THE StellaR PAth WP1: Sun-as-a-star plasma Emission Measure Distributions

{"references": ["Coffaro, M., Stelzer, B., Orlando, S. 2022, A&A, 661, A79", "Coffaro, M., Stelzer, B., Orlando, S. 2021, AN 343, Issue 4, article id. e10066", "Coffaro, M., Stelzer, B., Orlando, S., et al. 2020, A&A, 636, A49", "Orlando, S., Favata, F., Micela, G., et al. 2017, A&A, 605, A19", "Orlando, S., Peres, G., & Reale, F. 2004, A&A 424, 677", "Orlando, S., Peres, G., & Reale, F. 2001, ApJ, 560, 499", "Reale, F., Peres, G., & Orlando, S. 2001, ApJ, 557, 906"]}

This folder contains a set of plasma Emission Measure Distributions (EMDs) vs. temperature, derived from observations of the solar corona with the Soft X-ray Telescope (SXT) on board the solar satellite Yohkoh, and the prescription to build EMDs for coronae of solar-type stars with different activity levels, including both quiescent and flaring components. For details read the Description PDF file.

Keywords

high-energy radiation, solar corona, solar-like stars, spectral modeling

Impact byBIP!

	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