WHY IS THE SOLAR CONSTANT NOT A CONSTANT?
- 1. National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011 (China)
- 2. Research Center of Analysis and Measurement, Kunming University of Science and Technology, Kunming 650093 (China)
- 3. Department of Physics, Yunnan Normal University, Kunming 650093 (China)
- 4. Jingdezhen Ceramic Institute, Jingdezhen 333001, Jiangxi (China)
Description
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) × 1019 Mx.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-637X/747/2/135Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 747
- Journal Issue
- 2
- Journal Page Range
- [5 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43103349
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANNUAL VARIATIONS; FREQUENCY ANALYSIS; MAGNETIC FLUX; RADIANT FLUX DENSITY; ROTATION; SIGNALS; SOLAR CONSTANT; SOLAR CYCLE; SUN; SUNSPOTS
- Descriptors DEC
- FLUX DENSITY; MAIN SEQUENCE STARS; MOTION; SOLAR ACTIVITY; STARS; STARSPOTS; STELLAR ACTIVITY; VARIATIONS