output
20062026
most citedSolar Coronal Jets: Observations, Theory, and Modeling

361 citations

Showing 2014Show all

6 papers · 1 filter

astro-ph.SR2014★ 92 cited

Quasi-periodic pulsations in solar and stellar flares: re-evaluating their nature in the context of power-law flare Fourier spectra

A. R. Inglis, J. Ireland, M. Dominique

The nature of quasi-periodic pulsations in solar and stellar flares remains debated. Recent work has shown that power-law-like Fourier power spectra, also referred to as 'red' nois…

astro-ph.SR2014★ 251 cited

Key Aspects of Coronal Heating

James A. Klimchuk

We highlight ten key aspects of coronal heating that must be understood before we can consider the problem to be solved. (1) All coronal heating is impulsive. (2) The details of co…

astro-ph.SR2014★ 110 cited

The Radiated Energy Budget of Chromospheric Plasma in a Major Solar Flare Deduced From Multi-Wavelength Observations

Ryan O. Milligan, Graham S. Kerr, Brian R. Dennis +7

This paper presents measurements of the energy radiated by the lower solar atmosphere, at optical, UV, and EUV wavelengths, during an X-class solar flare (SOL2011-02-15T01:56) in r…

astro-ph.SR2014★ 12 cited

Relaxation Processes in Solar Wind Turbulence

S. Servidio, C. Gurgiolo, V. Carbone +1

Based on global conservation principles, magnetohydrodynamic (MHD) relaxation theory predicts the existence of several equilibria, such as the Taylor state or global dynamic alignm…

hep-ph2014★ 7 cited

Precision measurements of θ12 for testing models of discrete leptonic flavour symmetries

Peter Ballett, Stephen F. King, Christoph Luhn +2

Models of leptonic flavour with discrete symmetries can provide an attractive explanation of the pattern of elements found in the leptonic mixing matrix. The next generation of neu…

astro-ph.SR2014★ 41 cited

Investigating the differential emission measure and energetics of microflares with combined SDO/AIA and RHESSI observations

A. R. Inglis, S. Christe

An important question in solar physics is whether solar microflares, the smallest currently observable flare events in X-rays, possess the same energetic properties as large flares…