Problems
1. A more conservative dB/dt estimate 15 points
Suppose a more conservative reanalysis found the Carrington-era field-change rate to be only 500 nT/minute (rather than the >700 nT/min value used in the lab), still compared to the modern 350-400 nT/minute benchmark (use 375 nT/min as the benchmark's midpoint). Recompute the dB/dt ratio and the implied sqrt-scaling GIC factor, and compare both to the lab's original values.
2. Full chain for a different bracketing event 10 points
Using this course's seven-unit framework (as tabulated in the lab for the 6 September 2017 event), briefly identify what the equivalent Unit 6 (Dst/magnetosphere) quantity would be if this course instead used the Carrington Event as the primary running case study rather than as a comparison point, and state which one of its two published Dst estimates you would choose to headline and why.
3. GIC scaling with grid length 15 points
A simple resistive model predicts total GIC in a power line scales linearly with both the induced geoelectric field and the line's length. If a regional grid operator doubles the length of a vulnerable transmission line (through a grid expansion) without changing anything else, state, using this simple scaling, what happens to the GIC magnitude for a fixed geoelectric field, and connect this to why grid operators in high-latitude regions (like Quebec) have historically been more concerned about GIC risk than operators of shorter, lower-latitude grids.
4. Course-long synthesis 10 points
In two to three sentences, describe the complete physical chain this course has derived from the solar interior (Lecture 01) to a real ground-based technological impact (Lecture 14), naming at least four of the seven thematic units in the correct order.
OpenStax Companion Reading
OpenStax Astronomy 2e (local extracted reference copy: references/openstax-astronomy-2e-extracted.txt) covers the Sun in Chapter 15 ("The Sun: A Garden-Variety Star"): 15.1 The Structure and Composition of the Sun, 15.2 The Solar Cycle, and 15.3 Solar Activity above the Photosphere. Chapter 15’s section numbering was cross-checked directly against its own embedded figure numbering this session (Figures 15.1 through 15.24 all appear under their matching section headers with no offset), so this citation is verified against the local extracted text rather than extrapolated by analogy from a prior course. OpenStax’s treatment throughout Chapter 15 is descriptive and qualitative; nearly every quantitative derivation in this course (the hydrostatic solar-atmosphere/scale-height argument, the sunspot magnetic-pressure balance, the Parker solar-wind critical-point argument and its numerical transonic solution, flare free-energy budgets, the Chapman-Ferraro magnetopause standoff distance, and the Dessler-Parker-Sckopke ring-current/Dst relation) goes well beyond OpenStax Astronomy 2e’s introductory level; each lecture states explicitly where this course extends beyond the assigned reading.