NASA NTRS · 20140011665
Sounding Rocket Instrument Development at UAHuntsville/NASA MSFC
Abstract
We present an overview of solar sounding rocket instruments developed jointly by NASA Marshall Space Flight Center and the University of Alabama in Huntsville. The High Resolution Coronal Imager (Hi-C) is an EUV (19.3 nm) imaging telescope which was flown successfully in July 2012. The Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP) is a Lyman Alpha (121.6 nm) spectropolarimeter developed jointly with the National Astronomical Observatory of Japan and scheduled for launch in 2015. The Marshall Grazing Incidence X-ray Spectrograph is a soft X-ray (0.5-1.2 keV) stigmatic spectrograph designed to achieve 5 arcsecond spatial resolution along the slit.
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Kobayashi, Ken, Cirtain, Jonathan, Winebarger, Amy, Savage, Sabrina, Golub, Leon, Korreck, Kelly, Kuzin, Sergei, Walsh, Robert, DeForest, Craig, DePontieu, Bart, Title, Alan, Podgorski, William, Kano, Ryouhei, Narukage, Noriyuki, Trujillo-Bueno, Javier. 2013-08-25. Sounding Rocket Instrument Development at UAHuntsville/NASA MSFC. https://ntrs.nasa.gov/citations/20140011665
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