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Edward Hertz

Researcher at Smithsonian Astrophysical Observatory

Publications -  15
Citations -  2391

Edward Hertz is an academic researcher from Smithsonian Astrophysical Observatory. The author has contributed to research in topics: Spectrometer & Telescope. The author has an hindex of 7, co-authored 12 publications receiving 2211 citations.

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Journal ArticleDOI

The Interface Region Imaging Spectrograph (IRIS)

TL;DR: The Interface Region Imaging Spectrograph (IRIS) as mentioned in this paper provides simultaneous spectra and images of the photosphere, chromosphere, transition region, and corona with 0.33 arcsec and up.
Journal ArticleDOI

The Interface Region Imaging Spectrograph (IRIS)

TL;DR: The Interface Region Imaging Spectrograph (IRIS) as mentioned in this paper is a small explorer spacecraft that provides simultaneous spectra and images of the photosphere, chromosphere, transition region, and corona with 0.33-0.4 arcsec spatial resolution, 2 s temporal resolution and 1 km/s velocity resolution over a field-of-view of up to 175 arcsec.
Proceedings ArticleDOI

Arcus: the x-ray grating spectrometer explorer

TL;DR: Arcus as discussed by the authors is a free-flying satellite mission that will enable high-resolution soft X-ray spectroscopy (8-50) with unprecedented sensitivity, effective areas of >500 sq cm and spectral resolution >2500.
Proceedings ArticleDOI

The Marshall Grazing Incidence X-ray Spectrometer (MaGIXS)

TL;DR: The Marshall Grazing Incidence X-ray Spectrometer (MaGIXS) as discussed by the authors is a NASA sounding rocket instrument designed to obtain spatially resolved soft Xray spectra of the solar atmosphere in the 6-24 A (0.5-2.0 keV) range.
Proceedings ArticleDOI

On the Alignment and Focusing of the Marshall Grazing Incidence X-Ray Spectrometer (MaGIXS)

TL;DR: The Marshall Grazing Incidence X-ray Spectrometer (MaGIXS) as discussed by the authors is a NASA sounding rocket instrument that is designed to observe soft Xray emissions from 24 - 6.0 A (0.5 - 2.0 keV energies) in the solar atmosphere.