NuSTAR observations of 113 faint solar X-ray transients show they are cooler and dimmer than RHESSI microflares, with quiet-Sun events having lower energies and no cases above 3x10^27 erg.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
representative citing papers
Network regions with more compact positive-polarity magnetic features produce both visible coronal plumes and higher, faster transition-region jets.
Long-term near-Earth solar wind observations establish a robust empirical connection between flow speed and magnetohydrodynamic turbulence energy.
citing papers explorer
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A Statistical Survey of Faint Solar X-ray Transients Observed by NuSTAR
NuSTAR observations of 113 faint solar X-ray transients show they are cooler and dimmer than RHESSI microflares, with quiet-Sun events having lower energies and no cases above 3x10^27 erg.
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On the relation between transition region network jets and coronal plumes
Network regions with more compact positive-polarity magnetic features produce both visible coronal plumes and higher, faster transition-region jets.
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A robust empirical relationship between speed and turbulence energy in the near-Earth solar wind
Long-term near-Earth solar wind observations establish a robust empirical connection between flow speed and magnetohydrodynamic turbulence energy.