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由于表面磁性导致的明显太阳扁率的大量过剩。

A large excess in apparent solar oblateness due to surface magnetism.

作者信息

Fivian Martin D, Hudson Hugh S, Lin Robert P, Zahid H Jabran

机构信息

Space Sciences Laboratory, University of California-Berkeley, Berkeley, CA 94720, USA.

出版信息

Science. 2008 Oct 24;322(5901):560-2. doi: 10.1126/science.1160863. Epub 2008 Oct 2.

Abstract

The shape of the Sun subtly reflects its rotation and internal flows. The surface rotation rate, approximately 2 kilometers per second at the equator, predicts an oblateness (equator-pole radius difference) of 7.8 milli-arc seconds, or approximately 0.001%. Observations from the Reuven Ramaty High-Energy Solar Spectroscopic Imager satellite show unexpectedly large flattening, relative to the expectation from surface rotation. This excess is dominated by the quadrupole term and gives a total oblateness of 10.77 +/- 0.44 milli-arc seconds. The position of the limb correlates with a sensitive extreme ultraviolet proxy, the 284 angstrom limb brightness. We relate the larger radius values to magnetic elements in the enhanced network and use the correlation to correct for it as a systematic error term in the oblateness measurement. The corrected oblateness of the nonmagnetic Sun is 8.01 +/- 0.14 milli-arc seconds, which is near the value expected from rotation.

摘要

太阳的形状微妙地反映了其自转和内部流动情况。太阳表面的自转速度在赤道处约为每秒2公里,据此预测其扁率(赤道半径与极半径之差)为7.8毫角秒,约为0.001%。鲁文·拉马蒂高能太阳光谱成像卫星的观测结果显示,相对于表面自转的预期值,太阳的扁率出人意料地大。这种偏差主要由四极项主导,总扁率为10.77±0.44毫角秒。太阳边缘的位置与一个敏感的极紫外代理指标——284埃的边缘亮度相关。我们将较大的半径值与增强网络中的磁元素联系起来,并利用这种相关性将其作为扁率测量中的一个系统误差项进行校正。非磁性太阳经校正后的扁率为8.01±0.14毫角秒,接近自转预期值。

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