| Reference Type | Journal (article/letter/editorial) |
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| Title | Using a New Infrared Si x Coronal Emission Line for Discriminating between Magnetohydrodynamic Models of the Solar Corona During the 2006 Solar Eclipse |
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| Journal | The Astrophysical Journal |
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| Authors | Dima, Gabriel I. | Author |
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| Kuhn, Jeffrey R. | Author |
| Mickey, Don | Author |
| Downs, Cooper | Author |
| Year | 2018 (January 2) | Volume | 852 |
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| Issue | 1 |
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| Publisher | American Astronomical Society |
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| DOI | doi:10.3847/1538-4357/aa9e87Search in ResearchGate |
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| Generate Citation Formats |
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| Mindat Ref. ID | 3545156 | Long-form Identifier | mindat:1:5:3545156:5 |
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|
| GUID | 0 |
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| Full Reference | Dima, Gabriel I., Kuhn, Jeffrey R., Mickey, Don, Downs, Cooper (2018) Using a New Infrared Si x Coronal Emission Line for Discriminating between Magnetohydrodynamic Models of the Solar Corona During the 2006 Solar Eclipse. The Astrophysical Journal, 852 (1). 23pp. doi:10.3847/1538-4357/aa9e87 |
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| Plain Text | Dima, Gabriel I., Kuhn, Jeffrey R., Mickey, Don, Downs, Cooper (2018) Using a New Infrared Si x Coronal Emission Line for Discriminating between Magnetohydrodynamic Models of the Solar Corona During the 2006 Solar Eclipse. The Astrophysical Journal, 852 (1). 23pp. doi:10.3847/1538-4357/aa9e87 |
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| In | (2018, January) The Astrophysical Journal Vol. 852 (1) American Astronomical Society |
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