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First Results for Solar Soft X-ray Irradiance Measurements from the Third Generation Miniature X-Ray Solar Spectrometer
Thomas N. Woods, Bennet Schwab, Robert Sewell +11
Three generations of the Miniature X-ray Solar Spectrometer (MinXSS) have flown on small satellites with the goal "to explore the energy distribution of soft X-ray (SXR) emissions…
Modeling the Daily Variations of the Coronal X-ray Spectral Irradiance with Two Temperatures and Two Emission Measures
Bennet D. Schwab, Thomas N. Woods, James P. Mason
The Miniature X-ray Solar Spectrometer (MinXSS-1) CubeSat observed solar X-rays between 0.5 and 10 keV. A two-temperature, two-emission measure model is fit to each daily averaged…
Fast Prograde Coronal Flows in Solar Active Regions
Hugh S. Hudson, Sargam M. Mulay, Lyndsay Fletcher +6
We report the discovery and characterization of high-speed (>100 km/s) horizontal flows in solar active regions, making use of the Sun-as-a-star spectroscopy in the range 5-105 nm…
Study of Time Evolution of Thermal and Non-Thermal Emission from an M-Class Solar Flare
Shunsaku Nagasawa, Tomoko Kawate, Noriyuki Narukage +3
We conduct a wide-band X-ray spectral analysis in the energy range of 1.5-100 keV to study the time evolution of the M7.6 class flare of 2016 July 23, with the Miniature X-ray Sola…
SunCET: A compact EUV instrument to fill a critical observational gap
James Paul Mason, Phillip C. Chamberlin, Daniel Seaton +16
The Sun Coronal Ejection Tracker (SunCET) is an extreme ultraviolet imager and spectrograph instrument concept for tracking coronal mass ejections through the region where they exp…
CME Acceleration as a Probe of the Coronal Magnetic Field
James Paul Mason, Phillip C. Chamberlin, Thomas N. Woods +5
By 2050, we expect that CME models will accurately describe, and ideally predict, observed solar eruptions and the propagation of the CMEs through the corona. We describe some of t…