First NuSTAR Limits on Quiet Sun Hard X-Ray Transient Events
Andrew J. Marsh, David M. Smith, Lindsay Glesener, Iain G. Hannah,, Brian W. Grefenstette, Amir Caspi, S\"am Krucker, Hugh S. Hudson, Kristin K., Madsen, Stephen M. White, Matej Kuhar, Paul J. Wright, Steven E. Boggs, Finn, E. Christensen, William W. Craig, Charles J. Hailey

TL;DR
This study uses NuSTAR to set the first upper limits on transient hard X-ray emissions from the quiet Sun, improving sensitivity and providing constraints on solar microflare activity in hard X-ray bands.
Contribution
It demonstrates NuSTAR's capability to observe the quiet Sun in hard X-rays and establishes upper limits on transient emissions, advancing solar X-ray observational techniques.
Findings
Set upper limits on quiet Sun hard X-ray emissions in 2.5-4 keV and 10-20 keV bands.
Detected no transient brightenings above the established thresholds.
Projected increased sensitivity during solar minimum with future observations.
Abstract
We present the first results of a search for transient hard X-ray (HXR) emission in the quiet solar corona with the \textit{Nuclear Spectroscopic Telescope Array} (\textit{NuSTAR}) satellite. While \textit{NuSTAR} was designed as an astrophysics mission, it can observe the Sun above 2~keV with unprecedented sensitivity due to its pioneering use of focusing optics. \textit{NuSTAR} first observed quiet Sun regions on 2014 November 1, although out-of-view active regions contributed a notable amount of background in the form of single-bounce (unfocused) X-rays. We conducted a search for quiet Sun transient brightenings on time scales of 100 s and set upper limits on emission in two energy bands. We set 2.5--4~keV limits on brightenings with time scales of 100 s, expressed as the temperature T and emission measure EM of a thermal plasma. We also set 10--20~keV limits on brightenings with…
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