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Interstellar Processes

Overview of attention for book
Cover of 'Interstellar Processes'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 1 The Milky Way as a Galaxy
  3. Altmetric Badge
    Chapter 2 H2 in the Galaxy
  4. Altmetric Badge
    Chapter 3 Molecular Clouds: An Overview
  5. Altmetric Badge
    Chapter 4 Observations of Molecular Cloud Structure and Internal Motions
  6. Altmetric Badge
    Chapter 5 The Atomic Component
  7. Altmetric Badge
    Chapter 6 Hot Interstellar Gas in the Galactic Disk and Halo
  8. Altmetric Badge
    Chapter 7 The High-Energy Component of the ISM—Cosmic-Ray Phenomena
  9. Altmetric Badge
    Chapter 8 Interstellar Magnetic Fields
  10. Altmetric Badge
    Chapter 9 The Theory of the Galactic Magnetic Field
  11. Altmetric Badge
    Chapter 10 Panel Discussion: Phases of the Interstellar Medium
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    Chapter 11 Mass and Energy Balance in the Interstellar Medium: How to Model the Disk Gas in our Galaxy
  13. Altmetric Badge
    Chapter 12 Cloud Formation and Destruction
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    Chapter 13 The Physics of Interstellar Shock Waves
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    Chapter 14 Theory of Collapse and Protostar Formation
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    Chapter 15 Theoretical Approaches to Interstellar Turbulence
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    Chapter 16 Composition, Structure, and Chemistry of Interstellar Dust
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    Chapter 17 Infrared Absorption and Emission Characteristics of Interstellar PAHs
  19. Altmetric Badge
    Chapter 18 Grain Destruction, Formation, and Evolution
  20. Altmetric Badge
    Chapter 19 Interstellar Grains in the Solar System
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    Chapter 20 Element Abundances in the Interstellar Atomic Material
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    Chapter 21 Chemical Abundances in Molecular Clouds
  23. Altmetric Badge
    Chapter 22 Gas Phase Chemical Processes in Molecular Clouds
  24. Altmetric Badge
    Chapter 23 Chemical Evolution of Molecular Clouds
  25. Altmetric Badge
    Chapter 24 Chemical Evolution of Galaxies
  26. Altmetric Badge
    Chapter 25 The Solar System/Interstellar Medium Connection: Gas Phase Abundances
  27. Altmetric Badge
    Chapter 26 Observations of the Cooling of the Interstellar Gas
  28. Altmetric Badge
    Chapter 27 Heating and Cooling of the Interstellar Gas
  29. Altmetric Badge
    Chapter 28 Atomic and Molecular Physics of Interstellar Heating and Cooling
  30. Altmetric Badge
    Chapter 29 Masers in the Interstellar Medium
Attention for Chapter 8: Interstellar Magnetic Fields
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About this Attention Score

  • In the top 25% of all research outputs scored by Altmetric
  • High Attention Score compared to outputs of the same age (89th percentile)
  • High Attention Score compared to outputs of the same age and source (92nd percentile)

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Chapter title
Interstellar Magnetic Fields
Chapter number 8
Book title
Interstellar Processes
Published in
ADS, September 1987
DOI 10.1007/978-94-009-3861-8_8
Book ISBNs
978-9-02-772485-4, 978-9-40-093861-8
Authors

Carl Heiles

Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 9. 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 13 June 2014.
All research outputs
#3,279,161
of 22,828,180 outputs
Outputs from ADS
#2,260
of 37,360 outputs
Outputs of similar age
#678
of 12,117 outputs
Outputs of similar age from ADS
#2
of 55 outputs
Altmetric has tracked 22,828,180 research outputs across all sources so far. Compared to these this one has done well and is in the 84th percentile: it's in the top 25% of all research outputs ever tracked by Altmetric.
So far Altmetric has tracked 37,360 research outputs from this source. They receive a mean Attention Score of 4.6. This one has done particularly well, scoring higher than 92% 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 12,117 tracked outputs that were published within six weeks on either side of this one in any source. This one has done well, scoring higher than 89% of its contemporaries.
We're also able to compare this research output to 55 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 92% of its contemporaries.