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Solar Irradiance Variability is Caused by the Magnetic Activity on the Solar Surface
Online Contents | 2017| -
Intensity contrast of solar network and faculae -- II. Implications for solar irradiance modelling
Free accessArXiv | 2021| -
Intensity contrast of solar network and faculae
Free accessII. Implications for solar irradiance modellingEDP Sciences | 2019| -
How faculae and network relate to sunspots, and the implications for solar and stellar brightness variations
Free accessEDP Sciences | 2020| -
How faculae and network relate to sunspots, and the implications for solar and stellar brightness variations
Free accessArXiv | 2020| -
How faculae and network relate to sunspots, and the implications for solar and stellar brightness variations(Corrigendum)
Free accessEDP Sciences | 2020| -
Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI, and SDO/HMI observations
Free accessEDP Sciences | 2014| -
The relationship between bipolar magnetic regions and their sunspots
Free accessEDP Sciences | 2021|
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