from photome
โœ G. A. Chapman; A. D. Meyer ๐Ÿ“‚ Article ๐Ÿ“… 1986 ๐Ÿ› Springer ๐ŸŒ English โš– 442 KB

The Extreme Limb Photometer (ELP) has been used to measure the irradiance fluctuation of the Sun due to selected active regions. Forty-five active regions that were completely scanned at various disk positions are included in the analysis. The contribution of these active regions to a global solar i

Slow changes of solar irradiance and ene
โœ A. V. Mordvinov ๐Ÿ“‚ Article ๐Ÿ“… 1996 ๐Ÿ› Springer ๐ŸŒ English โš– 538 KB

A new numerical technique is applied to study long-term variations of total solar irradiance. The background solar flux is estimated not from, e.g., a running mean but as the mode on a moving short time interval. Statistical properties of short-term variations with respect to the running mode are st

Solar total irradiance observations by A
โœ Richard C. Willson ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 697 KB

Pyrheliometry, definition of the radiation scale in the International System of Units and monitoring the variability of solar total irradiance have been a focus of research at the Jet Propulsion Laboratory since the mid 1960's. A series of automated, electrically self-calibrating, cavity pyrheliomet

Observable Physical Effects during New S
โœ V. Bumba ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 763 KB

## Formations'' I n the present paper we are trying to demonstrate the importance of detailed observations for the theory of solar local magnetic field generation. Mutual relations of solar background magnetic fields and new active region formations are described. The influence of various factors,