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The top documents tagged [euv images]
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Identifying Coronal Holes in Solar Disk Images (and how to compare to models) Working Group Report Nick Arge Rachel Hock Carl Henney
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Observations. The SPIRIT sometimes observes in a high-temperature Mg XII 8.42 Å line large-scale features existing many hours high in the corona (Zhitnik
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Instructor Notes There is one picture of the Sun in all wavelengths except: Gamma ray – there are no images of the full Sun in gamma ray
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Low-Coronal and Coronagraphic Images: Their Complementary Roles in Understanding Geo-Effective Eruptions N. V. Nitta, Lockheed Martin Solar and Astrophysics
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Measures of solar oblateness using active- region masking H.J. Zahid, M.D. Fivian, H.S. Hudson Space Sciences Lab, UC Berkeley
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Growing the Space Weather Business (Using the Four Basic C.H. Strong Business Growth Techniques)
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Conclusions. 1. Plasma parameters in the arcade: Ne ~10 10 cm -3 , Te ~6 MK
30 views
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XUV monochromatic imaging spectroscopy in the SPIRIT experiment on the CORONAS-F mission
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Identifying Coronal Holes in Solar Disk Images (and how to compare to models)
25 views
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FOREST
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N. V. Nitta, Lockheed Martin Solar and Astrophysics Lab
53 views