Search Publications

Coronal bright points
DOI: 10.1007/s41116-019-0018-8 Bibcode: 2019LRSP...16....2M

Madjarska, Maria S.

Coronal bright points (CBPs) are a fundamental class of solar activity. They represent a set of low-corona small-scale loops with enhanced emission in the extreme-ultraviolet and X-ray spectrum that connect magnetic flux concentrations of opposite polarities. CBPs are one of the main building blocks of the solar atmosphere outside active regions u…

2019 Living Reviews in Solar Physics
Hinode IRIS SOHO 65
Solar UV and X-ray spectral diagnostics
DOI: 10.1007/s41116-018-0015-3 Bibcode: 2018LRSP...15....5D

Del Zanna, Giulio; Mason, Helen E.

X-ray and ultraviolet (UV) observations of the outer solar atmosphere have been used for many decades to measure the fundamental parameters of the solar plasma. This review focuses on the optically thin emission from the solar atmosphere, mostly found at UV and X-ray (XUV) wavelengths, and discusses some of the diagnostic methods that have been us…

2018 Living Reviews in Solar Physics
IRIS SOHO 175