Kontar, EP; Perez, JE; Harra, LK; Kuznetsov, AA; Emslie, AG; Jeffrey, NLS; Bian, NH; Kontar, EP; Perez, JE; Harra, LK; Kuznetsov, AA; Emslie, AG; Jeffrey, NLS; Bian, NH; Dennis, BR; - view fewer (2017) Turbulent Kinetic Energy in the Energy Balance of a Solar Flare. Physical Review Letters , 118 , Article 155101. 10.1103/PhysRevLett.118.155101.

Preview

Text Harra_PhysRevLett.118.155101.pdf - Published Version Download (607kB) | Preview

Abstract

The energy released in solar flares derives from a reconfiguration of magnetic fields to a lower energy state, and is manifested in several forms, including bulk kinetic energy of the coronal mass ejection, acceleration of electrons and ions, and enhanced thermal energy that is ultimately radiated away across the electromagnetic spectrum from optical to x rays. Using an unprecedented set of coordinated observations, from a suite of instruments, we here report on a hitherto largely overlooked energy component—the kinetic energy associated with small-scale turbulent mass motions. We show that the spatial location of, and timing of the peak in, turbulent kinetic energy together provide persuasive evidence that turbulent energy may play a key role in the transfer of energy in solar flares. Although the kinetic energy of turbulent motions accounts, at any given time, for only ∼ð0.5–1Þ% of the energy released, its relatively rapid (∼1–10 s) energization and dissipation causes the associated throughput of energy (i.e., power) to rival that of major components of the released energy in solar flares, and thus presumably in other astrophysical acceleration sites.

Download activity - last month

Export as XMLCSVJSON

Download activity - last 12 months

Export as XMLCSVJSON

Downloads by country - last 12 months

Export as CSVXMLJSON

Archive Staff Only

View Item