S M Levin
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Explore the profile of S M Levin including associated specialties, affiliations and a list of published articles.
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78
Citations
693
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Recent Articles
1.
Park R, Jacobson R, Gomez Casajus L, Nimmo F, Ermakov A, Keane J, et al.
Nature
. 2024 Dec;
638(8049):69-73.
PMID: 39667409
Io experiences tidal deformation as a result of its eccentric orbit around Jupiter, which provides a primary energy source for Io's continuing volcanic activity and infrared emission. The amount of...
2.
Bolton S, Levin S, Guillot T, Li C, Kaspi Y, Orton G, et al.
Science
. 2021 Oct;
374(6570):968-972.
PMID: 34709937
Jupiter’s atmosphere has a system of zones and belts punctuated by small and large vortices, the largest being the Great Red Spot. How these features change with depth is unknown,...
3.
Haggerty D, Mauk B, Paranicas C, Clark G, Kollmann P, Rymer A, et al.
Geophys Res Lett
. 2019 Nov;
46(16):9397-9404.
PMID: 31762519
The polar orbit of Juno at Jupiter provides a unique opportunity to observe high-latitude energetic particle injections. We measure energy-dispersed impulsive injections of protons and electrons. Ion injection signatures are...
4.
Iess L, Folkner W, Durante D, Parisi M, Kaspi Y, Galanti E, et al.
Nature
. 2018 Mar;
555(7695):220-222.
PMID: 29517001
The gravity harmonics of a fluid, rotating planet can be decomposed into static components arising from solid-body rotation and dynamic components arising from flows. In the absence of internal dynamics,...
5.
Guillot T, Miguel Y, Militzer B, Hubbard W, Kaspi Y, Galanti E, et al.
Nature
. 2018 Mar;
555(7695):227-230.
PMID: 29517000
Jupiter's atmosphere is rotating differentially, with zones and belts rotating at speeds that differ by up to 100 metres per second. Whether this is also true of the gas giant's...
6.
Kaspi Y, Galanti E, Hubbard W, Stevenson D, Bolton S, Iess L, et al.
Nature
. 2018 Mar;
555(7695):223-226.
PMID: 29516995
The depth to which Jupiter's observed east-west jet streams extend has been a long-standing question. Resolving this puzzle has been a primary goal for the Juno spacecraft, which has been...
7.
Gladstone G, Versteeg M, Greathouse T, Hue V, Davis M, Gerard J, et al.
Geophys Res Lett
. 2017 Oct;
44(15):7668-7675.
PMID: 28989207
Juno ultraviolet spectrograph (UVS) observations of Jupiter's aurora obtained during approach are presented. Prior to the bow shock crossing on 24 June 2016, the Juno approach provided a rare opportunity...
8.
Mauk B, Haggerty D, Paranicas C, Clark G, Kollmann P, Rymer A, et al.
Nature
. 2017 Sep;
549(7670):66-69.
PMID: 28880294
The most intense auroral emissions from Earth's polar regions, called discrete for their sharply defined spatial configurations, are generated by a process involving coherent acceleration of electrons by slowly evolving,...
9.
Connerney J, Adriani A, Allegrini F, Bagenal F, Bolton S, Bonfond B, et al.
Science
. 2017 May;
356(6340):826-832.
PMID: 28546207
The Juno spacecraft acquired direct observations of the jovian magnetosphere and auroral emissions from a vantage point above the poles. Juno's capture orbit spanned the jovian magnetosphere from bow shock...
10.
Bolton S, Adriani A, Adumitroaie V, Allison M, Anderson J, Atreya S, et al.
Science
. 2017 May;
356(6340):821-825.
PMID: 28546206
On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing less than 5000 kilometers above the equatorial cloud tops. Images of Jupiter's poles show a chaotic scene,...