Authors: Maxim Kramar (University of Hawaii at Manoa), Haosheng Lin (University of Hawaii at Manoa) The coronal magnetic field is important driving force for transientView More
Authors: Gabor Toth (University of Michigan), Nishtha Sachdeva (University of Michigan), Lulu Zhao (University of Michigan), Bart van der Holst (University of Michigan), Igor SokolovView More
Authors: Tom Schad (National Solar Observatory), Alexandra Tritschler (National Solar Observatory), and the DKIST Science Team The chromospheric and coronal polarimetric capabilities of DKIST, inView More
Authors: Joan Burkepile (High Altitude Observatory HAO), Steven Tomczyk (HAO), Ben Berkey (HAO), Marc Cotter (HAO) , Michael Galloy (HAO), Sarah Gibson (HAO), Don KolinskiView More
Authors: Johnathan Stauffer (CU Boulder), Kevin Reardon (NSO) The solar chromosphere is a crucial interface for the overall energy balance of the stellar atmosphere, asView More
Authors: Sajay Gosain, Han Uitenbroek The distribution and evolution of the magnetic field at the solar poles through a solar cycle is an important parameterView More
Authors: Miralles, M. P. (Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA); Cranmer, S. R. (University of Colorado, Boulder, CO) The origin of theView More
Authors: Sarah A. Spitzer (University of Michigan), Susan T. Lepri (University of Michigan), Jim M. Raines (University of Michigan), Frederic Allegrini (Southwest Research Institute), ConnorView More
Authors: Michael Hahn (Columbia University), Xiangrong Fu (New Mexico Consortium), Daniel Wolf Savin (Columbia University) We have found evidence for the parametric decay instability (PDI)View More