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1. Microwave Heating Outperforms Conventional Heating for a Thermal Reaction that Produces a Thermally Labile Product: Observations Consistent with Selective Microwave Heating

   https://doi.org/10.1002/asia.201900625  

   Duangkamol, Chuthamat; Batsomboon, Paratchata; Stiegman, Albert_E; Dudley, Gregory_B (June 2019, Chemistry – An Asian Journal)

   Abstract Microwave (MW) heating is more effective than conventional (CONV) heating for promoting a high‐temperature oxidative cycloisomerization reaction that was previously reported as a key step in a total synthesis of the natural product illudinine. The thermal reaction pathway as envisioned is an inverse electron‐demand dehydro‐Diels–Alder reaction with in situ oxidation to generate a substituted isoquinoline, which itself is unstable to the reaction conditions. Observed reaction yields were higher at a measured bulk temperature of 200 °C than at 180 °C or 220 °C; at 24 hours than at earlier or later time points; and when the reaction solution was heated using MW energy as opposed to CONV heating with a metal heat block. Selective MW heating of polar solute aggregates is postulated to explain these observations. 

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2. Pretreatment of waste biomass in deep eutectic solvents: Conductive heating versus microwave heating

   https://doi.org/10.1016/j.indcrop.2019.111865  

   Kumar, Narendra; Muley, Pranjali D; Boldor, Dorin; Coty, Gary G; Lynam, Joan G (December 2019, Industrial Crops and Products)
3. Navigating Soft Robots through Wireless Heating

   https://doi.org/10.1109/ICRA48891.2023.10161540  

   Song, Yiwen; Zadan, Mason; Misra, Kushaan; Li, Zefang; Wang, Jingxian; Majidi, Carmel; Kumar, Swarun (May 2023, ICRA 2023)
4. Emerging Dimming as Coronal Heating Episodes

   https://doi.org/10.3847/1538-4357/abee8d  

   Payne, Anna V.; Sun, Xudong (April 2021, The Astrophysical Journal)

   Abstract Emerging dimming occurs in isolated solar active regions (ARs) during the early stages of magnetic flux emergence. Observed by the Atmospheric Imaging Assembly, it features a rapid decrease in extreme-ultraviolet (EUV) emission in the 171 Å channel images, and a simultaneous increase in the 211 Å images. Here, we analyze the coronal thermodynamic and magnetic properties to probe its physical origin. We calculate the time-dependent differential emission measures for a sample of 18 events between 2010 and 2012. The emission measure (EM) decrease in the temperature range is well correlated with the EM increase in over eight orders of magnitude. This suggests that the coronal plasma is being heated from the quiet-Sun, sub-MK temperature to 1–2 MK, more typical for ARs. Potential field extrapolation indicates significant change in the local magnetic connectivity: the dimming region is now linked to the newly emerged flux via longer loops. We conclude that emerging dimming is likely caused by coronal heating episodes, powered by reconnection between the emerging and the ambient magnetic fields. 

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5. Symbiosis and host responses to heating

   https://doi.org/10.1016/j.tree.2022.03.011  

   Hector, Tobias E.; Hoang, Kim L.; Li, Jingdi; King, Kayla C. (July 2022, Trends in Ecology & Evolution)