Stuart Bale

Research Expertise and Interest

experimental space physics, plasma astrophysics, solar physics, low frequency radio astronomy

Research Description

Stuart Bale is interested in plasma astrophysics from the experimental point of view. Much of the universe is in the plasma state and we are just coming to appreciate the role of plasma dynamics and magnetic fields in the large-scale evolution of astrophysical systems. However, many of the fundamental processes are poorly understood and can only be studied in a limited parameter regime in the laboratory. Examples are magnetic reconnection, collisionless shocks, and solar/stellar wind generation and evolution.

His research is focused on developing experiments to understand these processes and, in particular, how microscale, kinetic phenomena, affect large-scale plasma evolution.

He is also interested in low frequency (LF) radio astronomy, at frequencies below the ionospheric cutoff (~12 MHz); these observations need to be made from space. Signatures of solar flare electrons and CMEs dominate the dynamics at these frequencies, however the large-scale structure of the radio sky below 15 MHz remains mostly unexplored. This structure maps the galactic magnetic field and cosmic ray electrons and may hold information from the recombination epoch.

His research group at the Space Sciences Laboratory develops, builds, and operates space-borne experiments to study in situ the plasma processes active in astrophysical, heliospheric, and magnetospheric systems. These experiments are flown on NASA and ESA spacecraft missions and are often developed as balloon and sounding rocket payloads.

In the News

Parker Solar Probe Touches the Sun — a First for Any Spacecraft

or the first time in history, a spacecraft has touched the sun. NASA’s Parker Solar Probe, which carries instruments built at UC Berkeley, flew through the sun’s upper atmosphere — the corona — for a few hours on April 28, 2021, sampling particles and magnetic fields for the first time from one of the hottest places in the solar system.

Parker probe traces solar wind to its source on sun’s surface

A year ago, NASA’s Parker Solar Probe flew closer to the sun than any satellite in history, collecting a spectacular trove of data from the very edge of the sun’s million-degree corona. Now, that data has allowed solar physicists to map the source of a major component of the solar wind that continually peppers Earth’s atmosphere, while revealing strange magnetic field reversals that could be accelerating these particles toward our planet.

Fierce solar magnetic storm barely missed Earth in 2012

According to University of California, Berkeley, and Chinese researchers, a rapid succession of coronal mass ejections — the most intense eruptions on the sun — sent a pulse of magnetized plasma barreling into space and through Earth’s orbit.

Scrutinizing Space Storms for a Calmer Life on Earth

Thomas Immel and his team at the Space Sciences Lab will design, build and operate two instruments and oversee development of two others to be loaded on a solar-powered satellite for a two-year science mission tentatively set to launch in 2017.

NASA Selects Investigations for First Mission to Encounter the Sun

NASA has chosen a UC Berkeley experiment and three others to fly aboard Solar Probe Plus, a satellite scheduled for launch in 2018 to explore the sun's million-degree atmosphere. Physicist Stuart Bale, director of the Space Sciences Lab, will lead development of instruments to detect radio emissions, magnetic fields, shock waves and dust as the spacecraft plunges into the sun.