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Internetwork Magnetic Field Distribution from Simultaneous Fe I 1.5 um and Fe i 630 nm Observations

机译：来自同时Fe的互联网磁场分布1.5 um和Fe I 630 NM观察

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摘要

We took simultaneous observations in Fe I 1.5 um and Fe I 630 urn of an internetwork region. We discuss the compatibility of the data in the two spectral ranges, and present results for the magnetic field distribution. We show that the larger contribution comes from hG field strengths.

机译：我们在互联网地区的FE 1.5 UM和FE 630 URN中同时观察。我们讨论了两种光谱范围中数据的兼容性，并对磁场分布的结果进行了结果。我们表明，较大的贡献来自HG现场优势。

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来源
《Solar Polarization Workshop》|2006年||共6页
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作者
NI. J. Martinez Gonzalez; M. Collados; B. Ruiz Cobo;
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正文语种
中图分类太阳的磁场;
关键词
Magnetic; Distribution; Observations;

机译：磁性;分布;观察;

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4. Internetwork Magnetic Field Distribution from Simultaneous Fe I 1.5 um and Fe i 630 nm Observations [C] . NI. J. Martinez Gonzalez, M. Collados, B. Ruiz Cobo Solar Polarization Workshop . 2006

机译：来自同时Fe的互联网磁场分布1.5 um和Fe I 630 NM观察
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机译：同时1.56微米的网络磁场分布和630纳米观测

Internetwork Magnetic Field Distribution from Simultaneous Fe I 1.5 um and Fe i 630 nm Observations

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