Due to the increase in the spatial and temporal resolution of observations of the solar
atmosphere, which is mainly associated with progress in space research, we now …

NuSTAR is a highly sensitive focusing hard X-ray (HXR) telescope and has observed
several small microflares in its initial solar pointings. In this paper, we present the first joint …

Three generations of the Miniature X-ray Solar Spectrometer (MinXSS) have flown on small
satellites with the goal" to explore the energy distribution of soft X-ray (SXR) emissions from …

The properties that are expected of" hot" non-flaring plasmas due to nanoflare heating in
active regions are investigated using hydrodynamic modeling tools, including a two-fluid …

The solar corona is orders of magnitude hotter than the underlying photosphere, but how the
corona attains such high temperatures is still not understood. Soft X-ray (SXR) emission …

The goal of the Miniature X-ray Solar Spectrometer (MinXSS) CubeSat is to explore the
energy distribution of soft X-ray (SXR) emissions from the quiescent Sun, active regions, and …

A new methodology is given to determine basic parameters of flares from their X-ray light
curves. Algorithms are developed from the analysis of small X-ray flares occurring during the …

Solar-terrestrial environment is manifested primarily by the physical conditions of the solar
interior, solar atmosphere and eruptive solar plasma. Each parameter gives unique …

The SphinX X-ray spectrophotometer on the CORONAS–PHOTON spacecraft measured soft
X-ray emission in the 1–15 keV energy range during the deep solar minimum of 2009 with a …

Nanoflare-heating theory predicts steady hot-plasma emission in non-flaring active regions.
It is hard to find this emission with conventional non-monochromatic imagers (such as the …