3 papers
astro-ph.SR2024
131 and 304 Å Emission Variability Increases Hours Prior to Solar Flare Onset
Kara L. Kniezewski, Emily I. Mason, Vadim M. Uritsky +1
Thermal changes in coronal loops are well-studied, both in quiescent active regions and in flaring scenarios. However, relatively little attention has been paid to loop emission in…
astro-ph.IM2023
Small Platforms, High Return: The Need to Enhance Investment in Small Satellites for Focused Science, Career Development, and Improved Equity
James Paul Mason, Robert G. Begbie, Maitland Bowen +33
In the next decade, there is an opportunity for very high return on investment of relatively small budgets by elevating the priority of smallsat funding in heliophysics. We've lear…
astro-ph.IM2023
Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release
Amir Caspi, Daniel B. Seaton, Roberto Casini +12
The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…