Views provided by UsageCounts
<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>This data set corresponds to the simulation data presented in the article "Charting nearby stellar systems: The intensity of Galactic cosmic rays for a sample of solar-type stars" (Rodgers-Lee, Vidotto & Mesquita, MNRAS, 2021). Details of the stellar wind and cosmic ray model used for the simulations are available in the article. The data consists of the differential intensity of Galactic cosmic rays as a function of cosmic ray kinetic energy at different orbital distances from the star. The data is given for a number of different stellar systems. The first line gives the column headings. File names are formatted as "gcr_data_XXX.dat" where "XXX" corresponds to the name of the star considered. The simulation details can be found in Tables 1 and 2 of the article.
| citations 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 | 3 |

Views provided by UsageCounts