Views provided by UsageCounts
The HelioML team is happy to announce the release of HelioML 0.3.0. We would like to acknowledge the following people for contributing new chapters to the textbook since v0.2.0: Ryan M. McGranaghan, along with collaborators Anthony J. Mannucci, Brian Wilson, Chris A. Mattmann, and Richard Chadwick, for contributing Chapter 4 on predicting high-latitude ionospheric scintillation, Brandon Panos for contributing Chapter 5 on analyzing the behavior of the Mg II spectral line during solar flares, and Tobías Felipe, along with collaborator and Andrés Asensio Ramos, for contributing Chapter 6 on detecting far-side solar active regions. Sincerely, The HelioML Team
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
| views | 6 |

Views provided by UsageCounts