Measurement of Vector Magnetic Fields, Sunsport Motions, and Doppler Fields, and Observations of Micropores

建议继续在大熊太阳天文台进行太阳研究，利用优越的观测条件和专门的太阳仪器。然后，加州理工学院对获得的数据进行研究。他们建议：1)继续对不同波长的太阳以及多普勒磁场和矢量磁场进行全面的观测。2)连续测量HO活动区的矢量磁场和速度场以及HO的磁性电影，以了解太阳耀斑的成因。3)研究新的数据，显示太阳黑子运动对引起耀斑有很强的影响。4)研究太阳黑子中的运动和流动，以了解它们是如何形成的，以及是什么保持它们的稳定。5)在红外氦谱线上观测太阳耀斑，这到目前为止还不可能定期进行。6)继续我们的高概率太阳耀斑电子警报BEARALERT计划。7)研究太阳黑子结构的重要细节。8)对太阳磁场进行全天候观测，了解其演化和发展。

The proposal is to continue the studies of the Sun at the Big Bear Solar Observatory, exploiting the excellent observing conditions and specialized solar instruments. The data obtained are then studied at Caltech. They propose to: 1) continue comprehensive observations of the Sun in various wavelengths, and of the Doppler and vector magnetic fields. 2) continuous measurements of vector magnetic fields and velocity fields in active regions and magnetic movies in Ho to understand the causes of solar flares. 3) study new data showing a strong influence of sunspot motions in causing flares. 4) study the motions and flows in sunspots to understand how they form and what keeps them stable. 5) observe solar flares in the infrared helium line, hitherto not possible on a regular basis. 6) continue our BEARALERT program of electronic warning of high probability of solar flares. 7) study important details of sunspot structures. 8) make round-the-clock observations of solar magnetic fields to understand their evolution and development.