7 citations · 7 across the 3 of their papers we have counts for
4 papers
Understanding how Coronal Heating and Magnetic Field Scaling Affect Global Properties of the Low and Middle Corona
Caroline L. Evans, Cooper Downs, Donald Schmit
The magnetic field of the Sun is a key driver of coronal heating and solar wind acceleration. In tandem, these influence the observable morphology of the corona, along with definin…
Quantifying how Surface Complexity Influences Properties of the Solar Corona and Solar Wind
Caroline L. Evans, Cooper Downs, Donald Schmit
The Sun's magnetic field is a key driver in coronal heating and consequently solar wind acceleration. Remote measurement of the photosphere provides the magnetic surface boundary c…
Unveiling Unprecedented Fine Structure in Coronal Flare Loops with the DKIST
Cole A. Tamburri, Maria D. Kazachenko, Gianna Cauzzi +8
We present the highest-resolution H observations of a solar flare to date, collected during the decay phase of an X1.3-class flare on 8 August 2024 at 20:12 UT. Observations wit…
Are the brightest coronal loops always rooted in mixed-polarity magnetic flux?
Sanjiv K. Tiwari, Caroline L. Evans, Navdeep K. Panesar +2
A recent study demonstrated that freedom of convection and strength of magnetic field in the photospheric feet of active-region (AR) coronal loops, together, can engender or quench…