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- Surface Gravity As a Diagnostic of Stellar Youth
- The Solar Atmosphere
- The Sun's Atmosphere
- Lecture 2 What Is a Star? a Huge Ball of Ionized Gas (Plasma) Producing
- The Solar Chromosphere: the Inner Frontier of the Heliospheric System
- Solar Radio Bursts and Space Weather
- Lecture 2: Formation of a Stellar Spectrum
- Our Star -- the Sun Lithograph
- Stellar Structure and the Sun 8.1 Stellar Structure Basics How Stars Work • Hydrostatic Equilibrium: Gas and Radiation Pressure Balance the Gravity
- The Sun Structure
- Stellar Magnetic Fields Across the HR Diagram
- First Radio Evidence for Ubiquitous Magnetic Reconnections and Impulsive Heating in the Quiet Solar Corona
- Lecture 6 the Sun: from the Core to the Photosphere
- On the Nature of Nonthermal Radiation from Cosmological
- The Low Solar Corona and the Stars N
- Study of Supernovae Important for Cosmology P
- Searching for and Identifying Pulsars Ryan S
- Asymmetry of Lines in the Spectra of the Sun and Solar-Type Stars
- Lecture 7: Radio Observations of Coronal Mass Ejections I
- Supernova Resonance-Scattering Line Profiles in the Absence of a Photosphere
- Spectra of Supernovae During the Photospheric Phase 31
- Solar Structure (11/16/17)
- Lecture 7: from the Photosphere to the Hot Corona
- Synchronized Observations of Bright Points from the Solar Photosphere to Corona 3
- Lecture 16 - the Solar Surface and Atmosphere O Topics to Be Covered
- “Surface” of the Sun, Called the Photosphere
- The Structure of the Sun
- The Classification of Stellar Spectra Student Manual
- PHYS-633: Introduction to Stellar Astrophysics
- High-Resolution Observations of the Solar Photosphere, Chromosphere, and Transition Region a Database of Coordinated IRIS and SST Observations
- The Solar Atmosphere at Radio Wavelengths
- Radiative Processes, Stellar Atmospheres and Winds
- Exam #2 Review
- Polarimetric Evidence of the First White Dwarf Pulsar: the Binary System AR Scorpii
- The Sun As a Typical Star
- A Model for Redistributing Heat Over the Surface of Irradiated Spider Companions
- How to Observe The
- The Solar Atmosphere
- Connections: Photosphere – Chromosphere - Corona
- Core to Solar Wind: a Stepwise Model for Heating the Solar Corona Claudio Vita-Finzi Earth Sciences, Natural History Museum Cromwell Road, London SW7 5BD, UK
- Studying the Sun
- Distances to Core-Collapse Supernovae
- Applying the Expanding Photosphere and Standardized Candle Methods to Type II-Plateau Supernovae at Cosmologically Significant R
- Solar Interior
- Photosphere Photosynthesis
- Astronomy 101.002 Hour Exam 3 April 13, 2009 Answers Given in BOLD
- Calculating the Sun's Photospheric Temperature, an Undergraduate Physics Laboratory Austin B
- Stellar Magnetic Activity Who’S Active, Who’S Not