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Increased diagnostic capability of the EUV Imaging Spectrometer (EIS) aboard Hinode (former Solar-B) has been demonstrated with a set of iron emission lines emerging in the two EIS observing wavelength bands (170–210 Å and 250–290 Å) and their line-intensity ratios. “Abundance-uncertainty” free relative emission measure distributions as a function of temperature were deduced using only iron emissi...

Temperature and Density Structures of Solar Corona—A Test of Iron Line Diagnostic Capability of EIS Instrument on Board Hinode