Tag: 2024 Session 4. Beyond the Standard Flare Model

Authors: Silvina Guidoni (American University), Rebecca Bonness (American University) During solar eruptions, massive amounts of energy stored in the coronal magnetic field are converted intoView More

Authors: Bin Chen (NJIT), Dale Gary (NJIT), Gelu Nita (NJIT), Sijie Yu (NJIT), Pascal Saint-Hilaire (UC Berkeley), Gregg Hallinan (Caltech), and the EOVSA and OVRO-LWAView More

Authors: J. Lorincik (BAERI/LMSAL), V. Polito (LMSAL; Department of Physics, Oregon State University), G. Kerr (NASA GSFC; Catholic University of America), L. Hayes (ESTEC) TheView More

Authors: Maria D. Kazachenko (University of Colorado Boulder / National Solar Observatory), Yuhong Fan (High Altitude Observatory), Andrei Afanasev (University of Colorado Boulder / NationalView More

Authors: Nian Liu (NJIT), Satoshi Inoue (NJIT), Ju Jing (NJIT, BBSO), Haimin Wang (NJIT, BBSO) We conducted both data-constrained and data-driven magnetohydrodynamic (MHD) simulations ofView More

Authors: Tak Chu Li (Dartmouth College), Yi-Hsin Liu (Dartmouth College), and Yi Qi (University of Colorado Boulder) Electron-only magnetic reconnection was first identified by theView More

Authors: Ryan French (National Solar Observatory), Ritesh Patel (Southwest Research Institute), Maria Kazachenko (University of Colorado Boulder / National Solar Observatory), Joel Dahlin (NASA GSFC),View More

Authors: Drake Osaben (Montana State University), Jiong Qiu, (Montana State University), Dana Longcope (Montana State University) Flare loops are formed by magnetic reconnection, which restructuresView More

Authors: Charles Fred Driscoll (UCSD) A model of “charge-electric” energization of the Solar Wind and Corona is developed, including electro-magnetic particle effects precluded by traditionalView More