2019
DOI: 10.1029/2018gl078097
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Sources, Sinks, and Transport of Energetic Electrons Near Saturn's Main Rings

Abstract: The inner boundary of Saturn's electron radiation belts, near the planet's A ring (∼2.27 Rs), is studied using Cassini's proximal orbit measurements. We find that variable convective flows transport energetic electrons to the A ring, which absorbs them instantaneously, forming the inner belt boundary. These flows are also responsible for a variable and longitudinally asymmetric boundary configuration. Prenoon, the boundary oscillates toward and away from the A ring with a 2‐week period. Postnoon, it maps persi… Show more

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Cited by 16 publications
(36 citation statements)
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References 30 publications
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“…Large‐scale variations in the noon‐midnight electric field are known to occur in the dawn‐dusk electric field of Jupiter, triggering fast transport of energetic electrons (Han et al, ; Murakami et al, ). Similar variations at Saturn are hinted by electron belt observations near Saturn's A ring (Roussos et al, ).…”
Section: Discussionsupporting
confidence: 70%
“…Large‐scale variations in the noon‐midnight electric field are known to occur in the dawn‐dusk electric field of Jupiter, triggering fast transport of energetic electrons (Han et al, ; Murakami et al, ). Similar variations at Saturn are hinted by electron belt observations near Saturn's A ring (Roussos et al, ).…”
Section: Discussionsupporting
confidence: 70%
“…All the observations prove the importance of CDR electron transport due to time‐variable local time fixed convective electric fields (Roussos et al, ). The global noon‐to‐midnight electric field remains the best candidate for driving this electron transport process (Andriopoulou et al, ; Wilson et al, ), it causes a quasi‐uniform, dawnward E × B convection flow.…”
Section: Discussionmentioning
confidence: 80%
“…The global noon‐to‐midnight electric field remains the best candidate for driving this electron transport process (Andriopoulou et al, ; Wilson et al, ), it causes a quasi‐uniform, dawnward E × B convection flow. It will shift electrons' circular orbits toward the direction of noon if E < E CDR , or midnight if E > E CDR (Roussos et al, ). As electrons drift on constant μ curves, we traced electrons with the method of Roussos et al (), a guiding center test particle tracing in a dipole field considering a noon‐midnight electric field and corotation.…”
Section: Discussionmentioning
confidence: 99%
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“…Magnetic mapping of the in situ measurements was performed by calculating the L-shell, equatorial pitch angle, and the loss cone through an empirical third-order magnetic field model (24). We define the L-shell value (L) as the distance from the planet (in Saturn radii) that a field line crosses the magnetic equator.…”
Section: Instrumentation and Methodologymentioning
confidence: 99%