We investigate how representing active regions with bipolar magnetic regions (BMRs) affects the end-of-cycle polar field predicted by the surface flux transport model. Our study is based on a new database of BMRs derived from the SDO/HMI active region patch data between 2010 and 2020. An automated code is developed for fitting each active region patch with a BMR, matching both the magnetic flux and axial dipole moment of the region and removing repeat observations of the same region. By comparing the predicted evolution of each of the 1090 BMRs with the predicted evolution of their original active region patches, we show that the bipolar approximation leads to a 24% overestimate of the net axial dipole moment, given the same flow parameters...
The emergence of tilted bipolar active regions (ARs) and the dispersal of their flux, mediated via p...
Context. The area asymmetry between the preceding and following regions of opposite magnetic polari...
Magnetic flux emerging on the Sun's surface in the form of bipolar magnetic regions is redistributed...
As an observational case study, we consider the origin of a prominent poleward surge of leading pola...
Context. The solar dipole moment at cycle minimum is considered to be the most reliable precursor wi...
Aims. We aim to determine the effect of converging flows on the evolution of a bipolar magnetic regi...
Context. The relationship between bipolar magnetic regions (BMRs) and their sunspots is an important...
The emergence of tilted bipolar active regions (ARs) and the dispersal of their flux, mediated via p...
Context. The magnetic polarities of bipolar active regions (ARs) exhibit elongations in line-of-sigh...
Citation and Acknowledgements Please cite both this database, the papers describing it, as well a...
Aims. We aim to investigate how converging flows towards active regions affect the surface transport...
Context. The choice of free parameters in surface flux transport (SFT) models describing the evoluti...
Abstract This thesis studies the long-term evolution of the photospheric magnetic field using surfa...
One of the major sources of perturbation in the solar cycle amplitude is believed to be the emergenc...
International audienceContext. Active regions (ARs) appear in the solar atmosphere as a consequence ...
The emergence of tilted bipolar active regions (ARs) and the dispersal of their flux, mediated via p...
Context. The area asymmetry between the preceding and following regions of opposite magnetic polari...
Magnetic flux emerging on the Sun's surface in the form of bipolar magnetic regions is redistributed...
As an observational case study, we consider the origin of a prominent poleward surge of leading pola...
Context. The solar dipole moment at cycle minimum is considered to be the most reliable precursor wi...
Aims. We aim to determine the effect of converging flows on the evolution of a bipolar magnetic regi...
Context. The relationship between bipolar magnetic regions (BMRs) and their sunspots is an important...
The emergence of tilted bipolar active regions (ARs) and the dispersal of their flux, mediated via p...
Context. The magnetic polarities of bipolar active regions (ARs) exhibit elongations in line-of-sigh...
Citation and Acknowledgements Please cite both this database, the papers describing it, as well a...
Aims. We aim to investigate how converging flows towards active regions affect the surface transport...
Context. The choice of free parameters in surface flux transport (SFT) models describing the evoluti...
Abstract This thesis studies the long-term evolution of the photospheric magnetic field using surfa...
One of the major sources of perturbation in the solar cycle amplitude is believed to be the emergenc...
International audienceContext. Active regions (ARs) appear in the solar atmosphere as a consequence ...
The emergence of tilted bipolar active regions (ARs) and the dispersal of their flux, mediated via p...
Context. The area asymmetry between the preceding and following regions of opposite magnetic polari...
Magnetic flux emerging on the Sun's surface in the form of bipolar magnetic regions is redistributed...