Add to ORKGThis thesis presents results concerning the properties of magnetic bright points(MBPs) in the solar atmosphere in different environments obtained using high spatial and temporal resolution observations and numerical solutions. The first study presented looks at the properties of photospheric MBPs in a quiet sun region at disk centre.EThOS - Electronic Theses Online ServiceGBUnited Kingdo
We present a comparative study of photometric and dynamic properties of photospheric bright points (...
The Sun shows a global magnetic field cycle traditionally best visible in the photosphere as a chang...
Magnetic bright points (MBPs) are among the smallest observable objects on the solar photosphere. A ...
Magnetic bright points (MBPs) are small-scale (generally kG) magnetic features, ubiqui- tous in the ...
Magnetic bright points (MBPs) are small-scale magnetic elements ubiquitous across the solar disc, wi...
Magnetic bright points (MBPs) are small-scale magnetic elements ubiquitous across the solar disc, wi...
Context. Bright points (BPs) are small-scale, magnetic features ubiquitous across the solar surface....
Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with f...
Context. High-resolution observations of the solar photosphere reveal the presence of fine structure...
We use high spatial resolution observations and numerical simulations to study the velocity distribu...
High-cadence, multiwavelength observations and simulations are employed for the analysis of solar ph...
We use high spatial resolution observations and numerical simulations to study the velocity distribu...
We present a visual determination of the number of bright points (BPs) existing in the quiet Sun, wh...
We present a comparative study of photometric and dynamic properties of photospheric bright points (...
The Sun shows a global magnetic field cycle traditionally best visible in the photosphere as a chang...
Magnetic bright points (MBPs) are among the smallest observable objects on the solar photosphere. A ...
Magnetic bright points (MBPs) are small-scale (generally kG) magnetic features, ubiqui- tous in the ...
Magnetic bright points (MBPs) are small-scale magnetic elements ubiquitous across the solar disc, wi...
Magnetic bright points (MBPs) are small-scale magnetic elements ubiquitous across the solar disc, wi...
Context. Bright points (BPs) are small-scale, magnetic features ubiquitous across the solar surface....
Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with f...
Context. High-resolution observations of the solar photosphere reveal the presence of fine structure...
We use high spatial resolution observations and numerical simulations to study the velocity distribu...
High-cadence, multiwavelength observations and simulations are employed for the analysis of solar ph...
We use high spatial resolution observations and numerical simulations to study the velocity distribu...
We present a visual determination of the number of bright points (BPs) existing in the quiet Sun, wh...
We present a comparative study of photometric and dynamic properties of photospheric bright points (...
The Sun shows a global magnetic field cycle traditionally best visible in the photosphere as a chang...
Magnetic bright points (MBPs) are among the smallest observable objects on the solar photosphere. A ...