Add to ORKGWe simulate the transport of magnetic flux in the Sun s photosphere by an evolving pattern of cellular horizontal flows (supergranules). Characteristics of the simulated flow pattern match observed characteristics including the velocity power spectrum, cell lifetimes, and cell pattern motion in longitude and latitude. Simulations using an average, and north-south symmetric, meridional motion of the cellular pattern produce polar magnetic fields that are too weak in the North and too strong in the South. Simulations using cellular patterns with meridional motions that evolve with the observed changes in strength and north-south asymmetry will be analyzed to see if they reproduce the polar field evolution observed during the rise of Cycle 24
Observations of filaments and filament channels on the Sun indicate that the magnetic fields in thes...
In this paper the origin and evolution of the Sun’s open magnetic flux is considered by conducting m...
We measured the flows of magnetic elements on the Sun at very high latitudes by analyzing magnetic i...
Abstract This thesis studies the long-term evolution of the photospheric magnetic field using surfa...
The cause of the low and extended minimum in solar activity between Sunspot Cycles 23 and 24 was the...
The faster meridional flow that preceded the solar cycle 23/24 minimum is thought to have led to wea...
Abstract Context: The evolution of the photospheric magnetic field can be simulated with surface fl...
Aims. Sunspot activity is often hemispherically asymmetric, and during the Maunder minimum, activity...
Models of the photospheric flows due to supergranulation are generated using an evolving spectrum of...
We simulate the evolution of the Sun’s large-scale magnetic field during solar cycle 21, including t...
The Sun’s polar magnetic fields are directly related to solar cycle variability. The strength of the...
In this paper the origin and evolution of the Sun's open magnetic flux is considered by conducting m...
Coupled flux transport and magneto-frictional simulations are extended to simulate the continuous ma...
<p>We present an investigation of the large-scale flows that influence magnetic fields at the solar ...
The distribution of magnetic fields of positive and negative polarities over the surface of the Sun ...
Observations of filaments and filament channels on the Sun indicate that the magnetic fields in thes...
In this paper the origin and evolution of the Sun’s open magnetic flux is considered by conducting m...
We measured the flows of magnetic elements on the Sun at very high latitudes by analyzing magnetic i...
Abstract This thesis studies the long-term evolution of the photospheric magnetic field using surfa...
The cause of the low and extended minimum in solar activity between Sunspot Cycles 23 and 24 was the...
The faster meridional flow that preceded the solar cycle 23/24 minimum is thought to have led to wea...
Abstract Context: The evolution of the photospheric magnetic field can be simulated with surface fl...
Aims. Sunspot activity is often hemispherically asymmetric, and during the Maunder minimum, activity...
Models of the photospheric flows due to supergranulation are generated using an evolving spectrum of...
We simulate the evolution of the Sun’s large-scale magnetic field during solar cycle 21, including t...
The Sun’s polar magnetic fields are directly related to solar cycle variability. The strength of the...
In this paper the origin and evolution of the Sun's open magnetic flux is considered by conducting m...
Coupled flux transport and magneto-frictional simulations are extended to simulate the continuous ma...
<p>We present an investigation of the large-scale flows that influence magnetic fields at the solar ...
The distribution of magnetic fields of positive and negative polarities over the surface of the Sun ...
Observations of filaments and filament channels on the Sun indicate that the magnetic fields in thes...
In this paper the origin and evolution of the Sun’s open magnetic flux is considered by conducting m...
We measured the flows of magnetic elements on the Sun at very high latitudes by analyzing magnetic i...