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Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case Studies
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Assessing student engagement with teamwork in an online, large-enrollment course-based undergraduate research experience in physics
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The Fractality and Size Distributions of Astrophysical Self-Organized Criticality Systems
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Variable X-Ray Emission of Comet 46P/Wirtanen
Emanuele Bonamente, Damian J. Christian, Zexi 泽曦 Xing 邢, Kumar Venkataramani, Dimitra Koutroumpa and Dennis Bodewits The Planetary Science Journal 2(6) 224 (2021) https://doi.org/10.3847/PSJ/ac2aac
Statistical analysis of soft X-ray solar flares during solar cycles 22, 23, and 24
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Statistical Properties of Superflares on Solar-type Stars: Results Using All of the Kepler Primary Mission Data
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The High-energy Radiation Environment around a 10 Gyr M Dwarf: Habitable at Last?
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An Observational Test of Solar Plasma Heating by Magnetic Flux Cancellation
When “Boring” Stars Flare: The Ultraviolet Activity of GJ 887, a Bright M Star Hosting Newly Discovered Planets*
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What Determines Solar Flares Producing Interplanetary Type III Radio Bursts?
Y. K. Kou, Z. C. Jing, X. Cheng, W. Q. Pan, Y. Liu, C. Li and M. D. Ding The Astrophysical Journal Letters 898(1) L24 (2020) https://doi.org/10.3847/2041-8213/aba362
Statistical Study of Hard X-Ray Emitting Electrons Associated with Flare-related Coronal Jets
Lyman‐alpha Variability During Solar Flares Over Solar Cycle 24 Using GOES‐15/EUVS‐E
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Bivariate Number Distribution of Solar Soft X-Ray Flares
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Magnetic field strengths of hot Jupiters from signals of star–planet interactions
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The Mars Topside Ionosphere Response to the X8.2 Solar Flare of 10 September 2017
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