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Solar radius

  • Solar Radius Determined from PICARD/SODISM Observations and Extremely Weak Wavelength Dependence in the Visible and the Near-Infrared

    Solar Radius Determined from PICARD/SODISM Observations and Extremely Weak Wavelength Dependence in the Visible and the Near-Infrared

  • 2. Astrophysical Constants and Parameters

    2. Astrophysical Constants and Parameters

  • Apparent and Absolute Magnitudes of Stars: a Simple Formula

    Apparent and Absolute Magnitudes of Stars: a Simple Formula

  • Useful Constants

    Useful Constants

  • PHAS 1102 Physics of the Universe 3 – Magnitudes and Distances

    PHAS 1102 Physics of the Universe 3 – Magnitudes and Distances

  • Arxiv:0908.2624V1 [Astro-Ph.SR] 18 Aug 2009

    Arxiv:0908.2624V1 [Astro-Ph.SR] 18 Aug 2009

  • Solar Radius Determination from Sodism/Picard and HMI/SDO

    Solar Radius Determination from Sodism/Picard and HMI/SDO

  • How Stars Work: • Basic Principles of Stellar Structure • Energy Production • the H-R Diagram

    How Stars Work: • Basic Principles of Stellar Structure • Energy Production • the H-R Diagram

  • Observing the Stars

    Observing the Stars

  • Lectures on Astronomy, Astrophysics, and Cosmology

    Lectures on Astronomy, Astrophysics, and Cosmology

  • A Astronomical Terminology

    A Astronomical Terminology

  • Arxiv:1510.00485V1

    Arxiv:1510.00485V1

  • 44 Closest Stars and How They Compare to Our Sun

    44 Closest Stars and How They Compare to Our Sun

  • The Sun: Its Structure and Energy Generation

    The Sun: Its Structure and Energy Generation

  • How Big Is the Sun: Solar Diameter Changes Over Time J.P

    How Big Is the Sun: Solar Diameter Changes Over Time J.P

  • How Far to a Star ? Astronomical Distances Astronomical Distances

    How Far to a Star ? Astronomical Distances Astronomical Distances

  • Solar Elemental Abundances Table of Contents Summary

    Solar Elemental Abundances Table of Contents Summary

  • Determining the Sizes of Stars Using the H-R Diagram

    Determining the Sizes of Stars Using the H-R Diagram

Top View
  • Determining the Sizes & Distances of Stars Using the H-R Diagram
  • Stars, Galaxies, and Beyond, 2012
  • Transits of Venus and Mercury
  • Resolution B3 on Recommended Nominal Conversion Constants for Selected Solar and Planetary Properties
  • Solar Radius at Sub-Terahertz Frequencies
  • Stellar Structure and the Sun 8.1 Stellar Structure Basics How Stars Work • Hydrostatic Equilibrium: Gas and Radiation Pressure Balance the Gravity
  • AST 110-5: Announcements
  • Astronomical Units
  • Determination of the Size, Distance and Mass of the Sun by High-Resolution Solar Spectroscopy and the Cavendish Experiment
  • Unit 1 Astronomical Scales
  • Distance and Size of a Celestial Body
  • Solar Astrophysical Fundamental Parameters Mustapha Meftah, Abdanour Irbah, Alain Hauchecorne
  • CHAPTER 7 the NATURE of EXOPLANETARY SYSTEMS Now That the Various Methods of Detecting Exoplanets Have Been Described, We Turn to the Results of the Various Searches
  • Solar Radius at Subterahertz Frequencies and Its Relation to Solar Activity F
  • Solar Disc Radius Determined from Observations Made During Eclipses with Bolometric and Photometric Instruments on Board the PICARD Satellite G
  • A Brief History of the Solar Diameter Measurements: a Critical Quality Assessment of the Existing Data
  • IAU 2015 Resolutions
  • GLOSSARY of SOLAR-TERRESTRIAL TERMS a a Index


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