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Diagnostics of a Coronal Hole and the Adjacent Quiet Sun by The Hinode/EUV Imaging Spectrometer (EIS)

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ON THE DOPPLER VELOCITY OF EMISSION LINE PROFILES FORMED IN THE “CORONAL CONTRAFLOW” THAT IS THE CHROMOSPHERE-CORONA MASS CYCLE

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ACTIVE REGION LOOPS:HINODE/EXTREME-ULTRAVIOLET IMAGING SPECTROMETER OBSERVATIONS

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The Astrophysical Journal 694 (2) 1256 (2009)
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