activity
20172020
most citedThe MUSCLES Treasury Survey IV: Scaling Relations for Ultraviolet, Ca II K, and Energetic Particle Fluxes from M Dwarfs

123 citations · 124 across the 6 of their papers we have counts for

collaborators

7 papers

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

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.IM2019

Advanced Astrophysics Discovery Technology in the Era of Data Driven Astronomy

Richard K. Barry, Jogesh G. Babu, John G. Baker +12

Experience suggests that structural issues in how institutional Astrophysics approaches data-driven science and the development of discovery technology may be hampering the communi…

astro-ph.SR20191 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.EP2019

EUV influences on exoplanet atmospheric stability and evolution

Allison Youngblood, Kevin France, Tommi Koskinen +15

The planetary effective surface temperature alone is insufficient to characterize exoplanet atmospheres and their stability or evolution. Considering the star-planet system as a wh…