From the 1 of 9 linked papers with an AI index.
9 papers
Re-evaluating solar irradiance reconstructions: No evidence for large secular trends
Theodosios Chatzistergos, Natalie A. Krivova, Mathew J. Owens +1
The authors reassess solar irradiance reconstructions that previously suggested large secular increases and find that, after correcting the linking of cosmogenic isotope and neutro…
The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates
Emre Isik, Sami K. Solanki, Natalie A. Krivova +1
The rotation-activity relationship of G-type stars results from surface magnetic fields emerging from the interior. How the magnetic flux and its emergence rate scale with rotation…
Cyclic sunspot activity during the first millennium CE as reconstructed from radiocarbon
Ilya Usoskin, Sami K. Solanki, Natalie A. Krivova +1
Context. Solar activity, dominated by the 11-year cyclic evolution, has been observed directly since 1610. Before that, indirect cosmogenic proxy data are used to reconstruct it ov…
Structure and Dynamics of the Sun's Interior Revealed by Helioseismic and Magnetic Imager
Alexander Kosovichev, Sarbani Basu, Yuto Bekki +43
High-resolution helioseismology observations with the Helioseismic and Magnetic Imager (HMI) onboard Solar Dynamics Observatory (SDO) provide a unique three-dimensional view of the…
Revisiting the SATIRE-S irradiance reconstruction: Heritage of Mt Wilson magnetograms and Ca II K observations
Theodosios Chatzistergos, Natalie A. Krivova, Sami K. Solanki +1
Accurate information on long-term variations in solar irradiance, important for understanding the solar influence on Earth's climate, cannot be derived from direct irradiance measu…
Detectability of Solar Rotation Period Across Various Wavelengths
Valeriy Vasilyev, Timo Reinhold, Alexander I. Shapiro +3
The light curves of old G-dwarfs obtained in the visible and near-infrared wavelength ranges are highly irregular. This significantly complicates the detectability of the rotation…