Fundamental–Harmonic Pairs of Interplanetary Type III Radio Bursts
Type III radio bursts are not only the most intense but also the most frequently observed
solar radio bursts. However, a number of their defining features remain poorly understood …
solar radio bursts. However, a number of their defining features remain poorly understood …
The existence of hot X-ray onsets in solar flares
Context. It is well known among the scientific community that solar flare activity often begins
well before the main impulsive energy release. However, a consistent explanation for this …
well before the main impulsive energy release. However, a consistent explanation for this …
Connecting remote and in situ observations of shock-accelerated electrons associated with a coronal mass ejection
Context. One of the most prominent sources for energetic particles in our Solar System are
huge eruptions of magnetised plasma from the Sun, known as coronal mass ejections …
huge eruptions of magnetised plasma from the Sun, known as coronal mass ejections …
Relativistic electron beams accelerated by an interplanetary shock
Context. Collisionless shock waves have long been considered to be among the most
prolific particle accelerators in the universe. Shocks alter the plasma they propagate …
prolific particle accelerators in the universe. Shocks alter the plasma they propagate …
Very Large and Long-lasting Anisotropies Caused by Sunward Streaming Energetic Ions: Solar Orbiter and STEREO A Observations
The anisotropy of energetic particles provides essential information to help resolve the
underlying fundamental physics of their spatial distributions, injection, acceleration, and …
underlying fundamental physics of their spatial distributions, injection, acceleration, and …
An Overview of Solar Orbiter Observations of Interplanetary Shocks in Solar Cycle 25
Interplanetary shocks are fundamental constituents of the heliosphere, where they form as a
result of solar activity. We use previously unavailable measurements of interplanetary …
result of solar activity. We use previously unavailable measurements of interplanetary …
[HTML][HTML] Observation of solar radio burst events from Mars orbit with the Shallow Radar instrument
Context. Multispacecraft and multiwavelength observations of solar eruptions, such as flares
and coronal mass ejections, are essential to understanding the complex processes behind …
and coronal mass ejections, are essential to understanding the complex processes behind …
Juno Observations of Langmuir Waves in Association with Interplanetary Shocks from~ 1.3 to~ 5.4 au
Langmuir waves are often observed upstream of planetary bow shocks and interplanetary
(IP) shocks. Waveform capture (WFC) measurements, obtained during Juno's cruise phase …
(IP) shocks. Waveform capture (WFC) measurements, obtained during Juno's cruise phase …
Determining the acceleration regions of in situ electrons using remote radio and X-ray observations
Context. Solar energetic particles in the heliosphere are produced by flaring processes on
the Sun or by shocks driven by coronal mass ejections. These particles are regularly …
the Sun or by shocks driven by coronal mass ejections. These particles are regularly …
Delay of Near-relativistic Electrons with Respect to Type III Radio Bursts throughout the Inner Heliosphere
JG Mitchell, ER Christian, GA de Nolfo… - The Astrophysical …, 2025 - iopscience.iop.org
Energetic electrons accelerated by solar eruptive events are frequently observed to have
inferred injection times that appear significantly delayed with respect to electromagnetic …
inferred injection times that appear significantly delayed with respect to electromagnetic …