activity
20122023
most citedCritical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)

110 citations · 319 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2023★ 2 cited

Are Non-thermal Velocities in Active Region Coronal Loops Anisotropic?

Michael Hahn, Mahboubeh Asgari-Targhi, Daniel Wolf Savin

We have measured line widths in active region coronal loops in order to determine whether the non-thermal broadening is anisotropic with respect to the magnetic field direction. Th…

astro-ph.IM2022★ 2 cited

Deriving instrumental point spread functions from partially occulted images

Stefan Johann Hofmeister, Michael Hahn, Daniel Wolf Savin

The point-spread function (PSF) of an imaging system describes the response of the system to a point source. Accurately determining the PSF enables one to correct for the combined…

astro-ph.SR2022★ 12 cited

Evidence for Parameteric Decay Instability in the Lower Solar Atmosphere

Michael Hahn, Xiangrong Fu, Daniel Wolf Savin

We find evidence for the first observation of the parametric decay instability (PDI) in the lower solar atmosphere. Specifically, we find that the power spectrum of density fluctua…

astro-ph.SR2020★ 110 cited

Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)

Mark P. Rast, Nazaret Bello González, Luis Bellot Rubio +84

The Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand and model the basic physical processes that control the structure and dynamics of…

astro-ph.IM2017★ 28 cited

Electron-Impact Multiple Ionization Cross Sections for Atoms and Ions of Helium through Zinc

Michael Hahn, Alfred Mueller, Daniel Wolf Savin

We have compiled a set of electron-impact multiple ionization (EIMI) cross sections for astrophysically relevant ions. EIMI can have a significant effect on the ionization balance…

astro-ph.SR2016★ 4 cited

Inferring the Coronal Density Irregularity from EUV Spectra

Michael Hahn, Daniel Wolf Savin

Understanding the density structure of the solar corona is important for modeling both coronal heating and the solar wind. Direct measurements are difficult because of line-of-sigh…