The solar chromosphere at high resolution with IBIS. IV. Dual-line evidence of heating in chromospheric network
The solar continuum intensity distribution: Settling the conflict between observations and simulations
The Solar Cycle: A new prediction technique based on logarithmic values
The solar energetic balance revisited by young solar analogs, helioseismology and neutrinos
The Solar Flare Chlorine Abundance from RESIK X-ray Spectra
The Solar Flare Iron Abundance
The Solar Flare Sulphur Abundance from RESIK Observations
The solar magnetic field
The solar magnetic field since 1700: I. Characteristics of sunspot group emergence and reconstruction of the butterfly diagram
The solar magnetic field since 1700: II. Physical reconstruction of total, polar and open flux
The Solar Microwave Flux and the Sunspot Number
The Solar Neighborhood XXIII CCD Photometric Distance Estimates of SCR Targets -- 77 M Dwarf Systems within 25 Parsecs
The Solar Neighborhood XXIV. Parallax Results from the CTIOPI 0.9-m Program: Stars with $μ$ $\ge$ 1\farcs0 yr$^{-1}$ (MOTION Sample) and Subdwarfs
The Solar Neighborhood XXV: Discovery of New Proper Motion Stars with 0.40 "/yr > mu > 0.18 "/yr between Declinations -47 degrees and 00 degrees
The Solar Neighborhood XXVII: Discovery of New Proper Motion Stars with mu > 0.18 "/yr in the Southern Sky with 16.5 > R_59F > 18.0
The Solar Neighborhood. XXII. Parallax Results from the CTIOPI 0.9m Program: Trigonometric Parallaxes of 64 Nearby Systems with 0\farcs5 $\leq μ\leq$ 1\farcs0 yr$^{-1}$ (SLOWMO sample)
The Solar Neighborhood. XXVI. AP Col: The Closest (8.4 pc) Pre-Main-Sequence Star
The Solar Orbiter mission and its prospects for helioseismology
The solar photospheric abundance of carbon.Analysis of atomic carbon lines with the CO5BOLD solar model
The solar photospheric abundance of zirconium