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Resources by Speaker

Please view the presentations and videos form the lectures given at the Heliophysics Summer Schools, sorted by speaker last name.

 

Nick Achilleos
Year Presentations
Planetary Magnetospheres Homework Solution
Introducing the Seasons of the Sun-Planetary System Connections
  • Textbook I, Chapter 2
  • Textbook I, Chapter 13
  • Textbook II, Chapter 2
  • Textbook III, Chapter 11
Vladimir Airapetian
Year Presentations
Comparative Heliophysics
  • Textbook I, Chapter 13
Caspar M. Ammann
Year Presentations
Climate Models of Earth and Planets
Solar Variability and Earth’s Climate
Nick Arge
Year Presentations
Model Inputs for Solar Models

Video from presentation: The Solar Magnetic Field

Tom Ayres
Year Presentations
Observing/Measuring Solar/Stellar Activity and Solar/Stellar Wind
  • Textbook II, Chapter 4
Fran Bagenal
Year Presentations
Planetary Magnetospheres
  • Textbook I, Chapter 10
  • Textbook I, Chapter 13
Planetary Magnetospheres (pdf)
  • Textbook I, Chapter 10
  • Textbook I, Chapter 13
Planetary Magnetic Fields - PDFPlanetary Magnetic Fields - PPT
Introduction to Magnetospheric Physics 1Introduction to Magnetospheric Physics 2
  • Textbook I, Chapter 10
  • Textbook I, Chapter 13
  • Textbook II, Chapter 10
Homework Solution
Comparative Magnetospheres: Planets and Their Satellites
  • Textbook I, Chapter 10
  • Textbook I, Chapter 13
Homework
Dynamos and Magnetospheres of the Planets
  • Textbook I, Chapter 13
  • Textbook III, Chapter 7
Formation & Habitability of Planets
  • Textbook III, Chapter 4
Homework
A Casebook of Universal Plasma Processes 1A Casebook of Universal Plasma Processes 2
Daniel Baker
Year Presentations
Couplings with Magnetospheres: Missions Throughout the Heliosphere
  • Textbook II, Chapter 4
Energetic Particles and Their Impacts Around the Heliosphere
  • Textbook II, Chapter 2
  • Textbook II, Chapter 13
  • Textbook II, Chapter 14
An Overview of Heliophysical Exploration
  • Textbook I, Chapter 2
Space Weather Effects - PPSpace Weather Effects - PDF
  • Textbook II, Chapter 14
Stuart Bale
Year Presentations
Calculating Quantities: Plasma and Field Parameters
Stellar and Solar Winds
  • Textbook I, Chapter 9
  • Textbook III, Chapter 8
Timothy Bastian
Year Presentations
Radiative Signatures of Energetic Particles
  • Textbook II, Chapter 4
Homework
Juerg Beer
Year Presentations
Evidence of external influences on planetary climates
Amitava Bhattacharjee
Year Presentations
Dynamo Theory Basics

Start video at 1:28:28

Earth and Planetary Magnetospheres

Start video at 1:16:28

Particle Energization

Start Video at 0:04:00

Core Lecture 2: Kinetic Theory
Magnetic Reconnection
  • Textbook I, Chapter 5
  • Textbook II, Chapter 10
Explosive Events: CMEs, Flares and Substorms
  • Textbook II, Chapter 5
  • Textbook II, Chapter 6
Dynamo Theory: Basics
  • Textbook I, Chapter 3
  • Textbook III, Chapter 6
Turbulence in Fluids and Space Plasmas
  • Textbook I, Chapter 7
Dynamo Theory: Basics
  • Textbook I, Chapter 3
  • Textbook III, Chapter 6
Large-Scale Instabilities
Magnetic Reconnection and Energy Conversions
  • Textbook II, Chapter 10
Basic Plasma Concepts and Models
Magnetic Reconnection
  • Textbook I, Chapter 4
  • Textbook I, Chapter 5
  • Textbook II, Chapter 5
  • Textbook II, Chapter 6
Homework Solution
Basic Plasma Concepts and Models
  • Textbook II, Chapter 11
Introductory Lecture I: Basic Plasma Concepts/Plasma Models
Doug Biesecker
Year Presentations
Effects of Space Weather & Mitigation Strategies
  • Textbook II, Chapter 2
  • Textbook II, Chapter 13
  • Textbook II, Chapter 14
Forecasting Space Weather Events
Mario Bisi
Year Presentations
Planetary and Solar Radio Occultation/ScintillationsPlanetary and Solar Radio Occultation/Scintillations: Additional Material Brief Quasar History Twinkle-Twinkle
Tom Bogdan
Year Presentations
A Gentle Introduction to Heliophysics
  • Textbook I, Chapter 2
David Boteler
Year Presentations
The Impact of Space Weather on the Electric Power Grid
  • Textbook II, Chapter 2
Stephen Bougher
Year Presentations
ITM Physics of Terrestrial Planets (Including GMD Couplings from Above and Atmospheric from Below)
  • Textbook I, Chapter 12
  • Textbook II, Chapter 12
  • Textbook III, Chapter 13
  • Textbook III, Chapter 14
Homework
David Brain
Year Presentations
Planetary Atmospheres and Habitability
Climates of Terrestrial Planets 1Climates of Terrestrial Planets 2
  • Textbook III, Chapter 4
  • Textbook IV, Chapter 8
Student Brainstorming
Year Presentations
Student Brainstorming
Donald Brownlee
Year Presentations
Planetary HabitabilityThe Drake Equation
David Burgess
Year Presentations
Shocks and Energetic Particles: Corona, Wind, Planets, Solar System
  • Textbook II, Chapter 7
  • Textbook II, Chapter 8
Homework Solution
Ben Chandran
Year Presentations
Solar Wind Acceleration and Coronal Heating
Solar Wind: Structure and Turbulence
  • Textbook I, Chapter 7
  • Textbook I, Chapter 9
  • Textbook III, Chapter 9
Solar Wind: Particle Distribution Functions
  • Textbook II, Chapter 8
  • Textbook II, Chapter 9
  • Textbook IV, Chapter 12
Introduction to Turbulence and Heating in the Solar Wind
  • Textbook I, Chapter 7
Homework
Paul Charbonneau
Year Presentations
Stellar Dynamos
  • Textbook I, Chapter 3
  • Textbook III, Chapter 5
  • Textbook III, Chapter 6
Solar and Stellar Dynamo Models
Subhamoy Chatterjee
Year Presentations
Where does AI/ML stand in the domain of Heliophysics
Mark Cheung
Year Presentations
Solar Data
Solar Data Part 2
Ulrich Christensen
Year Presentations
Planetary Magnetic Fields and Dynamos
Christina Cohen
Year Presentations
SEP’s and Other Energetic Particles
High Energy Particle Telescopes
Role of Instrument Release NotesCalibration and Measurement Algorithms Document (CMAD) Magnetospheric Multiscale (MMS) Project Data Management Plan
Core Lecture Activities: SEP's and Space Weather Impacts
Ofer Cohen
Year Presentations
Evolution on Short and Long Time Scales
  • Textbook IV, Chapter 2
  • Textbook IV, Chapter 4
Coronae, Heliospheres and Astrospheres
  • Textbook I, Chapter 2
  • Textbook IV, Chapter 1
  • Textbook IV, Chapter 3
Comparative Heliophysics
  • Textbook I, Chapter 2
  • Textbook IV, Chapter 1
Effects of Stellar Eruptions Throughout Astrospheres
  • Textbook II, Chapter 7
  • Textbook IV, Chapter 4
Homework
Community Coordinated Modeling Center
Year Presentations
Anthea Jane Coster
Year Presentations
Review of Ionosphere Physics
ISR & Distributed GPS
Thomas Crowley
Year Presentations
A Vintage 2009 Assessment of the Sun-Climate Connection in Paleoclimate Records
Mihir Desai
Year Presentations
Energetic Particles from Solar Explosions
Krauss-Varban Dietmar
Year Presentations
ECP II: Shock Acceleration
  • Textbook II, Chapter 8
Lab: Hybrid Simulations: Numerical Details and Current Applications
Chuanfei Dong
Year Presentations
Living with Stars and Societal Relevance
  • Textbook III, Chapter 4
  • Textbook III, Chapter 11
Eric Donovan
Year Presentations
The Substorm: An Introduction to the Topic in the THEMIS EraThe Substorm: An Introduction to the Topic in the THEMIS Era Primer
  • Textbook II, Chapter 10
  • Textbook II, Chapter 12
Homework
John Dorelli
Year Presentations
Earth’s Magnetosphere
  • Textbook I, Chapter 10
  • Textbook I, Chapter 11
  • Textbook II, Chapter 10
Homework
Robert Ergun
Year Presentations
Magnetosphere: Reconnection & Substorms, Part 1
  • Textbook II, Chapter 2
  • Textbook II, Chapter 10
Magnetopshere: Reconnection & Substorms Part 2
Stefan Eriksson
Year Presentations
Calculation Using Spacecraft Constellations: MMS
Nicholas Featherstone
Year Presentations
Large-Scale Dynamics of the Solar Interior
Stellar Dynamos
  • Textbook III, Chapter 5
  • Textbook III, Chapter 6
Planetary Dynamos
  • Textbook III, Chapter 7
  • Textbook IV, Chapter 6
Debra Fischer
Year Presentations
Characteristics of Planetary Systems 1Characteristics of Planetary Systems 2
  • Textbook III, Chapter 3
  • Textbook IV, Chapter 5
Terry Forbes
Year Presentations
Magnetic Energy Conversion Processes in the Sun and Planets
  • Textbook II, Chapter 5
  • Textbook II, Chapter 6
  • Textbook II, Chapter 10
Homework Solution
Models of Flares and CMEs
  • Textbook I, Chapter 5
  • Textbook II, Chapter 6
Homework
ECP (Energy Conversion Processes) I: Buildup to Instability Then Explosive Conversion
  • Textbook II, Chapter 6
Magnetic ReconnectionCME's and Flares
  • Textbook I, Chapter 5
Kevin Forbes
Year Presentations
Establishing the Economic Impacts of Space Weather: The Case of Electricity
  • Textbook II, Chapter 2
John Foster
Year Presentations
Geospace Variability Through the Solar Cycle 1 Geospace Variability Through the Solar Cycle 2
Tim Fuller-Rowell
Year Presentations
Earth's Ionosphere and Atmosphere
Space Weather in the Upper Atmosphere
  • Textbook II, Chapter 10
  • Textbook II, Chapter 11
Ionosphere thermosphere response
  • Textbook II, Chapter 12
Homework Solution
EM Flare Radiation and Atmospheric Response: ITM and Chromosphere
  • Textbook II, Chapter 12
Christine Gabrielse
Year Presentations
Magnetosphere Data
Magnetosphere Data Part 2
Marina Galand
Year Presentations
Planetary Outer Atmospheres: Interfaces from Atmospheres to Magnetospheres
  • Textbook I, Chapter 11
Homework
Michael Gehmeyr
Year Presentations
Introduction to CISM_DX and Overview of OpenDX
Joe Giacalone
Year Presentations
Solar Wind Modeling Part 2
Solar Wind Modeling
Aspects of the Physics of High-Energy Charged Particles in the Heliopshere

Start video at 49:40

Galactic Cosmic Rays: Sources, Propagation, Entry Throughout Solar System Galactic Cosmic Rays: Sources, Propagation, Entry Throughout Solar System
  • Textbook II, Chapter 11
  • Textbook III, Chapter 9
Homework
Sarah Gibson
Year Presentations
  • Textbook I, Chapter 2
  • Textbook II, Chapter 2
Gary Glatzmaier
Year Presentations
Planetary Dynamo(s) and Their Seasons 1Planetary Dynamo(s) and Their Seasons 2
  • Textbook I, Chapter 3
Goerge Gloeckler
Year Presentations
Energetic Particles and their Detection in Situ (Particle Detectors) 1Energetic Particles and their Detection in Situ (Particle Detectors) 2 Energetic Particles and their Detection in Situ (Particle Detectors) 3
  • Textbook II, Chapter 3
Tamas Gombosi
Year Presentations
Introducing Heliophysics from the Perspective of Universal Processes
  • Textbook II, Chapter 1

Homework is embedded in Video 2

Jack Gosling
Year Presentations
Structure and Evolution of the Three Dimensional Solar Wind
  • Textbook I, Chapter 9
Homework Solution
J. Grebowsky
Year Presentations
IT Science Overlay
Janet Green
Year Presentations
Space Weather: How Does it Impact Satellites and Power Grids?

Start video at 2:03:13

ECP II: Energization of Trapped Particles in Planetary Radiation Belts
  • Textbook II, Chapter 11
Nicholas Gross
Year Presentations
Lab 1: Expert Group Summary
Lab 4: Ionosphere Lab Part 2
Lab 1: Jigsaw Groups
Lab 1: Jigsaw Groups Part 2
Lab 3: Review of Magnetosphere Lab Results
Core Lecture Activities: Solar Interior
Lab 3: Comparative Magnetospheres
Lab 2: Global Structure of the Solar Wind Part 1
Lab 2: Global Structure of the Solar Wind Part 2
Lab 4: Ionosphere Lab Part 1
Lab 2: Solar Dynamos
Lab 5: Variations in Solar IrradianceLab 6: Exploring Ionosphere Structures
Lab 1: Tracking a Solar Storm
Lab 3: Solar Wind
Lab 4: Comparative Magnetospheres
Lab 1: SWx Events
Lab 2: Solar Dynamo
Lab 3: Solar Wind
Lab 5: Comparative Magnetospheres

Lab 1: Sun to Earth Storms
Lab 2: Solar Dynamo/Stellar Dynamos
Lab 3: Sources of Solar Spectral Irradiance
Lab 4: Solar Wind Properties Through the Solar Cycle
Lab 5: Magneospheric Dipole

Lab 1: Tracking a Solar Storm: - Expert-Jigsaw Analysis
Lab 2: Solar Wind Variation Throughout the Heliosphere
Lab 3a: Magnetosphere 1 - A Different Magnetosphere
Lab 3b: Magnetosphehere 2 - A Magnetosphere in Different Places
Lab 4: Simple Comparative Ionospheres Using the Chapman Layer
Lab 3: Magnetosphere 1 - A Different Magnetosphere
Lab 4: Magnetosphere 2 - A Magnetospshere in Different Places
Lab 5: Ionospheres
Lab 1: Tracking a Storm
Lab 2: Solar Wind Variation Throughout the Heliosphere
Lab 1: Investigating the Magnetosphere
Lab 2: The Dynamic Magnetosphere
Lab 3: Solar Activity
Lab 4: Exploring the Structure of the Solar Wind
Lika Guhathakurta
Year Presentations
Review the Heliophysics Observatory
Madhulika Guhathakurta
Year Presentations
Heliosphere Division Snapshot
Next Generation Radiation Characterization from Aviation Altitude to Deep Space

Video starts at 1:12:35

Artificial Intelligence for Space Exploration and All Humankind
Eclipse & Comparative Heliophysics
  • Textbook I, Chapter 2
  • Textbook IV, Chapter 1
Comparative Heliophysics
  • Textbook I, Chapter 13
General Introduction to Heliophysics: Science
  • Textbook I, Chapter 1
  • Textbook I, Chapter 2
Lika Guhathakurta, Ryan McGranaghan, Andres Munoz-Jaramillo
Year Presentations
Big DataArtificial Intelligence for Space Exploration and All Humankind Applications of Deep Learning in Heliophysics
Viggo Hansteen
Year Presentations
The Solar AtmosphereThermally Driven Winds
  • Textbook I, Chapter 8
  • Textbook I, Chapter 9
Mike Hartinger
Year Presentations
Global Structure of the Magnetosphere
Plasma Instruments and Magnetometers
Lee Hartmann
Year Presentations
Formation of Stars and Their Planets
Rod Heelis
Year Presentations
Introduction to ITM Processes
  • Textbook I, Chapter 12
  • Textbook II, Chapter 12
  • Textbook III, Chapter 13
  • Textbook III, Chapter 14
Homework
Mihaly Horanyi
Year Presentations
Dusty Plasmas in the Solar System Homework
Hugh Hudson
Year Presentations
Observations of Solar and Stellar Eruptions, Flares, and Jets
  • Textbook II, Chapter 5
Thomas Immel
Year Presentations
Ionosphere Part 2
Ionosphere Part 1
  • Textbook I, Chapter 12
  • Textbook III, Chapter 13
  • Textbook IV, Chapter 8
Norbert Jakowski
Year Presentations
Radio Wave Propagation for Communication and Probing; Ionospheric Scintillation
Allison Jaynes
Year Presentations
Calculating Quantities: Energetic Particles
Randy Jokipii
Year Presentations
Cosmic Rays
  • Textbook II, Chapter 9
Homework
The Evolving Heliosphere and its Particle Environment
  • Textbook II, Chapter 9
  • Textbook III, Chapter 3
  • Textbook III, Chapter 8
  • Textbook III, Chapter 9
Homework Solution
Philip Judge
Year Presentations
Physics of the Solar Chromosphere
  • Textbook I, Chapter 12
Homework
Justin Kasper
Year Presentations
The Solar Wind
  • Textbook III, Chapter 8
Homework Solution
Mona Kessel
Year Presentations
Margaret Kivelson
Year Presentations
Interaction of Moons, Asteroids, & Comets with their Surroundings
  • Textbook IV, Chapter 10
Homework
David Klumpar
Year Presentations
Detection of Energetic Particles
  • Textbook II, Chapter 3
Homework
Delores Knipp
Year Presentations
Geomagnetic Storms: Great Storms Over the Centuries

Start video at 0:36:00

Geomagnetic Storms: Classical Views & Developing Views

Video: Bursty Bulk Flow

Greg Kopp
Year Presentations
Solar Spectral Irradiance: Measurements and Models
  • Textbook III, Chapter 10
Solar Irradiances
  • Textbook III, Chapter 10
Solar Variability and Earth’s Climate
  • Textbook III, Chapter 11
  • Textbook III, Chapter 12
Janet Kozyra
Year Presentations
The Complete Disturbance: Energy Transport
  • Textbook I, Chapter 2
Norbert Krupp
Year Presentations
Comparative Energetic Particle Environments (SEP/GCR/Local)
Enrico Landi
Year Presentations
Viewing the Sun Across the EM Spectrum
Judith Lean
Year Presentations
Solar Total and Spectral Irradiance Measurements and Models: A Users Guide
Marty Lee
Year Presentations
Acceleration and Heating in the Solar Wind (pdf)Cosmic Rays
  • Textbook I, Chapter 9
Energetic Particles in the Heliosphere (pdf)
  • Textbook II, Chapter 9
Particle Acceleration in Shocks
  • Textbook I, Chapter 8
  • Textbook II, Chapter 8
Homework Solution
Sue Lepri
Year Presentations
Solar Wind Data
Solar Wind Data Part 2
Michael Liemohn
Year Presentations
Energization of Trapped Particles
  • Textbook II, Chapter 11
Homework
Dana Longcope
Year Presentations
Why Do the Earth and Sun Have Magnetic Fields?
Overview of Cycles and Long Term Variability in the Heliopshere
Why Do the Earth and Planets Have an Ionosphere and Magnetosphere
Heliophysics Core Lecture Review: Why does the Sun have a Corona and Wind?
Heliophysics Core Lecture Review: Why do the Earth & Planets have Ionospheres? Magnetospheres?
Solar Flares
Core 3:Ionosphere-Thermosphere-Mesosphere Focus
Orbital Mechanics
Core Lecture 1: Why does the Sun have a Corona and Wind?
Why do the Earth & Planets have Ionospheres? Magnetospheres?
  • Textbook I, Chapter 10
  • Textbook I, Chapter 11
  • Textbook I, Chapter 12
  • Textbook II, Chapter 11
  • Textbook III, Chapter 13
  • Textbook IV, Chapter 8
Why do Sun and Planets have Magnetic Fields?
  • Textbook I, Chapter 3
  • Textbook III, Chapter 2
  • Textbook III, Chapter 6
  • Textbook III, Chapter 7
  • Textbook IV, Chapter 6
Why does the Sun Have a Corona and a Wind?
  • Textbook I, Chapter 9
  • Textbook III, Chapter 8
  • Textbook IV, Chapter 3
Why Does the Earth Have a Magnetosphere, Radiation Belts & an Ionosphere?
  • Textbook I, Chapter 10
  • Textbook I, Chapter 11
  • Textbook I, Chapter 12
  • Textbook II, Chapter 11
  • Textbook III, Chapter 13
  • Textbook IV, Chapter 8
Why do the Sun and Planets have Magnetic Fields?
  • Textbook I, Chapter 3
  • Textbook III, Chapter 2
  • Textbook III, Chapter 6
  • Textbook III, Chapter 7
  • Textbook IV, Chapter 6
Why is there a Corona and a Wind?
  • Textbook I, Chapter 9
  • Textbook III, Chapter 8
  • Textbook IV, Chapter 3
Why do Sun and Planets Have Magnetic Fields?
  • Textbook I, Chapter 3
  • Textbook III, Chapter 2
  • Textbook III, Chapter 6
  • Textbook III, Chapter 7
  • Textbook IV, Chapter 6
Why is There a Corona & a Wind?
  • Textbook I, Chapter 9
  • Textbook III, Chapter 8
  • Textbook IV, Chapter 3
Solar Flares
  • Textbook II, Chapter 6
Why does the Earth have a Magnetosphere, Radiation Belts & an Ionosphere?
  • Textbook I, Chapter 10
  • Textbook I, Chapter 11
  • Textbook I, Chapter 12
  • Textbook II, Chapter 11
  • Textbook III, Chapter 13
  • Textbook IV, Chapter 8
Shocks in Heliophysics
  • Textbook II, Chapter 7
  • Textbook II, Chapter 8
Homework
Introduction to Heliophysics
Magnetic Reconnection
  • Textbook I, Chapter 1
  • Textbook I, Chapter 4
  • Textbook I, Chapter 5
Magnetic Field Topology
  • Textbook I, Chapter 4
Bill Lotko
Year Presentations
Janet Luhmann
Year Presentations
Solar-Wind Through the Sunspot Cycle, (I)CME Modulations by Eruptive & Explosive Phenomena, and Effects on GCRs 1Solar-Wind Through the Sunspot Cycle, (I)CME Modulations by Eruptive & Explosive Phenomena, and Effects on GCRs 2
Introducing the Seasons of the Sun-Planetary System Connections
  • Textbook I, Chapter 2
  • Textbook II, Chapter 2
Scott McIntosh
Year Presentations
Solar Cycle Prediction

Start video at 1:29:00

Slava Merkin
Year Presentations
Magnetosphere Modeling
Magnetosphere Modeling Part 2
Mark Miesch
Year Presentations
Planetary Fields and Dynamos (pdf)
  • Textbook III, Chapter 7
  • Textbook IV, Chapter 6
Solar Internal Flows and Dynamo Action
  • Textbook III, Chapter 5
  • Textbook III, Chapter 6
Homework

This is an optional homework problem (e-mail Dr. Miesch for solution key).

Solar Convection and the Solar Dynamo
  • Textbook III, Chapter 5
  • Textbook III, Chapter 6
Homework Solution
Lab: Solar Convection and Dynamo
Solar Internal Flows and Dynamo Action
  • Textbook III, Chapter 5
Mark Moldwin
Year Presentations
Calculation Using Spacecraft Constellations: Structure and Scale Size of the Solar Wind
Core Lecture Activities: Why do the planets have a magnetosphere and ionsphere
A Tribute to Parker and Siscoe
Universal Plasma Processes in Heliophysics 1Universal Plasma Processes in Heliophysics 2
  • Textbook II, Chapter 1
Introduction to Heliophysics System Physics: Processes and Environments, Similarities and Differences
  • Textbook I, Chapter 1
  • Textbook I, Chapter 2
  • Textbook II, Chapter 1
  • Textbook III, Chapter 1
Homework
Magnetic Flux Ropes in Space Plasmas
  • Textbook I, Chapter 6
Homework Solution
Luke Moore
Year Presentations
Atmosphere-Ionosphere-Magnetosphere Coupling at the Giant Planet
  • Textbook IV, Chapter 9
Homework
Andres Munoz
Year Presentations
Solar Cycle & Dynamo (including extended minima and maxima), and the Large-Scale Field 1Solar Cycle & Dynamo (including extended minima and maxima), and the Large-Scale Field 2
Bill Murtagh
Year Presentations
Space Weather and its Impacts on Society
General introduction to Heliophysics: Society
  • Textbook II, Chapter 2
  • Textbook II, Chapter 13
  • Textbook II, Chapter 14
NASA
Year Presentations
Sten Odenwald
Year Presentations
Space Weather: Impacts, Mitigation & ForecastingSpace Weather and Its Societal Impacts
  • Textbook II, Chapter 2
Merav Opher
Year Presentations
Structure of the Heliosphere Part 2

Start Video at 51:00

Structure of the Heliosphere Part 1
  • Textbook II, Chapter 7
  • Textbook II, Chapter 8
  • Textbook II, Chapter 9
  • Textbook II, Chapter 11
Shocks in Heliophysics
  • Textbook I, Chapter 7
  • Textbook II, Chapter 7
Homework Solution
The Varieties of Shocks: Coronal, CME, CIR, Heliospheric, and Planetary
Rachel Osten
Year Presentations
Solar Explosive Activity Throughout the Evolution of the Solar System - Introduction ProcessSolar Explosive Activity Throughout the Evolution of the Solar System - Trends With Time
  • Textbook II, Chapter 5
  • Textbook II, Chapter 6
  • Textbook IV, Chapter 2
Homework Solution
Elena Provornikova
Year Presentations
Interstellar Probe

Start Video at 47:20

Jiong Qiu
Year Presentations
CME's And Transients
Matthias Rempel
Year Presentations
Creation and Destruction of Magnetic Fields
  • Textbook I, Chapter 3
Homework Solution
Creation and Destruction of Magnetic Fields 1Creation and Destruction of Magnetic Fields 2
  • Textbook I, Chapter 3
Jon Sample
Year Presentations
In Situ Instruments and Measurements
  • Textbook II, Chapter 3
Neal Savani
Year Presentations
CMEs
  • Textbook II, Chapter 6
  • Textbook IV, Chapter 4
Antonia Savcheva
Year Presentations
Solar Modeling
Solar Modeling Part 2
Karel Schrijver
Year Presentations
Discussion Activities
Proposal Elements
Observations of Stellar Dynamos
  • Textbook I, Chapter 3
  • Textbook III, Chapter 5
  • Textbook III, Chapter 6
Solar Spectral Irradiation & Wind Over Time Scales up to a Decade
  • Textbook I, Chapter 8
  • Textbook I, Chapter 9
  • Textbook III, Chapter 2
  • Textbook III, Chapter 8
  • Textbook III, Chapter 10
Homework Solution
The Solar Atmosphere
  • Textbook II, Chapter 5
  • Textbook II, Chapter 6
  • Textbook III, Chapter 2
Long-Term Evolution of Magnetic Activity of Sun-Like StarsImpact Generated Shockwaves are Proposed for the Origin of Sunspots to Explain the Detected Planetary Correlations with Solar Activity Extreme-Ultraviolet Flare Activity in Late-Type Stars Twenty-Seven Day Recurrences in Terrestrial Magnetic and Solar Activity, 1923-1933 On a Transition from Solar-Like Coronae to Rotation-Dominated Jovian-Like Magnetospheres in Ultracool Main-Sequence Stars
Tutorial: The Magnetic Connection Between the Sun and the Heliosphere
Yuri Shprits
Year Presentations
Radiation Belts
  • Textbook II, Chapter 11
Homework
George Siscoe
Year Presentations
The Palemagnetoshere
Lab: The Chapman-Feraro Problem
Lab: A Tour of the Magnetosphere with CCMC Models
David Siskind
Year Presentations
Aeronomy of Terrestrial Planet Atmospheres
  • Textbook III, Chapter 13
  • Textbook III, Chapter 14
  • Textbook IV, Chapter 7
James Slavin
Year Presentations
Planetary MagnetospheresPlanetary Magnetospheres (part 2)
  • Textbook I, Chapter 10
  • Textbook I, Chapter 13
Chuck Smith
Year Presentations
Turbulence in Space Plasmas
Jan Sojka
Year Presentations
Planetary Ionospheres
  • Textbook III, Chapter 13
  • Textbook IV, Chapter 8
Long-Term Evolution of the Geospace Climate
  • Textbook III, Chapter 2
  • Textbook III, Chapter 14
Long-term Evolution of the Geospace Climate (pdf)
  • Textbook III, Chapter 14

This lecture is actually Jan Sojka's Chapter 14 in Textbook III

Terrestrial Ionospheres (pdf)Terrestrial Ionospheres (animated)
  • Textbook III, Chapter 13
The Ionosphere-Thermosphere
  • Textbook I, Chapter 12
  • Textbook III, Chapter 13
The Earth's IonosphereLong Term Evolution of Geospace Climate
  • Textbook I, Chapter 12
  • Textbook III, Chapter 13
Homework
Introductory Lecture II: An Overview of Space Storms
Long-Term Evolution of the Geospace Climate
Stan Solomon
Year Presentations
Orbital Seasons, Radiative Transport, Ionization, and Chemistry in Planetary Outer Atmospheres
  • Textbook II, Chapter 12
Ionospheres of the Terrestrial Planets
Harlan Spence
Year Presentations
Particle Effects on Humans and Biological Tissues - PPParticle Effects on Humans and Biological Tissues - PDF
  • Textbook II, Chapter 13
Sabine Stanley
Year Presentations
Planetary Fields and Dynamos

Start Video at 1:50:40

Planetary Dynamos: Updates & New Frontiers
  • Textbook I, Chapter 13
  • Textbook III, Chapter 7
Homework Solution
Dynamos in Planets and Stars
  • Textbook I, Chapter 3
  • Textbook III, Chapter 5
  • Textbook III, Chapter 6
  • Textbook III, Chapter 7
Homework
Barbara Thompson
Year Presentations
The Solar Corona and Solar Wind
Kent Tobiska
Year Presentations
Characterizing the Global Aviation Radiation Environment
Impacts of Space Weather
Frank Toffoletto
Year Presentations
Solar Wind/Magnetosphere Coupling
  • Textbook I, Chapter 11
  • Textbook II, Chapter 10
Homework
Lab: Magnetosphere
Solar Wind Magnetosphere CouplingGeomagnetic Storms and Substorms
Alan Tribble
Year Presentations
Particle Interaction with Technology
  • Textbook II, Chapter 14
Lisa Upton
Year Presentations
Solar Cycle Predictions (pdf)
  • Textbook III, Chapter 2
  • Textbook III, Chapter 6
Introduction to the Solar Dynamo
Vytenis Vasyliunas
Year Presentations
Planetary magnetospheres
  • Textbook I, Chapter 10
  • Textbook II, Chapter 10
Homework Solution
Application of ECP I: Magnetic (Sub-)Storms, and Planetary Counterparts
  • Textbook II, Chapter 10
Richard Walterscheid
Year Presentations
Waves in Planetary Atmospheres
  • Textbook III, Chapter 15
Harry Warren
Year Presentations
Solar Spectral Radiance and Their Origins Through Cycles of Solar Magnetism 1Solar Spectral Radiance and Their Origins Through Cycles of Solar Magnetism 2
Dan Welling
Year Presentations
Model Inputs for Magnetosphere Models
Brian Wood/Jeffrey Linsky
Year Presentations
Stellar Winds and Their Interaction with the Variable ISM
  • Textbook III, Chapter 8
  • Textbook III, Chapter 9
  • Textbook IV, Chapter 3
Homework
Matt Zetterren
Year Presentations
Ionosphere Modeling
Ionosphere Modeling Part 2
Shasha Zou
Year Presentations
Ionosphere Data
Ionosphere and Thermosphere Basics