This white paper, submitted to the Heliophysics 2050 Workshop, discusses the diagnostic power and need for soft X-ray spectroscopy of the Sun to understand heating of plasma in the solar corona. Significant progress into the critical coronal heating question – and other closely related questions – is easily achievable by 2050 if we leverage these advances and prioritize development of new solar SXR observatorie
Aims: The detection of very hot plasma in the quiescent corona is important for diagnosing heating m...
Aims: The detection of very hot plasma in the quiescent corona is important for diagnosing heating m...
The soft X-ray telescope (SXRT) will provide direct images of the solar corona with spatial resoluti...
We discuss the diagnostics available to study the 5–10 MK plasma in the solar corona, which is key t...
We discuss the diagnostics available to study the 5–10 MK plasma in the solar corona, which is key t...
The solar corona is an extremely hot, dynamic region of the solar atmosphere. Hard X-ray (HXR) obser...
We study the physics of the solar corona as a whole, i.e. of the Sun as a Star, in order to understa...
We study the physics of the solar corona as a whole, i.e. of the Sun as a Star, in order to understa...
In this paper we perform an analysis of the energetics of the solar flaring chromosphere irradiated ...
We present new RHESSI upper limits in the 3-200 keV energy range for solar hard X-ray emission in th...
We present new RHESSI upper limits in the 3-200 keV energy range for solar hard X-ray emission in th...
In this paper we perform an analysis of the energetics of the solar flaring chromosphere irradiated ...
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
While our Sun may appear boring at first glance, the solar corona, the outermost layer of the Sun's ...
Soft X-ray spectroscopy of the Sun is an important tool to understand the coronal dynamics and compo...
Aims: The detection of very hot plasma in the quiescent corona is important for diagnosing heating m...
Aims: The detection of very hot plasma in the quiescent corona is important for diagnosing heating m...
The soft X-ray telescope (SXRT) will provide direct images of the solar corona with spatial resoluti...
We discuss the diagnostics available to study the 5–10 MK plasma in the solar corona, which is key t...
We discuss the diagnostics available to study the 5–10 MK plasma in the solar corona, which is key t...
The solar corona is an extremely hot, dynamic region of the solar atmosphere. Hard X-ray (HXR) obser...
We study the physics of the solar corona as a whole, i.e. of the Sun as a Star, in order to understa...
We study the physics of the solar corona as a whole, i.e. of the Sun as a Star, in order to understa...
In this paper we perform an analysis of the energetics of the solar flaring chromosphere irradiated ...
We present new RHESSI upper limits in the 3-200 keV energy range for solar hard X-ray emission in th...
We present new RHESSI upper limits in the 3-200 keV energy range for solar hard X-ray emission in th...
In this paper we perform an analysis of the energetics of the solar flaring chromosphere irradiated ...
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
While our Sun may appear boring at first glance, the solar corona, the outermost layer of the Sun's ...
Soft X-ray spectroscopy of the Sun is an important tool to understand the coronal dynamics and compo...
Aims: The detection of very hot plasma in the quiescent corona is important for diagnosing heating m...
Aims: The detection of very hot plasma in the quiescent corona is important for diagnosing heating m...
The soft X-ray telescope (SXRT) will provide direct images of the solar corona with spatial resoluti...