After summarizing the relevant observational data, we discuss how a study of flux tube dynamics in the solar convection zone helps us to understand the formation of sunspots. Then we introduce the flux transport dynamo model and assess its success in modelling both the solar cycle and its departures from strictly periodic behaviour
Abstract: The present state of art in solar physics indicates that some key ingredients in explainin...
The solar dynamo is the action of flows inside the Sun to maintain its magnetic field against Ohmic ...
This is the author accepted manuscript. The final version is available from Cambridge University Pre...
After summarizing the relevant observational data, we discuss how a study of flux tube dynamics in t...
Abstract. Sunspots, seen as cool regions on the surface of the Sun, are a thermal phenomenon. Sunspo...
Sunspot observations inspired solar dynamo theory and continue to do so. Simply counting them establ...
In 1844 Schwabe discovered that the number of sunspots increased and decreased over a period of abou...
We discuss the current status of solar dynamo theory and describe the dynamo model developed by our ...
The Sun, by the virtue of its proximity to Earth, serves as an excellent astrophysical laboratory fo...
A collection of papers edited by four experts in the field, this book sets out to describe the way s...
2014 Summer.The Sun exhibits cyclic properties of its large-scale magnetic field on the order of ~22...
The Sun’s magnetic field drives the solar wind and produces space weather. It also acts as the proto...
Spontaneous formation of self-organized magnetic structures, such as sunspots and pores, is one of i...
Sunspots have been observed for over four centuries and the magnetic nature of sunspot cycles has be...
The articles collected in this volume present all aspects of solar magnetism: from its origin in the...
Abstract: The present state of art in solar physics indicates that some key ingredients in explainin...
The solar dynamo is the action of flows inside the Sun to maintain its magnetic field against Ohmic ...
This is the author accepted manuscript. The final version is available from Cambridge University Pre...
After summarizing the relevant observational data, we discuss how a study of flux tube dynamics in t...
Abstract. Sunspots, seen as cool regions on the surface of the Sun, are a thermal phenomenon. Sunspo...
Sunspot observations inspired solar dynamo theory and continue to do so. Simply counting them establ...
In 1844 Schwabe discovered that the number of sunspots increased and decreased over a period of abou...
We discuss the current status of solar dynamo theory and describe the dynamo model developed by our ...
The Sun, by the virtue of its proximity to Earth, serves as an excellent astrophysical laboratory fo...
A collection of papers edited by four experts in the field, this book sets out to describe the way s...
2014 Summer.The Sun exhibits cyclic properties of its large-scale magnetic field on the order of ~22...
The Sun’s magnetic field drives the solar wind and produces space weather. It also acts as the proto...
Spontaneous formation of self-organized magnetic structures, such as sunspots and pores, is one of i...
Sunspots have been observed for over four centuries and the magnetic nature of sunspot cycles has be...
The articles collected in this volume present all aspects of solar magnetism: from its origin in the...
Abstract: The present state of art in solar physics indicates that some key ingredients in explainin...
The solar dynamo is the action of flows inside the Sun to maintain its magnetic field against Ohmic ...
This is the author accepted manuscript. The final version is available from Cambridge University Pre...
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