activity
20142023
most citedThe MUSCLES Treasury Survey IV: Scaling Relations for Ultraviolet, Ca II K, and Energetic Particle Fluxes from M Dwarfs

123 citations · 676 across the 29 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

17 papers · 1 filter

astro-ph.SR2023★ 17 cited

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…

astro-ph.SR2023★ 8 cited

Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case Studies

James Paul Mason, Alexandra Werth, Colin G. West +999

Flare frequency distributions represent a key approach to addressing one of the largest problems in solar and stellar physics: determining the mechanism that counter-intuitively he…

astro-ph.SR2022★ 3 cited

SuNeRF: Validation of a 3D Global Reconstruction of the Solar Corona Using Simulated EUV Images

Kyriaki-Margarita Bintsi, Robert Jarolim, Benoit Tremblay +8

Extreme Ultraviolet (EUV) light emitted by the Sun impacts satellite operations and communications and affects the habitability of planets. Currently, EUV-observing instruments are…

astro-ph.SR2022★ 56 cited

Defining the Middle Corona

Matthew J. West, Daniel B. Seaton, David B. Wexler +31

The middle corona, the region roughly spanning heliocentric altitudes from to , encompasses almost all of the influential physical transitions and processes that…

astro-ph.SR2022★ 5 cited

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…

astro-ph.SR2022★ 42 cited

Constraining the Physical Properties of Stellar Coronal Mass Ejections with Coronal Dimming: Application to Far Ultraviolet Data of Eridani

R. O. Parke Loyd, James Mason, Meng Jin +9

Coronal mass ejections (CMEs) are a prominent contributor to solar system space weather and might have impacted the Sun's early angular momentum evolution. A signal diagnostic of C…

astro-ph.SR2021

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…

astro-ph.SR2020

Solar Analogs as a Tool to Understand the Sun

Allison Youngblood, Steve Cranmer, Sam Van Kooten +6

Solar analogs, broadly defined as stars similar to the Sun in mass or spectral type, provide a useful laboratory for exploring the range of Sun-like behaviors and exploring the phy…

astro-ph.SR2020

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…

astro-ph.SR2020★ 20 cited

Soft X-Ray Observations of Quiescent Solar Active Regions using Novel Dual-zone Aperture X-ray Solar Spectrometer (DAXSS)

Bennet D. Schwab, Robert H. A. Sewell, Thomas N. Woods +3

The Dual-zone Aperture X-ray Solar Spectrometer (DAXSS) was flown on 2018 June18 on the NASA 36.336 sounding rocket flight and obtained the highest resolution to date for solar sof…

astro-ph.SR2020★ 14 cited

Coronal Dimming as a Proxy for Stellar Coronal Mass Ejections

Meng Jin, Mark C. M. Cheung, Marc L. DeRosa +6

Solar coronal dimmings have been observed extensively in the past two decades and are believed to have close association with coronal mass ejections (CMEs). Recent study found that…

astro-ph.SR2019★ 1 cited

EUV observations of cool dwarf stars

Allison Youngblood, Jeremy Drake, James Mason +15

The EUV (100-912 Å) is a spectral region notoriously difficult to observe due to attenuation by neutral hydrogen gas in the interstellar medium. Despite this, hundreds to thousands…

astro-ph.SR2018★ 56 cited

The Instruments and Capabilities of the Miniature X-ray Solar Spectrometer (MinXSS) CubeSats

Christopher S. Moore, Amir Caspi, Thomas N. Woods +6

The Miniature X-ray Solar Spectrometer (MinXSS) CubeSat is the first solar science oriented CubeSat mission flown for the NASA Science Mission Directorate, with the main objective…

astro-ph.SR2017★ 123 cited

The MUSCLES Treasury Survey IV: Scaling Relations for Ultraviolet, Ca II K, and Energetic Particle Fluxes from M Dwarfs

Allison Youngblood, Kevin France, R. O. Parke Loyd +18

Characterizing the UV spectral energy distribution (SED) of an exoplanet host star is critically important for assessing its planet's potential habitability, particularly for M dwa…

astro-ph.SR2016★ 49 cited

New Solar Irradiance Measurements from the Miniature X-Ray Solar Spectrometer CubeSat

Thomas N. Woods, Amir Caspi, Phillip C. Chamberlin +9

The goal of the Miniature X-ray Solar Spectrometer (MinXSS) CubeSat is to explore the energy distribution of soft X-ray (SXR) emissions from the quiescent Sun, active regions, and…

astro-ph.SR2016★ 76 cited

Relationship of EUV Irradiance Coronal Dimming Slope and Depth to Coronal Mass Ejection Speed and Mass

James Paul Mason, Thomas N. Woods, David F. Webb +3

Extreme ultraviolet (EUV) coronal dimmings are often observed in response to solar eruptive events. These phenomena can be generated via several different physical processes. For s…

astro-ph.SR2014★ 58 cited

Mechanisms and Observations of Coronal Dimming for the 2010 August 7 Event

J. P. Mason, T. N. Woods, A. Caspi +2

Coronal dimming of extreme ultraviolet (EUV) emission has the potential to be a useful forecaster of coronal mass ejections (CMEs). As emitting material leaves the corona, a tempor…