Table 3.
Characteristic parameters of Solar System magnetospheres determining planetary space weather. Adapted from Bagenal (2013) and Krupp (2015).
Solar System body | Magnetopause nose distance | Surface magnetic field at the equator (T) | Dipole tilt1 | Obliquity2 | Plasma sources3 | Plasma composition (main species) | Plasma motion | Plasma β 4 | Lifetime |
---|---|---|---|---|---|---|---|---|---|
Neptune | 24 RN | 0.14 × 10−4 | −47° | 29.6° | Triton (solar wind?) | N+, H+ | Rotation (and solar wind driven?) | 0.2 | days |
Uranus | 25 RU | 0.23 × 10−4 | −59° | 97.9° | Ionosphere (solar wind) | H+ | Solar wind driven and rotation | 0.1 | 1–30 days |
Saturn | 19 RS | 0.22 × 10−4 | −0° | 26.7° | Enceladus (Rings, Tethys, Dione, Titan, solar wind)6 | H2O+, O+, H+ | Rotation | 1–5 | 30–50 days |
Jupiter | 42 RJ | 4.28 × 10−4 | −9.6° | 3.1° | Io, Europa (ionosphere)7 | On+, Sn+, H+ | Rotation | 10–100 | 20–80 days |
Mercury | 1.4–1.6 RM | 2 × 10−7 | +14° | 0° | Solar wind | H+ | Solar wind driven | ~28 | Minutes |
Ganymede | ~2 RG | 7.19 × 10−7 5 | 176° | 0.2° | Jupiter’s magnetosphere (Ganymede’s exosphere) | On+, Sn+, H+ | Corotation (Jupiter’s magnetosphere driven) | 0.49 | Min to hours9 |
The dominant plasma sources are indicated. In parenthesis we indicate the believed secondary plasma sources.
The plasma β parameter is defined as the ratio of plasma pressure to magnetic pressure, β = nkT/(B2/2μ0).
From Kivelson et al. (1996).
Temporal analysis of the auroral power of Ganymede’s footprint reveals variations of different timescales: (a) a 5-h timescale, associated with the periodic flapping of Jupiter’s plasma sheet over Ganymede; (b) a 10–40 min timescale, possibly associated with energetic magnetospheric events, such as plasma injections; (c) a 100-s timescale corresponding to quasi periodic fluctuations, which might relate to bursty reconnections on Ganymede’s magnetopause and/or to the recurrent presence of acceleration structures above Jupiter’s atmosphere. From Grodent et al. (2009).
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