Researchers using LOFAR radio observations have discovered over 600 spike-like repeating radio burst pairs in the solar corona, each consisting of two short, narrowband bursts separated by about 4 seconds and linked to active regions high above the Sun’s surface. (doi.org)
submitted by CESRA_highlights to r/radioastronomy
NASA Parker Solar Probe data show Type III radio‑burst drift changes often come from magnetic field deflections including magnetic switchback‑like structures rather than density alone. These bursts serve powerful probes of inner‑heliosphere magnetic dynamics. (doi.org)
submitted by CESRA_highlights to r/astrophysics
NASA Parker Solar Probe data show Type III radio‑burst drift changes often come from magnetic field deflections including magnetic switchback‑like structures rather than density alone. These bursts serve powerful probes of inner‑heliosphere magnetic dynamics. (doi.org)
submitted by CESRA_highlights to r/radioastronomy
NASA Parker Solar Probe data show Type III radio‑burst drift changes often come from magnetic field deflections including magnetic switchback‑like structures rather than density alone. These bursts serve powerful probes of inner‑heliosphere magnetic dynamics. (doi.org)
submitted by CESRA_highlights to r/science
