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The Sun: New Challenges

Overview of attention for book
Cover of 'The Sun: New Challenges'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 1 The Unusual Sunspot Minimum: Challenge to the Solar Dynamo Theory
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    Chapter 2 The Evolution of Cyclic Activity of the Sun in the Context of Physical Processes on Late-Type Stars
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    Chapter 3 Long-Term Variations of the Solar Supergranulation Size According to the Observations in CaIIK Line
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    Chapter 4 On the Problem of Heat Transport in the Solar Atmosphere
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    Chapter 5 Dynamics of the Electrical Currents in Coronal Magnetic Loops
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    Chapter 6 Observations of Solar Flares from GHz to THz Frequencies
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    Chapter 7 On the Interaction of Solar Rotational Discontinuities with a Contact Discontinuity Inside the Solar Transition Region as a Source of Plasma Heating in the Solar Corona
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    Chapter 8 Complex Magnetic Evolution and Magnetic Helicity in the Solar Atmosphere
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    Chapter 9 On Our Ability to Predict Major Solar Flares
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    Chapter 10 Chromospheric Evaporation in Solar Flares
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    Chapter 11 Evolutionary of Discontinuous Plasma Flows in the Vicinity of Reconnecting Current Layers
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    Chapter 12 Analytical Models of Generalized Syrovatskii’s Current Layer with MHD ShockWaves
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    Chapter 13 Solar Convection and Self-Similar Atmosphere’s Structures
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    Chapter 14 SDO in Pulkovo Observatory
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    Chapter 15 Variations of Microwave Emission and MDI Topology in the Active Region NOAA 10030 Before and During the Power Flare Series
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    Chapter 16 Scenario of Evolution of the Epoch of Minimum at the Final Stage of Cycle 23
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    Chapter 17 Solar Magnetic Fields as a Clue for the Mystery of the Permanent Solar Wind and the Solar Corona
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    Chapter 18 Two Types of Coronal Bright Points in the 24-th Cycle of Solar Activity
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    Chapter 19 The Self-Similar Shrinkage of Force-Free Magnetic Flux Ropes in a Passive Medium of Finite Conductivity
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    Chapter 20 Solar Activity Indices in the Cycles 21–23
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    Chapter 21 Coronal Mass Ejections on the Sun and Their Relationship with Flares and Magnetic Helicity
Attention for Chapter 8: Complex Magnetic Evolution and Magnetic Helicity in the Solar Atmosphere
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About this Attention Score

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Chapter title
Complex Magnetic Evolution and Magnetic Helicity in the Solar Atmosphere
Chapter number 8
Book title
The Sun: New Challenges
Published in
arXiv, February 2013
DOI 10.1007/978-3-642-29417-4_8
Book ISBNs
978-3-64-229416-7, 978-3-64-229417-4
Authors

Alexei A. Pevtsov, Pevtsov, Alexei A.

X Demographics

X Demographics

The data shown below were collected from the profile of 1 X user who shared this research output. Click here to find out more about how the information was compiled.
Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 4 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
China 1 25%
Unknown 3 75%

Demographic breakdown

Readers by professional status Count As %
Researcher 2 50%
Student > Ph. D. Student 1 25%
Professor 1 25%
Readers by discipline Count As %
Physics and Astronomy 4 100%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 1. 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 07 February 2013.
All research outputs
#18,327,422
of 22,694,633 outputs
Outputs from arXiv
#531,495
of 930,365 outputs
Outputs of similar age
#219,309
of 282,807 outputs
Outputs of similar age from arXiv
#2,273
of 5,572 outputs
Altmetric has tracked 22,694,633 research outputs across all sources so far. This one is in the 11th percentile – i.e., 11% of other outputs scored the same or lower than it.
So far Altmetric has tracked 930,365 research outputs from this source. They receive a mean Attention Score of 3.9. This one is in the 28th percentile – i.e., 28% 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 282,807 tracked outputs that were published within six weeks on either side of this one in any source. This one is in the 11th percentile – i.e., 11% of its contemporaries scored the same or lower than it.
We're also able to compare this research output to 5,572 others from the same source and published within six weeks on either side of this one. This one is in the 37th percentile – i.e., 37% of its contemporaries scored the same or lower than it.