Sami K. Solanki

TL;DR: A reconstruction of the sunspot number covering the past 11,400 years is reported, based on dendrochronologically dated radiocarbon concentrations, and it is pointed out that solar variability is unlikely to have been the dominant cause of the strong warming during the past three decades.

TL;DR: The axion-photon coupling strength of the CERN Axion Solar Telescope (CAST) was shown to be at least 0.02$ eV in the first vacuum phase (2003-2004) with low-background x-ray detectors and a new xray telescope as mentioned in this paper.

TL;DR: Sunspots are the most readily visible manifestations of solar magnetic field concentrations and their interaction with the Sun's plasma as mentioned in this paper, and their internal structure has been extensively studied for almost 400 years and their magnetic nature has been known since 1908.

TL;DR: In this article, the authors describe the approach taken in defining the scenarios used in the PMIP3, document the forcing reconstructions and discuss likely implications and discuss the likely implications.

TL;DR: An overview of the observational and the theoretical methods used to investigate solar magnetic fields is given in this paper, which includes an introduction to the Stokes parameters, their radiative transfer in the presence of a magnetic field, and empirical techniques used to measure various properties of solar magnetic features.