One of the basic questions of solar research is the nature of the Sun. We show here how the plasma nature of the Sun leads to the self-generation of solar activity. The release of magnetic, rotational, gravitational, nuclear energies and that of the gravity mode oscillations deviate from uniformity and spherical symmetry. Through instabilities they lead to the emergence of sporadic and localized regions like flux tubes, electric filaments, magnetic elements and high temperature regions. A systematic approach exploring the solar collective degrees of freedom, extending to ordering phenomena of the magnetic features related to Higgs fields, is presented. Handling solar activity as transformations of energies from one form to another one prese...
Spontaneous formation of self-organized magnetic structures, such as sunspots and pores, is one of i...
The Sun’s magnetic activity has steadily declined during its main-sequence life. While the solar pho...
The articles collected in this volume present all aspects of solar magnetism: from its origin in the...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
Abstract: The present state of art in solar physics indicates that some key ingredients in explainin...
It is well established that magnetic fields exist in astronomical objects of all scales, in planets,...
The baryonic Universe is mainly composed by plasma and so, magnetism plays a fundamental role. Howev...
This lecture summarises how our understanding of many aspects of the Sun has been revolutionised ove...
Plasma, often referred to as the fourth state of matter, makes up most of the material in the known ...
The solar dynamo is the action of flows inside the Sun to maintain its magnetic field against Ohmic ...
The present article is the successor of Solar Dynamical Processes I. The previous article was focuse...
A fundamental property of the Sun's corona i s that it is violently dynamic. The most spectacular an...
The stellar equations of state treat the Sun much like an ideal gas, wherein the photo...
Over the past two decades, there have been a series of major solar space missions, namely Yohkoh, SO...
Spontaneous formation of self-organized magnetic structures, such as sunspots and pores, is one of i...
The Sun’s magnetic activity has steadily declined during its main-sequence life. While the solar pho...
The articles collected in this volume present all aspects of solar magnetism: from its origin in the...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
One of the basic questions of solar research is the nature of the Sun. We show here how the plasma n...
Abstract: The present state of art in solar physics indicates that some key ingredients in explainin...
It is well established that magnetic fields exist in astronomical objects of all scales, in planets,...
The baryonic Universe is mainly composed by plasma and so, magnetism plays a fundamental role. Howev...
This lecture summarises how our understanding of many aspects of the Sun has been revolutionised ove...
Plasma, often referred to as the fourth state of matter, makes up most of the material in the known ...
The solar dynamo is the action of flows inside the Sun to maintain its magnetic field against Ohmic ...
The present article is the successor of Solar Dynamical Processes I. The previous article was focuse...
A fundamental property of the Sun's corona i s that it is violently dynamic. The most spectacular an...
The stellar equations of state treat the Sun much like an ideal gas, wherein the photo...
Over the past two decades, there have been a series of major solar space missions, namely Yohkoh, SO...
Spontaneous formation of self-organized magnetic structures, such as sunspots and pores, is one of i...
The Sun’s magnetic activity has steadily declined during its main-sequence life. While the solar pho...
The articles collected in this volume present all aspects of solar magnetism: from its origin in the...