The University of California, Berkeley received a $736.8K research grant awarded on October 17, 2022, with a completion date of April 16, 2026, to investigate magnetic flux emergence and the coupling of scales in eruptive solar configurations. The project involves large-scale, high-resolution three-dimensional radiative magnetohydrodynamic simulations combined with observational data analyses to understand how magnetic flux emerges through the Sun's visible surface. The four primary scientific...
This is a $596,818.34 research grant awarded by the National Aeronautics and Space Administration (NASA) to the University of California, Berkeley (UC Berkeley) on April 1, 2017. The grant supports an investigation of momentum processes in solar eruptions by combining multi-instrument observations and numerical modeling. The research aims to address key questions related to the evolution of the photospheric magnetic field and its relation to the Lorentz force during solar eruptions, the...
This is a $191,510.00 grant award from NASA to the University of California, Berkeley (UC Berkeley) for research related to coronal mass ejections (CMEs) and their effects on Earth. The award, with a completion date of May 9, 2024, was made on May 10, 2021 and does not have a set-aside designation. UC Berkeley, a leading public research university, is the prime contractor on this grant. The research aims to provide new information relevant to understanding CMEs and their impact on Earth. UC...
This is a $385,622.42 grant awarded by NASA to the University of California, Berkeley to conduct research on solar flares and coronal mass ejections (CMEs). The research aims to model the development and evolution of coronal magnetic structure using the RADMHD code, with the model photospheric magnetic field vectors matching the observed data from NASA's Solar Dynamics Observatory. The research will compare the simulated emission from the model to observational data from NASA missions such as...
The National Aeronautics and Space Administration (NASA) awarded a $133,316.95 training grant to the Regents of the University of California, doing business as the University of California, Berkeley (UC Berkeley). The grant will fund research to obtain new measurements of the Sun's magnetic field interior to the Earth's orbit, using the time delay of arrival method to trace the trajectories of type III solar radio bursts. The objectives are to evaluate the accuracy of this method, automate the...
The University of California, Berkeley received a $7,486.46 research grant from a civilian federal agency (via the Shared Services Center) awarded on January 1, 2022, with completion expected by December 31, 2024. The grant funds research investigating X-ray bremsstrahlung signatures produced by non-thermal electrons within solar flares in the solar corona. The project employs disk occultation techniques utilizing NuSTAR and Solar Orbiter STIX instrumentation to study non-thermal processes...
This is a $520,337 grant award from the National Aeronautics and Space Administration (NASA) to the University of California, Berkeley to conduct research on solar wind turbulence and dissipation. The award aims to investigate how kinetic-scale fluctuations in the solar wind may contribute to heating and isotropizing the solar wind as it travels towards Earth. This research aligns with NASA's focus on understanding the physics of the Sun and solar system. The award was made directly to the...
This is a $367,127.99 grant awarded by NASA to the University of California, Berkeley (UC Berkeley) to conduct research on the structure and variability of the solar wind. The research aims to investigate how the magnetic geometry of the solar corona influences the heliospheric solar wind. This grant is not associated with a set-aside program. As a parent organization, the State of California Controller's Office would administer any funding provided to UC Berkeley under this grant. UC Berkeley...
This is a $103,999.84 federal training grant awarded by NASA to the University of California, Berkeley (UC Berkeley) for research related to understanding plasma heating in the solar corona and solar wind. The grant supports data analysis of electric field measurements from the THEMIS mission to characterize turbulence signatures, as well as modeling of electrostatic potentials around the Solar Probe Plus (SPP) spacecraft near perihelion. UC Berkeley will also assist in testing the electric...
The National Aeronautics and Space Administration (NASA) awarded a $599,572.13 grant to the Regents of the University of Michigan, Office of Research and Sponsored Projects, to conduct research on the physical processes that lead to large-scale solar eruptions, including flares and coronal mass ejections (CMEs). The research aims to understand how magnetic energy and helicity are transported from the solar convection zone to the corona, the mechanisms that trigger CMEs, the relationship...
This is a $861,330.72 grant from NASA's Living With a Star (LWS) program to the University of California, Berkeley (UC Berkeley) to conduct research on solar eruptive events. The goal is to use data-driven numerical magnetohydrodynamic (MHD) simulations to understand how energized active regions on the Sun trigger coronal mass ejections (CMEs) and other severe space weather disturbances. The research aims to determine the roles of photospheric boundary flows, adjacent magnetic fields, flux cancellation, and flux emergence in the energization and destabilization of active regions that produce large solar flares and CMEs. This work supports the LWS Focused Science Team's effort to understand the onset of major solar eruptions. UC Berkeley, a public research university, is the prime contractor on this grant. The funding is provided by NASA, a civilian federal agency.