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Going Nuclear: Notes from the officially unofficial book tour
I work in the analytical labs at one of Europe’s oldest and largest nuclear sites: Sellafield, in northwestern England. I spend my days at the fume hood front, pipette in one hand and radiation probe in the other (and dosimeter pinned to my chest, of course). Outside the lab, I have a second job: I moonlight as a writer and public speaker. My new popular science book—Going Nuclear: How the Atom Will Save the World—came out last summer, and it feels like my life has been running at full power ever since.
Nailya S. Akhmadullina, Valentin D. Borzosekov, Nina N. Skvortsova, Vladimir D. Stepakhin, Namik G. Gusein-Zade, Dmitriy V. Malakhov, Alexander V. Knyazev, Tatiana E. Gayanova, Anastasiya K. Kozak, Alexander S. Sokolov, Karen A. Sarksyan, Aleksey V. Ishchenko, Ilya A. Weinstein, Victor I. Grokhovsky, Oleg N. Shishilov
Fusion Science and Technology | Volume 80 | Number 7 | October 2024 | Pages 870-881
Research Article | doi.org/10.1080/15361055.2023.2250669
Articles are hosted by Taylor and Francis Online.
A new approach for simulation of the interaction of space and lunar dust with the surface of spacecrafts has been proposed. The approach is based on creating a dusty plasma cloud when the substance imitating the space or lunar dust is treated with high-power pulsed microwave radiation in the developed experimental facility. The facility consists of a high-power gyrotron (75 GHz, 0.8 MW); a plasma-chemical reactor; and a diagnostic complex, which includes optical emission spectrometers and a high-speed camera. The approach has been tested using the substance of the Tsarev meteorite, which represents a typical substance of meteorites. It was found that the substance mainly keeps the phase composition; however, the particles change their morphology due to rapid heating and melting.