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In Situ Observations of Interstellar Plasma with Voyager 1

Overview of attention for article published in Science, September 2013
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About this Attention Score

  • In the top 5% of all research outputs scored by Altmetric
  • High Attention Score compared to outputs of the same age (99th percentile)
  • High Attention Score compared to outputs of the same age and source (99th percentile)

Mentioned by

news
75 news outlets
blogs
13 blogs
twitter
54 tweeters
facebook
14 Facebook pages
wikipedia
1 Wikipedia page
googleplus
6 Google+ users
reddit
1 Redditor

Citations

dimensions_citation
149 Dimensions

Readers on

mendeley
57 Mendeley
citeulike
1 CiteULike
Title
In Situ Observations of Interstellar Plasma with Voyager 1
Published in
Science, September 2013
DOI 10.1126/science.1241681
Pubmed ID
Authors

D. A. Gurnett, W. S Kurth, L. F. Burlaga, N. F. Ness, Gurnett DA, Kurth WS, Burlaga LF, Ness NF

Abstract

Launched over 35 years ago, Voyagers 1 and 2 are on an epic journey outward from the Sun to reach the boundary between the solar plasma and the much cooler interstellar medium. The boundary, called the heliopause, is expected to be marked by a large increase in plasma density, from about 0.002 per cubic centimeter (cm(-3)) in the outer heliosphere, to about 0.1 cm(-3) in the interstellar medium. On 9 April 2013, the Voyager 1 plasma wave instrument began detecting locally generated electron plasma oscillations at a frequency of about 2.6 kilohertz. This oscillation frequency corresponds to an electron density of about 0.08 cm(-3), very close to the value expected in the interstellar medium. These and other observations provide strong evidence that Voyager 1 has crossed the heliopause into the nearby interstellar plasma.

Twitter Demographics

The data shown below were collected from the profiles of 54 tweeters who shared this research output. Click here to find out more about how the information was compiled.

Mendeley readers

The data shown below were compiled from readership statistics for 57 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
United States 3 5%
United Kingdom 2 4%
Estonia 1 2%
Switzerland 1 2%
Unknown 50 88%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 23 40%
Researcher 14 25%
Professor > Associate Professor 4 7%
Student > Bachelor 3 5%
Other 3 5%
Other 10 18%
Readers by discipline Count As %
Physics and Astronomy 36 63%
Earth and Planetary Sciences 5 9%
Medicine and Dentistry 3 5%
Engineering 3 5%
Unspecified 2 4%
Other 8 14%

Attention Score in Context

This research output has an Altmetric Attention Score of 796. 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 30 January 2018.
All research outputs
#4,660
of 11,671,562 outputs
Outputs from Science
#251
of 52,791 outputs
Outputs of similar age
#47
of 145,568 outputs
Outputs of similar age from Science
#8
of 802 outputs
Altmetric has tracked 11,671,562 research outputs across all sources so far. Compared to these this one has done particularly well and is in the 99th percentile: it's in the top 5% of all research outputs ever tracked by Altmetric.
So far Altmetric has tracked 52,791 research outputs from this source. They typically receive a lot more attention than average, with a mean Attention Score of 34.2. This one has done particularly well, scoring higher than 99% of its peers.
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 145,568 tracked outputs that were published within six weeks on either side of this one in any source. This one has done particularly well, scoring higher than 99% of its contemporaries.
We're also able to compare this research output to 802 others from the same source and published within six weeks on either side of this one. This one has done particularly well, scoring higher than 99% of its contemporaries.