WHY IS THE SOLAR CONSTANT NOT A CONSTANT?
Journal Article
·
· Astrophysical Journal
- National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011 (China)
- Research Center of Analysis and Measurement, Kunming University of Science and Technology, Kunming 650093 (China)
- Department of Physics, Yunnan Normal University, Kunming 650093 (China)
In order to probe the mechanism of variations of the solar constant on the inter-solar-cycle scale, the total solar irradiance (TSI; the so-called solar constant) in the time interval of 1978 November 7 to 2010 September 20 is decomposed into three components through empirical mode decomposition and time-frequency analyses. The first component is the rotation signal, counting up to 42.31% of the total variation of TSI, which is understood to be mainly caused by large magnetic structures, including sunspot groups. The second is an annual-variation signal, counting up to 15.17% of the total variation, the origin of which is not known at this point in time. Finally, the third is the inter-solar-cycle signal, counting up to 42.52%, which is inferred to be caused by the network magnetic elements in quiet regions, whose magnetic flux ranges from (4.27-38.01) Multiplication-Sign 10{sup 19} Mx.
- OSTI ID:
- 22016246
- Journal Information:
- Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 747; ISSN ASJOAB; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
Similar Records
THE LATITUDE DISTRIBUTION OF SMALL-SCALE MAGNETIC ELEMENTS IN SOLAR CYCLE 23
WHAT CAUSES THE INTER-SOLAR-CYCLE VARIATION OF TOTAL SOLAR IRRADIANCE?
THE SUN'S SMALL-SCALE MAGNETIC ELEMENTS IN SOLAR CYCLE 23
Journal Article
·
Thu Jan 19 23:00:00 EST 2012
· Astrophysical Journal
·
OSTI ID:22012001
WHAT CAUSES THE INTER-SOLAR-CYCLE VARIATION OF TOTAL SOLAR IRRADIANCE?
Journal Article
·
Mon Dec 14 23:00:00 EST 2015
· Astronomical Journal (Online)
·
OSTI ID:22520090
THE SUN'S SMALL-SCALE MAGNETIC ELEMENTS IN SOLAR CYCLE 23
Journal Article
·
Sun Apr 10 00:00:00 EDT 2011
· Astrophysical Journal
·
OSTI ID:21574774