The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool
photosphere and the intensely heated transition region and corona. Compressible and …

Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …

Abstract Algorithms based on Empirical Mode Decomposition (EMD) and Iterative Filtering
(IF) are largely implemented for representing a signal as superposition of simpler well …

Prominences are intriguing, but poorly understood, magnetic structures of the solar corona.
The dynamics of solar prominences has been the subject of a large number of studies, and …

Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …

Transverse magnetohydrodynamic (MHD) waves are ubiquitous in the solar atmosphere
and may be responsible for generating the Sun's million-degree outer atmosphere …

Transverse magnetohydrodynamic waves have been shown to be ubiquitous in the solar
atmosphere and can, in principle, carry sufficient energy to generate and maintain the Sun's …

Current analytical and numerical modeling suggest the existence of ubiquitous thin current
sheets in the corona that could explain the observed heating requirements. On the other …

The development of methods able to extract hidden features from non-stationary and non-
linear signals in a fast and reliable way is of high importance in many research fields. In this …

Hinode is Japan's third solar mission following Hinotori (1981–1982) and Yohkoh (1991–
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …