Origin of the Solar Rotation Harmonics Seen in the EUV and UV Irradiance

• Published in: Solar physics Vol. 296; no. 11
• Main Authors: Giono, G., Zender, J. J., Kariyappa, R., Damé, L.
• Format: Journal Article
• Language: English
• Published: Dordrecht Springer Netherlands 01-11-2021; Springer Nature B.V; Springer Verlag
• Subjects: Algorithms; Astrophysics; Astrophysics and Astroparticles; Atmospheric Sciences; Chromosphere; Clustering; Corona; Coronal holes; EUV and UV radiation; Feature extraction; Higher harmonics; Image segmentation; Irradiance; Periodicities; Periodicity; Photosphere; Physics; Physics and Astronomy; Power spectral density; Sciences of the Universe; Segmentation; Solar activity; Solar and Stellar Astrophysics; Solar EUV; Solar images; Solar irradiance; Solar limb; Solar observatories; Solar physics; Solar rotation; Solar surface; Space Exploration and Astronautics; Space Sciences (including Extraterrestrial Physics; Time series; Ultraviolet radiation; Segmentation; EUV and UV radiation; Periodicity; EUV radiation; UV Radiation
• ISSN: 0038-0938; 1573-093X; 1573-093X
• DOI: 10.1007/s11207-021-01918-x

Long-term periodicities in the solar irradiance are often observed with periods proportional to the solar rotational period of 27 days. These periods are linked either to some internal mechanism in the Sun or said to be higher harmonics of the rotation without further discussion of their origin. In this article, the origin of the peaks in periodicities seen in the solar extreme ultraviolet (EUV) and ultraviolet (UV) irradiance around the 7, 9, and 14 days periods is discussed. Maps of the active regions and coronal holes are produced from six images per day using the Spatial Possibilistic Clustering Algorithm (SPoCA), a segmentation algorithm. Spectral irradiance at coronal, transition-region/chromospheric, and photospheric levels are extracted for each feature as well as for the full disk by applying the maps to full-disk images (at 19.3, 30.4, and 170 nm sampling in the corona/hot flare plasma, the chromosphere/transition region, and the photosphere, respectively) from the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO) from January 2011 to December 2018. The peaks in periodicities at 7, 9, and 14 days as well as the solar rotation around 27 days can be seen in almost all of the solar irradiance time series. The segmentation also provided time series of the active regions and coronal holes visible area (i.e. in the area observed in the AIA images, not corrected for the line-of-sight effect with respect to the solar surface), which also show similar peaks in periodicities, indicating that the periodicities are due to the change in area of the features on the solar disk rather than to their absolute irradiance. A simple model was created to reproduce the power spectral density of the area covered by active regions also showing the same peaks in periodicities. Segmentation of solar images allows us to determine that the peaks in periodicities seen in solar EUV/UV irradiance from a few days to a month are due to the change in area of the solar features, in particular, active regions, as they are the main contributors to the total full-disk irradiance variability. The higher harmonics of the solar rotation are caused by the clipping of the area signal as the regions rotate behind the solar limb.