The visual complexity of coronal mass ejections follows the solar cycle-Reference-Cited by-同舟云学术

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The visual complexity of coronal mass ejections follows the solar cycle

Published:2020-06-10 Issue: Volume: Page:
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Author:

Jones Shannon¹^ORCID,Scott Christopher¹^ORCID,Barnard Luke¹^ORCID,Highfield Roger²^ORCID,Lintott Chris J³^ORCID,Baeten E M L⁴^ORCID

Affiliation:

1. University of Reading

2. Science Museum

3. University of Oxford

4. Unknown

Publisher

Wiley

Reference61 articles.

1. The Solar Stormwatch CME catalogue: Results from the first space weather citizen science project;Barnard L. A.;Space Weather,2015

2. Barnard L. A. C. J. Scott M. Owens M. Lockwood S. R. Crothers J. A. Davies and R. A. Harrison (2015b): Differences between the CME fronts tracked by an expert an automated algorithm and the Solar Stormwatch project. Space weather 13 709-725 doi: 10.1002/2015SW001280.

3. Barnard L. A. C. A. deKoning C. J. Scott M. J. Owens J. Wilkinson and J. A. Davies (2017): Testing the current paradigm for space weather prediction with heliospheric imagers. Space Weather 15 6 doi: 10.1002/2017SW001609.

4. Barnard L. A. M. J. Owens C. J. Scott and S. R. Jones (2019): Extracting inner-heliosphere solar wind speed information from heliospheric imager observations. Space Weather 17 6 doi: 10.1029/2019SW002226.

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