机译:DOT tomography of the solar atmosphere - VI. Magnetic elements as bright points in the blue wing of H alpha
Univ Utrecht, Sterrekundig Inst, NL-3508 TA Utrecht, Netherlands;
Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway;
Univ Oslo, Ctr Math Applicat, N-0316 Oslo, NorwayNSO Sacramento Peak, Sunspot, NM 88349 USA;
Sun : magnetic fields; Sun : granulation; Sun : photosphere; Sun : chromosphere; CA-II-H; REVERSED GRANULATION; ENERGY-BALANCE; SIMULATIONS; RESOLUTION; TELESCOPE; DYNAMICS; NETWORK; MODELS;