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Mark C. M. Cheung

Researcher at Stanford University

Publications -  123
Citations -  8217

Mark C. M. Cheung is an academic researcher from Stanford University. The author has contributed to research in topics: Photosphere & Magnetohydrodynamics. The author has an hindex of 39, co-authored 105 publications receiving 7188 citations. Previous affiliations of Mark C. M. Cheung include Advanced Technology Center & Max Planck Society.

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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.
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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.
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Simulation of the formation of a solar active region

TL;DR: In this article, a radiative magnetohydrodynamics simulation of the formation of an active region (AR) on the solar surface is presented, where the authors model the rise of a buoyant magnetic flux bundle from a depth of 7.5 Mm in the convection zone up into the solar photosphere.
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Thermal diagnostics with the atmospheric imaging assembly on board the solar dynamics observatory: a validated method for differential emission measure inversions

TL;DR: In this paper, a method for performing differential emission measure (DEM) inversions on narrow-band EUV images from the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory is presented.