ASTR 370: Lecture and Lab Schedule

14 lectures · 7 labs · 7 problem sets · one semester

Lecture Schedule

#TitleOpenStax Astronomy 2e ReadingPaired Lab/PS
01Solar Structure and Hydrostatic EquilibriumCh. 15.1 (The Structure and Composition of the Sun, descriptive only)Lab 01 / PS 01
02The Solar Atmosphere: Photosphere, Chromosphere, and the CoronaCh. 15.3 (Solar Activity above the Photosphere, descriptive only)
03The Solar Magnetic Field and the 11-Year CycleCh. 15.2 (The Solar Cycle, descriptive only)Lab 02 / PS 02
04Sunspots: Magnetic Pressure Balance and the Wilson DepressionNot in OpenStax; derived from first principles (Spruit 1976; Biermann 1941)
05Solar Flares I: Magnetic Reconnection and Free EnergyCh. 15.3 (Solar Activity above the Photosphere, descriptive only)Lab 03 / PS 03
06Solar Flares II: The 6 September 2017 X9.3 EventNot in OpenStax; real case-study synthesis
07Coronal Mass Ejections: Kinematics and EnergyNot in OpenStax; derived from first principlesLab 04 / PS 04
08The Solar Wind: Parker's Transonic Wind SolutionNot in OpenStax; derived from first principles (Parker 1958)
09Remote Sensing the Sun: Helioseismology and CoronagraphyNot in OpenStax; derived from first principlesLab 05 / PS 05
10In-Situ Heliophysics: Parker Solar ProbeNot in OpenStax; real mission case study
11The Sun-Earth Connection I: Solar Wind Transit and the MagnetopauseNot in OpenStax; derived from first principles (Chapman & Ferraro)Lab 06 / PS 06
12The Sun-Earth Connection II: Geomagnetic Storms and the Dst IndexNot in OpenStax; derived from first principles (Dessler & Parker 1959; Sckopke 1966)
13Space Weather Impacts on Technology I: Satellites and RadiationNot in OpenStax; applied synthesisLab 07 / PS 07
14Space Weather Impacts on Technology II: Power Grids and Course SynthesisNot in OpenStax; applied synthesis and course capstone

Lab Schedule

LabTitleReal Data Source
01Solar Hydrostatic Structure: Scale Heights of the Photosphere and CoronaIAU nominal solar parameters and standard solar model values (standard published, level 2)
02The Solar Cycle and Sunspot Pressure BalanceReal Solar Cycle 24/25 sunspot-number data (live-verified this session, SILSO/WDC-SILSO) and real sunspot umbral field strengths (Solanki 2003)
03Flare Free Energy and the 6 September 2017 Case StudyReal AR 12673 X9.3 flare, CME, and G4-storm data (standard published NOAA/GOES/CDAW/Kyoto WDC values, level 2)
04CME Transit Time and the Parker Wind's Numerical SolutionReal CME LASCO speed and solar wind climatology (standard published, level 2), numerically solved Parker wind equation
05Remote Sensing Geometry and Parker Solar Probe In-Situ PredictionReal Parker Solar Probe perihelion distance and record speed (live-verified this session)
06Magnetopause Compression and Ring-Current EnergyReal solar wind climatology (level 2) and the real 6 September 2017/historic Carrington Event Dst values (level 2 and live-verified this session respectively)
07Capstone: Geomagnetically Induced Currents and the Full Flare-to-Grid ChainThe 2024 Beggan et al. Carrington-era magnetometer reanalysis (live-verified this session) and this course's full seven-unit case-study chain