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A New Look at the Saturn System: The Voyager 2 Images

Overview of attention for article published in Science, January 1982
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11 Wikipedia pages

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Title
A New Look at the Saturn System: The Voyager 2 Images
Published in
Science, January 1982
DOI 10.1126/science.215.4532.504
Pubmed ID
Authors

Bradford A. Smith, Laurence Soderblom, Raymond Batson, Patricia Bridges, Jay Inge, Harold Masursky, Eugene Shoemaker, Reta Beebe, Joseph Boyce, Geoffrey Briggs, Anne Bunker, Stewart A. Collins, Candice J. Hansen, Torrence V. Johnson, Jim L. Mitchell, Richard J. Terrile, Allan F. Cook, Jeffrey Cuzzi, James B. Pollack, G. Edward Danielson, Andrew P. Ingersoll, Merton E. Davies, Garry E. Hunt, David Morrison, Tobias Owen, Carl Sagan, Joseph Veverka, Robert Strom, Verner E. Suomi

Abstract

Voyager 2 photography has complemented that of Voyager I in revealing many additional characteristics of Saturn and its satellites and rings. Saturn's atmosphere contains persistent oval cloud features reminiscent of features on Jupiter. Smaller irregular features track out a pattern of zonal winds that is symmetric about Saturn's equator and appears to extend to great depth. Winds are predominantly eastward and reach 500 meters per second at the equator. Titan has several haze layers with significantly varying optical properties and a northern polar "collar" that is dark at short wavelengths. Several satellites have been photographed at substantially improved resolution. Enceladus' surface ranges from old, densely cratered terrain to relatively young, uncratered plains crossed by grooves and faults. Tethys has a crater 400 kilometers in diameter whose floor has domed to match Tethys' surface curvature and a deep trench that extends at least 270 degrees around Tethys' circumference. Hyperion is cratered and irregular in shape. Iapetus' bright, trailing hemisphere includes several dark-floored craters, and Phoebe has a very low albedo and rotates in the direction opposite to that of its orbital revolution with a period of 9 hours. Within Saturn's rings, the "birth" of a spoke has been observed, and surprising azimuthal and time variability is found in the ringlet structure of the outer B ring. These observations lead to speculations about Saturn's internal structure and about the collisional and thermal history of the rings and satellites.

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 104 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
United Kingdom 2 2%
United States 2 2%
Italy 1 <1%
Puerto Rico 1 <1%
France 1 <1%
Unknown 97 93%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 24 23%
Researcher 20 19%
Student > Master 10 10%
Student > Bachelor 9 9%
Student > Doctoral Student 7 7%
Other 19 18%
Unknown 15 14%
Readers by discipline Count As %
Physics and Astronomy 38 37%
Earth and Planetary Sciences 25 24%
Engineering 5 5%
Chemistry 4 4%
Materials Science 3 3%
Other 12 12%
Unknown 17 16%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 3. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 19 July 2022.
All research outputs
#7,486,210
of 22,882,389 outputs
Outputs from Science
#48,114
of 78,002 outputs
Outputs of similar age
#5,326
of 30,300 outputs
Outputs of similar age from Science
#50
of 112 outputs
Altmetric has tracked 22,882,389 research outputs across all sources so far. This one is in the 44th percentile – i.e., 44% of other outputs scored the same or lower than it.
So far Altmetric has tracked 78,002 research outputs from this source. They typically receive a lot more attention than average, with a mean Attention Score of 62.3. This one is in the 21st percentile – i.e., 21% of its peers scored the same or lower than it.
Older research outputs will score higher simply because they've had more time to accumulate mentions. To account for age we can compare this Altmetric Attention Score to the 30,300 tracked outputs that were published within six weeks on either side of this one in any source. This one is in the 28th percentile – i.e., 28% of its contemporaries scored the same or lower than it.
We're also able to compare this research output to 112 others from the same source and published within six weeks on either side of this one. This one is in the 8th percentile – i.e., 8% of its contemporaries scored the same or lower than it.