Parker solar probe: Four years of discoveries at solar cycle minimum
Abstract Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
Tracking a Beam of Electrons from the Low Solar Corona into Interplanetary Space with the Low Frequency Array, Parker Solar Probe, and 1 au Spacecraft
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams
propagating from the low solar corona into the heliosphere where they can eventually be …
propagating from the low solar corona into the heliosphere where they can eventually be …
Source positions of an interplanetary type III radio burst and anisotropic radio-wave scattering
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 …
energetic electrons propagating in the interplanetary medium. Due to the lack of direct radio …
Comparative Analysis of Type III Radio Bursts and Solar Flares: Spatial Localization and Correlation with Solar Flare Intensity
V Krupar, O Kruparova, A Szabo, F Nemec… - The Astrophysical …, 2024 - iopscience.iop.org
We present a comprehensive study of type III radio bursts and their association with solar
flares of magnitude M1. 0 and larger, as observed by four widely separated spacecraft …
flares of magnitude M1. 0 and larger, as observed by four widely separated spacecraft …
Structured type III radio bursts observed in interplanetary space
Context. The last few decades have seen numerous studies dedicated to fine structures of
type III radio bursts observed in the meter–decameter wavelengths. Most of the explanations …
type III radio bursts observed in the meter–decameter wavelengths. Most of the explanations …
The solar origin of an in situ type III radio burst event
Solar type III radio bursts are generated by beams of energetic electrons that travel along
open magnetic field lines through the corona and into interplanetary space. However …
open magnetic field lines through the corona and into interplanetary space. However …
First observations and performance of the RPW instrument on board the Solar Orbiter mission
M Maksimovic, J Souček, T Chust… - Astronomy & …, 2021 - aanda.org
The Radio and Plasma Waves (RPW) instrument on the ESA Solar Orbiter mission is
designed to measure in situ magnetic and electric fields and waves from the continuum up to …
designed to measure in situ magnetic and electric fields and waves from the continuum up to …
Solar Radio Spikes and Type IIIb Striae Manifestations of Subsecond Electron Acceleration Triggered by a Coronal Mass Ejection
DL Clarkson, EP Kontar, N Vilmer… - The Astrophysical …, 2023 - iopscience.iop.org
Understanding electron acceleration associated with magnetic energy release at subsecond
scales presents major challenges in solar physics. Solar radio spikes observed as …
scales presents major challenges in solar physics. Solar radio spikes observed as …
[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 …
Solar Orbiter/RPW antenna calibration in the radio domain and its application to type III burst observations
Context. In order to allow for a comparison with the measurements from other antenna
systems, the voltage power spectral density measured by the Radio and Plasma waves …
systems, the voltage power spectral density measured by the Radio and Plasma waves …