Lab 06: Magnetopause Compression and Ring-Current Energy

Compute magnetopause standoff distance across real solar wind conditions and ring-current energy for two real/historical geomagnetic storms.

Apparatus and Setup

This lab computes the magnetopause standoff distance across a range of real published solar wind conditions (Lecture 11), then computes ring-current energy via the Dessler-Parker-Sckopke relation for both the real 6 September 2017 storm and the Carrington Event's estimated range (Lecture 12).

Materials and Data

Conditionn (cm^-3)v (km/s)
Quiet solar wind6400
Fast (coronal-hole) wind3700
CME sheath (storm)10800

All level 2, standard published OMNI-database climatological/storm-time values. Dst values: Sept 2017=-142 nT (level 2); Carrington range -800 to -1750 nT (live-verified this session).

Procedure

  1. Compute the magnetopause standoff distance for all three solar wind conditions and confirm the quiet and storm values match Lecture 11's stated values.
  2. Compute the dynamic-pressure enhancement factor (storm/quiet) and confirm the standoff-distance reduction is proportionally much smaller, illustrating the one-sixth-power scaling.
  3. Compute the dynamic-pressure enhancement factor that would be required to compress the magnetopause exactly to geosynchronous orbit (6.6 R_E), starting from the quiet-wind dynamic pressure.
  4. Compute ring-current energy (DPS relation) for the real 2017 storm and for both ends of the Carrington Dst range, and tabulate all three alongside their ratio to the 2017 value.

Analysis and Uncertainty

Discuss why the Carrington Event's ring-current-energy range should be presented as a range with an explicit factor-of-two-plus spread (reflecting genuine, disclosed historical-reconstruction uncertainty), not collapsed to a single "best" number.

Deliverables

Assessment Criteria

References and Provenance