The slow-mode nature of compressible wave power in solar wind turbulence
The SN 2008S Progenitor Star: Gone or Again Self-Obscured?
The Soft X-ray Lightcurves of Partially Eclipsed Stellar Flares
The Solar and $α$ Centauri A and B models improved by opacity enhancement - a possible explanation for the oversize cool stars
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)