Physics
Scientist
Sterrewacht Sonnenborgh, Utrecht, Netherlands
High-resolution spectroscopy of active regions. I - Observing procedures
High-resolution spectroscopy of active regions. II Line-profile interpretation, applied to an emerging flux region
High-resolution spectroscopy of active regions. III - Relations between the intensity, velocity, and magnetic structure in an emerging flux region
Morphological evolution of an emerging flux region
The structure of sunspots. IV - Magnetic field strengths in small sunspots and pores
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