Do you have a favorite RHESSI Science Nugget? The following list contains nominees in 12 categories, the descriptions of which will remain unknown until the glamorous and spectacular Award Ceremony. After considering the candidates, please vote for no more than three in the form below.
100: RHESSI: Concept to Fruition (Dennis & Lin)
203: Minoflares - Earmarks of widespread energetic events in the solar atmosphere (Hannah & Hudson)
264: How to better determine the power in non-thermal electrons from observed X-ray spectra - Incorporation of energy diffusion for electron transport helps with flare energetics (Kontar, Emslie, Jeffrey, & Bian)
292: RHESSI's 15th Anniversary - RHESSI celebrates 15 years in orbit (Dennis, Krucker, & Shih)
306: The Last Best Flare of Cycle 24? - Right on schedule, Cycle 24 has produced a great flare (with a GLE) (Krucker & Hudson)
307: The Kelvin Force and Loop-Top Concentration - New physics can explain the perplexing overpressure at the flare looptop regions (Shibasaki)
308: The Power of Turbulence - Turbulent energy content may underlie flare energy transfer, magnetic reconnection, and particle acceleration. (Bian)
323: To Beam or Not to Beam - Descriptions of the lower solar atmosphere of flares ca. Cycle 21 sound surprisingly current (Simoes & Hudson)
327: Microwave Imaging Spectroscopy of Flares is Here - Microwave imaging spectroscopy takes a giant leap forward with SOL2017-09-10 (Gary & two large teams)
330: Understanding the co-spatial return current in solar flares - Completing the circuit in a thick-target model (Alaoui & Holman)
336: Remembering Marcos Machado via his Research - Recalling a friend and colleague, and admiring his final paper (Hudson)
340: The flight of FOXSI-3 - Single-photon counting and direct focusing across hard and soft energies (Glesener & Narukage)
