Solar-B EUV Imaging Spectrometer

H. Hara

The performance of Solar-B EUV Imaging Spectrometer is briefly introduced. It covers two spectral ranges of 17 - 21 nm and 25 - 29 nm which contain emission lines from highly ionized species at temperatures of log T = 4.7 - 7.3. Target spatial and spectral resolutions as well as high throughput have been confirmed through calibration measurements. Science outputs from this instrument will strongly depend on on-orbit science operations because of its versatility.

Correspondence

Hirohisa Hara (hirohisa.hara@nao.ac.jp), NAOJ

presentation

oral