Nonsolar astronomy with the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI)

By David M. Smith, R. Lin, K. Hurley, W. Coburn, G. Hurford, C. Wigger, W. Hajdas, A. Zehnder, Mark McConnell. SPIE Astronomical Telescopes + Instrumentation, 2003

1,359 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/58b4c2dd433303400e6b26f9121e501f103ba112

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In Astronomy and Astrophysics

1. M. Temmer
2. B. Vršnak
3. Wei Liu
4. H. Hudson
5. J. C. Raymond
6. Jasmina Magdalenic
7. Astrid Veronig
8. Kazunari Shibata

In Nuclear and High Energy Physics

1. J. C. Raymond
2. H. Hudson
3. L. Fletcher
4. J. Laming

Citations in the corpus

• Single disperser design for coded aperture snapshot spectral imaging. (2008, methodology): “Spectral imaging is a technique that generates a spatial map of spectral variation, making it a useful tool in many applications including environmental remote sensing [1], military target discrimination [2], astrophysics [ 3 ], and biomedical optics [4].”
• The FIP and Inverse FIP Effects in Solar and Stellar Coronae (2015, background): “Later work with RHESSI (Lin et al., 2004) found much stronger enhancements in the abundance of Fe relative to H from line to continuum measurements (Phillips et al.”