Published March 10, 2012 | Version v1
Journal article

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/747/2/135

Additional 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