Expand description
Plasmoid perturbation analysis for SOLAR LINE.
Models the trajectory perturbation from a plasmoid encounter in the Uranus magnetosphere (EP04). Distinguishes between:
- Radiation effect (biological): modeled elsewhere (EP04 report)
- Momentum effect (trajectory): modeled here
Based on DiBraccio & Gershman (2019) Voyager 2 observations:
- Plasmoid dimensions: ~200,000 km × 400,000 km
- Composition: primarily ionized hydrogen
- Mass loss rate: ~0.007 kg/s (implies low density)
- Magnetic field: closed loop topology
Key physics:
- Ram pressure: P_ram = 0.5 × ρ × v²
- Magnetic pressure: P_mag = B² / (2μ₀)
- Force on ship: F = P × A_cross (cross-sectional area)
- Impulse: J = F × Δt (transit duration)
- Velocity change: Δv = J / m_ship
Structs§
- Plasmoid
Perturbation - Results of a plasmoid perturbation analysis.
Constants§
- MU_0 🔒
- Permeability of free space (H/m = kg⋅m/A²/s²)
- PROTON_
MASS_ 🔒KG - Proton mass (kg) for hydrogen plasma density calculations
Functions§
- correction_
dv_ m_ s - Course-correction ΔV needed to compensate for a perturbation.
- magnetic_
pressure_ pa - Magnetic pressure (Pa) from a magnetic field.
- miss_
distance_ from_ perturbation_ km - Miss distance from a velocity perturbation over remaining travel time.
- number_
density_ to_ mass - Plasma number density to mass density conversion.
- plasmoid_
force_ n - Force on spacecraft from combined magnetic and ram pressure.
- plasmoid_
perturbation - Full plasmoid perturbation analysis.
- ram_
pressure_ pa - Ram pressure (Pa) from bulk plasma flow.
- uranus_
plasmoid_ scenarios - Parameter scenarios for Uranus plasmoid analysis.
- velocity_
perturbation_ m_ s - Velocity perturbation from plasmoid encounter.