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3![Reprinted from the Journal of Geophysical Research, 102, 14031, 1997. material. In soft X-rays (SXRs), eruptive morpholo- gies have been identi
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4![Long-term trends in chromospheric activity Long-term trends in chromospheric activity](https://www.pdfsearch.io/img/26044e1bfbcbd37f407ad2d5efa4de5a.jpg) | Add to Reading ListSource URL: www.spaceclimate.fiLanguage: English - Date: 2016-04-11 08:21:19
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6![In the shops Daystar’s new views of the Sun On the odd days this summer when it didn’t rain, Steve Ringwood discarded his umbrella to ogle at that rarest of sights – the Sun – through Daystar’s new SolaREDi 80 In the shops Daystar’s new views of the Sun On the odd days this summer when it didn’t rain, Steve Ringwood discarded his umbrella to ogle at that rarest of sights – the Sun – through Daystar’s new SolaREDi 80](https://www.pdfsearch.io/img/206180404de4f8a1e45b2778b4f7b0a1.jpg) | Add to Reading ListSource URL: www.daystarfilters.comLanguage: English - Date: 2012-12-16 18:40:58
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7![Vector Spectromagnetograph 1. Introduction The Vector Spectromagnetograph (VSM) is responsible for taking high-quality magnetic field observations in the photosphere and the chromosphere by recording the Zeeman-induced p Vector Spectromagnetograph 1. Introduction The Vector Spectromagnetograph (VSM) is responsible for taking high-quality magnetic field observations in the photosphere and the chromosphere by recording the Zeeman-induced p](https://www.pdfsearch.io/img/8e4bbd7bb755aac87df2074313115244.jpg) | Add to Reading ListSource URL: nisp.nso.eduLanguage: English - Date: 2013-03-14 14:05:32
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8![Solar Physics DOI: /•••••-•••-•••-••••-• A Rapid, Manual Method to Map Coronal-Loop Structures of an Active Region Using Cubic B´ ezier Solar Physics DOI: /•••••-•••-•••-••••-• A Rapid, Manual Method to Map Coronal-Loop Structures of an Active Region Using Cubic B´ ezier](https://www.pdfsearch.io/img/b617c0b40a69d9dde3d1698b92c3ba73.jpg) | Add to Reading ListSource URL: solarscience.msfc.nasa.govLanguage: English - Date: 2013-07-08 09:59:41
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9![Science The chromosphere’s temperature increases with distance from the Sun’s surface, Science The chromosphere’s temperature increases with distance from the Sun’s surface,](https://www.pdfsearch.io/img/f64f3f5f2621184c25e6392d125b42fb.jpg) | Add to Reading ListSource URL: www.mssl.ucl.ac.uk- Date: 2013-11-04 13:23:52
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10![GLOSSARY 《Physics of the Sun》Glossary Chromosphere :【彩層】 The atmospheric layer outer than the photosphere, which iskm thick and is about 104 K temperature slightly hotter than the photosphere. The GLOSSARY 《Physics of the Sun》Glossary Chromosphere :【彩層】 The atmospheric layer outer than the photosphere, which iskm thick and is about 104 K temperature slightly hotter than the photosphere. The](https://www.pdfsearch.io/img/1a64ca2e9951e5b2746282a187e51511.jpg) | Add to Reading ListSource URL: www.jsps.go.jp- Date: 2013-12-26 00:19:02
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