Sabrina Savage

TL;DR: In this paper, the authors proposed a solar physics division of the American Astronomical Society (AAS) Division of Astronomy Division of the University of Washington (U.W.

TL;DR: The High-Resolution Coronal Imager (Hi-C) was launched on a NASA sounding rocket on 11 July 2012 to investigate the dynamics of solar coronal structures at small spatial scales as mentioned in this paper.

TL;DR: Though still in active development, SunPy already provides important functionality for solar data analysis, and future releases will build upon and integrate with current work in the Astropy project and the rest of the scientific python community, to bring greater functionality to SunPy users.

TL;DR: The High-Resolution Coronal Imager (Hi-C 2.1) as mentioned in this paper was modified from its original configuration to observe the solar corona in a passband that peaks near 172 A, and used a new, custom-built low-noise camera.

TL;DR: In this article, the authors present high-resolution, high-cadence observations of six fine-scale, on-disk jet-like events observed by the Hi-C 2.1 during its sounding-rocket flight and investigate each event's magnetic setting with co-aligned line-of-sight magnetograms from SDO/HMI.