Understanding the mechanism that causes the emergence of magnetic flux from the solar interior to the atmosphere, the drastic changes in the properties of the...
Magnetic Flux Emergence Observed with the Advanced Stokes Polarimeter
We have carried out quantitative observations of the vector magnetic field during the emergence of three small bipolar active regions in June, 1992, July 1993...
Magnetic Landscape Of Solar Polar Region With Solar Optical Telescope Aboard Hinode
Solar polar region is the final destination for remnant magnetic fields due to meridional flow and granular diffusion, and is very important for the global...
The magnetic sensitivity of the solar spectrum is caused by the Zeeman effect and by a variety of less familiar physical mechanisms by means of which a magnetic...
Bright points (BPs) visible in the G band at 430 nm are commonly used as tracers of magnetic fields, indicating the location of kG flux concentrations. To study...
Magnetic support and Alfvén heating in quasar broad-line region clouds
Gonçalves et al. (1996) showed the relevance of Alfvén heating in order to establish the stability of quasar broad-line region clouds in the intercloud medium...