Identifying Coronal Holes in Solar Disk Images (and how to compare to models) Working Group Report Nick Arge Rachel Hock Carl Henney.
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.
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.
Low-Coronal and Coronagraphic Images: Their Complementary Roles in Understanding Geo-Effective Eruptions N. V. Nitta, Lockheed Martin Solar and Astrophysics.
Measures of solar oblateness using active- region masking H.J. Zahid, M.D. Fivian, H.S. Hudson Space Sciences Lab, UC Berkeley.
Growing the Space Weather Business (Using the Four Basic C.H. Strong Business Growth Techniques)
Conclusions. 1. Plasma parameters in the arcade: Ne ~10 10 cm -3 , Te ~6 MK.
XUV monochromatic imaging spectroscopy in the SPIRIT experiment on the CORONAS-F mission
Identifying Coronal Holes in Solar Disk Images (and how to compare to models)
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N. V. Nitta, Lockheed Martin Solar and Astrophysics Lab.
