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- NASA's Heliophysics Portfolio (IG-19-018)
- Helioseismology and the Sun's Interior
- SOLAR PHYSICS in the 2020S: DKIST, PARKER SOLAR PROBE, and SOLAR ORBITER AS a MULTI-MESSENGER CONSTELLATION1
- Solar Flares
- Prediction of Arrival Time of Coronal Mass Ejections Ravishankar
- Helioseismology and Solar Abundances
- What Have We Learned from Helioseismology, What Have We Really Learned, and What Do We Aspire to Learn?∗
- Introduction to Solar Physics
- Physics of the Solar Corona an Introduction with Problems and Solutions Markus J Aschwanden Physics of the Solar Corona an Introduction with Problems and Solutions
- The Outer Heliosphere – Solar System's Final Frontier V
- Introduction to Solar Flares
- Solar Wind and Kinetic Heliophysics
- NASA FY13 Budget Estimates--Heliophysics
- The Heliosphere's Interaction with Interstellar Dust 1 The
- 2 Solar Phenomena and Solar Wind 2-1 Study of Energy Build-Up in Solar Flares
- Characterizing Coronal Mass Ejections in Solar Cycle Analysis *1,2Ryan Manuel D
- Heliophysics Division
- The Low Solar Corona and the Stars N
- Solar Neutrinos: Beyond Standard Solar Models Abstract
- The 2020 Senior Review of the Heliophysics Operating Missions
- Why Solar Physics
- 20 HELIOSEISMOLOGY II: Probing the Solar Interior
- Solar Magnetic Atmospheric Effects on Global Helioseismic Oscillations
- Cosmic-Ray Picture of the Heliosphere
- Lecture 9: Instabilities, Solar Flares and Cmes
- Outstanding Problems in Solar Physics Markus J. Aschwanden
- Lecture 9: Solar Activity
- The Solar Orbiter Science Activity Plan Translating Solar and Heliospheric Physics Questions Into Action
- Arxiv:2102.02943V2 [Astro-Ph.SR] 17 Mar 2021 Is Widely Used in Solar Physics for Modeling Emission Lines
- Solar and Heliospheric Physics with the Square Kilometre Array
- Exploring the Sun-Heliosphere Connection Solar Orbiter
- Solar Physics and Terrestrial Effects ⇥ ⇤⌅
- Solar Neutrinos: Where We Are, Where We Are Going1
- The Structure of the Sun
- Heliophysics Living with a Star Program Enabling Science, Technology, and Exploration to Advance Society
- The Properties of the Solar Corona and Its Connection to the Solar Wind
- Causes of Solar Activity
- The Sun As a Laboratory for Plasma Physics
- Standard Solar Model
- Heliophysics the SOLAR and SPACE PHYSICS of a NEW ERA
- Solar Origins of a Strong Stealth CME Detected by Solar Orbiter Jennifer O’Kane1, Lucie M
- Introduction to the Physics of the Sun, Heliosphere and Space Weather
- Helioseismology Lecture Contents
- Solar Interior
- Solar Physics and Instrumentation – Lecture 23 Sunspots
- The Flare Genesis Experiment: Studying the Sun from the Stratosphere
- NASA GSFC Heliophysics Science Division and Space Weather
- Solar Physics Career Brochure
- The Stars Lecture 4: the Sun – a Typical Star
- The Solar Physics Division of the American Astronomical Society
- White Paper for the Heliophysics 2050 Workshop
- A Brief History of Cme Science
- Helioseismology Challenges Models of Solar Convection
- Class Reference: K&R Chapter 3.1 and Links Given in These Slides
- Solar Physics at APL