High Resolution Studies of Solar Flares, Active Regions, Prominences, and the Quiet Sun at Centimeter and Millimeter Wavelengths

该建议为马里兰州大学开展的地面太阳射电天文学提供了核心支持。 该观测计划使用了来自甚大天线阵（VLA）、伯克利-伊利诺伊州马里兰州毫米波天线阵（比马）、野边山射电日像仪（NoRH）和南凯多频射电日像仪的数据。 它将解决日地研究中的一些悬而未决的问题，包括：㈠日冕磁场和相关电流系统的推断，㈡兆电子伏能量电子的特性，㈢耀斑加速点的大小、形态和空间分布的统计调查，㈣分米波长太阳大气中物理过程的新观点，以及（v）太阳活动区及其周围的环-环相互作用的性质。

This proposal provides the core support for ground-based solar radio astronomy carried out at the University of Maryland. This observational program employs data from the Very Large Array (VLA), the Berkeley-Illinois-Maryland Millimeter Array (BIMA), the Nobeyama Radioheliograph (NoRH), and the Nancay Multifrequency Radioheliograph. It will address a number of outstanding problems in solar-terrestrial research including, (i) the inference of coronal magnetic fields and associated electric current systems, (ii) the properties of MeV-energy electrons, (iii) a statistical survey of the sizes, morphology and spatial distribution of flare acceleration sites, (iv) new views of physical processes in the solar atmosphere at decimetric wavelengths, and (v) the nature of loop-loop interactions in and around solar active regions.