【摘要】 本文利用ZFM法则分析了紫金山天文台1979年11月所拍日面16398活动区精细色球照片,探讨了谱斑、耀斑、磁场、波湍动和H_a形态发展间的关系。并试用波场流体场的耦合方程去解释谱斑的垂直加热问题,认为观测到的细长谱斑亮条应是水平湍动加热的表征。更多还原

【Abstract】 According to the ZFM law by which chromospheric magnetic field can be derived, we analyse the fine chromospheric photographs, obtained by Purple mountain Observatory in November 1979, and study the relations among the plage, solar flare, magnetic field, wave turbulence and morphological development in H_α. The coupling equations for the flow-wave fields are applied to solve the problem about perpendicular heating of faeulae. We indicate that the narrow and long bright filament in the plage might be the feature showing horizontal heating.更多还原