The observed properties (ie, source size, source position, time duration, and decay time) of
solar radio emission produced through plasma processes near the local plasma frequency …

The concept of the Solar Ring mission was gradually formed from L5/L4 mission concept,
and the proposal of its pre-phase study was funded by the National Natural Science …

Context. A complex and long-lasting solar eruption on 17 April 2021 produced a widespread
solar energetic particle (SEP) event that was observed by five longitudinally well-separated …

Radio waves are strongly scattered in the solar wind, so that their apparent sources seem to
be considerably larger and shifted than the actual ones. Since the scattering depends on the …

The Radio Frequency Spectrometer (RFS) is a two‐channel digital receiver and
spectrometer, which will make remote sensing observations of radio waves and in situ …

Radio frequency electromagnetic noise (RF) of anthropogenic origin has been shown to
disrupt magnetic orientation behavior in some animals. Two sources of natural RF might …

We present initial results from the Radio Frequency Spectrometer, the high-frequency
component of the FIELDS experiment on the Parker Solar Probe (PSP). During the first PSP …

Context. Coronal mass ejections (CMEs) are eruptive phenomena that can accelerate
energetic particles and drive shock waves. The CME-driven shocks propagate from the low …

Context. We study the solar energetic particle (SEP) event observed on 9 October 2021 by
multiple spacecraft, including Solar Orbiter. The event was associated with an M1. 6 flare, a …

Interplanetary solar radio type III bursts provide the means to remotely study and track
energetic electrons propagating in the interplanetary medium. Due to the lack of direct radio …