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
International audienceThe M dwarf Proxima Centauri, the Sun’s closest stellar neighbour, is known to...
Based on Yohkoh Soft X-Ray Telescope (SXT) observations of the Sun near peak activity level obtained...
Epsilon Eri is a young solar-like star with a ~3 yr X-ray activity cycle, detected by us for the fir...
Studying the solar corona, due to its vicinity, is the starting point to understand stellar activity...
The scope of this work is to obtain the emission measure distributions vs. temperature, EM(T ), of t...
Emission line fluxes from cool stars are widely used to establish an apparent emission measure distr...
We study the physics of the solar corona as a whole, i.e. of the Sun as a Star, in order to understa...
The solar corona is a template to study and understand stellar activity. However the solar corona di...
Context: The solar corona is a template to understand stellar activity. The Sun is a moderately acti...
Context. Due to their wide wavelength coverage across the millimeter to centimeter (mm–cm) range and...
To solve a number of problems in solar physics related to mechanisms of energy release in solar coro...
Context. Due to their wide wavelength coverage across the millimeter to centimeter (mm–cm) range and...
A survey of 28 stars (22 active binary systems, plus 6 single stars or wide binaries for comparison)...
The Sun is the only star that we can spatially resolve and it can be regarded as a fundamental plasm...
The temperature distribution of the emitting plasma is a crucial constraint when studying the heatin...
International audienceThe M dwarf Proxima Centauri, the Sun’s closest stellar neighbour, is known to...
Based on Yohkoh Soft X-Ray Telescope (SXT) observations of the Sun near peak activity level obtained...
Epsilon Eri is a young solar-like star with a ~3 yr X-ray activity cycle, detected by us for the fir...
Studying the solar corona, due to its vicinity, is the starting point to understand stellar activity...
The scope of this work is to obtain the emission measure distributions vs. temperature, EM(T ), of t...
Emission line fluxes from cool stars are widely used to establish an apparent emission measure distr...
We study the physics of the solar corona as a whole, i.e. of the Sun as a Star, in order to understa...
The solar corona is a template to study and understand stellar activity. However the solar corona di...
Context: The solar corona is a template to understand stellar activity. The Sun is a moderately acti...
Context. Due to their wide wavelength coverage across the millimeter to centimeter (mm–cm) range and...
To solve a number of problems in solar physics related to mechanisms of energy release in solar coro...
Context. Due to their wide wavelength coverage across the millimeter to centimeter (mm–cm) range and...
A survey of 28 stars (22 active binary systems, plus 6 single stars or wide binaries for comparison)...
The Sun is the only star that we can spatially resolve and it can be regarded as a fundamental plasm...
The temperature distribution of the emitting plasma is a crucial constraint when studying the heatin...
International audienceThe M dwarf Proxima Centauri, the Sun’s closest stellar neighbour, is known to...
Based on Yohkoh Soft X-Ray Telescope (SXT) observations of the Sun near peak activity level obtained...
Epsilon Eri is a young solar-like star with a ~3 yr X-ray activity cycle, detected by us for the fir...