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Solar prominence dynamic model
Geomagnetism and Aeronomy, 2014The possibility of solar prominence formation due to the motion of magnetized plasma particles has been studied. As a result of such motions, chromospheric and coronal plasma can locally condense to density ∼1011 cm−3 and to appearance of the current of unmagnetized protons to ∼1012 A, which corresponds to the values typical of prominences.
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Perovskite solar cells with atomically coherent interlayers on SnO2 electrodes
Nature, 2021Hanul Min, Do Yoon Lee, Junu Kim
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Efficient perovskite solar cells via improved carrier management
Nature, 2021Jason J Yoo +2 more
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Pseudo-halide anion engineering for α-FAPbI3 perovskite solar cells
Nature, 2021Jaeki Jeong, Jongdeuk Seo, Haizhou Lu
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Piecewise mass flows within a solar prominence observed by the New Vacuum Solar Telescope
, 2018Hongbo Li +4 more
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The global incidence of lip, oral cavity, and pharyngeal cancers by subsite in 2012
Ca-A Cancer Journal for Clinicians, 2017Ahmedin Jemal +2 more
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Sequential deposition as a route to high-performance perovskite-sensitized solar cells
Nature, 2013Peng Gao, Michael Grätzel
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