首页> 外文期刊>Physica Scripta: An International Journal for Experimental and Theoretical Physics >New solar telescope in Big Bear: Evidence for super-diffusivity and small-scale solar dynamos?
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New solar telescope in Big Bear: Evidence for super-diffusivity and small-scale solar dynamos?

机译:Big Bear中的新型太阳望远镜:是否具有超扩散性和小规模太阳动力的证据?

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摘要

The 1.6m clear aperture New Solar Telescope (NST) in Big Bear Solar Observatory (BBSO) is now providing the highest resolution solar data ever. These data have revealed surprises about the Sun on small-scales including the observation that bright points (BPs), which can be used as proxies for the intense, compact magnetic elements that are apparent in photospheric intergranular lanes. The BPs are ever more numerous on ever smaller spatial scales as though there were no limit to how small the BPs can be. Here we discuss high resolution NST data on BPs that provide support for the ideas that a turbulent regime of super-diffusivity dominates in the quiet Sun, and there are local dynamos operating near the solar surface.
机译:大熊太阳天文台(BBSO)的1.6m透明光圈新型太阳望远镜(NST)现在提供有史以来最高分辨率的太阳数据。这些数据在小范围内揭示了关于太阳的惊奇,包括观察到亮点(BPs)可以用作光球粒间车道中明显的强而紧凑的磁性元素的代表。在较小的空间尺度上,BP越来越多,好像对BP的大小没有限制。在这里,我们讨论了有关BP的高分辨率NST数据,这些数据为以下观点提供了支持:在安静的太阳下,湍流的超扩散性占主导地位,并且在太阳表面附近有局部动力。

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