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Updated: Jul 5, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
Plasma observations near jupiter: initial results from voyager 2
Summary
Voyager 2
Area of Science:
- Planetary Science
- Space Physics
- Plasma Physics
Background:
- Voyager 2's inbound pass provided crucial data on Jupiter's magnetosphere.
- Previous observations by Voyager 1 established baseline plasma characteristics.
Purpose of the Study:
- To detail Voyager 2's magnetosphere crossings and plasma observations.
- To analyze plasma behavior, composition, and structure within Jupiter's magnetosphere.
Main Methods:
- In-situ measurements of plasma density, intensity, and composition by Voyager 2.
- Analysis of planetary spin modulation to infer plasma sheet geometry.
Main Results:
- Multiple bow shock crossings and magnetospheric entry at specific Jupiter radii.
- Plasma exhibited corotation; densities and intensities comparable to Voyager 1.
- Magnetospheric plasma dominated by heavy ions (mass density ratio ~100:1).
- Observed plasma intensity dropouts near Ganymede, suggesting complex interactions.
- Plasma sheet centered on dipole equator initially, deviating towards rotational equator with distance.
- Plasma sheet's longitudinal position lagged behind the rotating dipole.
Conclusions:
- Voyager 2's data confirm and expand upon previous findings about Jupiter's magnetosphere.
- The magnetosphere's structure and dynamics are influenced by heavy ions and interactions with moons like Ganymede.
- The plasma sheet's complex geometry and behavior provide insights into Jovian magnetospheric processes.
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