The articles collected in this volume present all aspects of solar magnetism: from its origin in the solar dynamo to its evolution and dynamics that create the variability of solar phenomena, its well-known 11-year activity cycle that leads to the ever-changing pattern of sunspots and active regions on the Sun. Several contributions deal with the solar dynamo, the driver of many solar phenomena. Other contributions treat the transport and emergence of the magnetic flux through the outer layers of the Sun. The coupling of magnetic fields from the surface to the solar corona and beyond is also described, together with current studies on the predictability of solar activity. This book is aimed at researchers and graduate students working in so...
In this article I review the fundamentals of solar-dynamo theory. I describe both historical and con...
The solar dynamo is the action of flows inside the Sun to maintain its magnetic field against Ohmic ...
Abstract: The almost stately evolution of the global heliospheric magnetic field pattern during most...
The articles collected in this volume present all aspects of solar magnetism: from its origin in the...
The year 2008 marked the one hundredth anniversary of the observational discovery by George Ellery H...
This review provides an introduction to the generation and evolution of the Sun’s magnetic field, su...
The article gives a concise overview of solar dynamical processes and their impacts on the space wea...
The Sun is a magnetically active star and is the source of the solar wind, electromagnetic radiation...
Abstract: The present state of art in solar physics indicates that some key ingredients in explainin...
A collection of papers edited by four experts in the field, this book sets out to describe the way s...
The origins of solar magnetism lie below the visible surface of the Sun, in the highly turbulent con...
Solar magnetism is responsible for the several active phenomena that occur in the solar atmosphere. ...
The Sun manifests its magnetic field in form of the solar activities, being observed on the surface ...
NASA's Solar Dynamics Observatory (SDO) mission has provided a large amount of new data on solar dyn...
The purpose of space weather is the systemic study of the Sun–Earth system, in order to determine th...
In this article I review the fundamentals of solar-dynamo theory. I describe both historical and con...
The solar dynamo is the action of flows inside the Sun to maintain its magnetic field against Ohmic ...
Abstract: The almost stately evolution of the global heliospheric magnetic field pattern during most...
The articles collected in this volume present all aspects of solar magnetism: from its origin in the...
The year 2008 marked the one hundredth anniversary of the observational discovery by George Ellery H...
This review provides an introduction to the generation and evolution of the Sun’s magnetic field, su...
The article gives a concise overview of solar dynamical processes and their impacts on the space wea...
The Sun is a magnetically active star and is the source of the solar wind, electromagnetic radiation...
Abstract: The present state of art in solar physics indicates that some key ingredients in explainin...
A collection of papers edited by four experts in the field, this book sets out to describe the way s...
The origins of solar magnetism lie below the visible surface of the Sun, in the highly turbulent con...
Solar magnetism is responsible for the several active phenomena that occur in the solar atmosphere. ...
The Sun manifests its magnetic field in form of the solar activities, being observed on the surface ...
NASA's Solar Dynamics Observatory (SDO) mission has provided a large amount of new data on solar dyn...
The purpose of space weather is the systemic study of the Sun–Earth system, in order to determine th...
In this article I review the fundamentals of solar-dynamo theory. I describe both historical and con...
The solar dynamo is the action of flows inside the Sun to maintain its magnetic field against Ohmic ...
Abstract: The almost stately evolution of the global heliospheric magnetic field pattern during most...