A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä

Fundamental-Harmonic Pairs of Interplanetary Type III Radio Bursts




TekijätJebaraj Immanuel Christopher, Krasnoselskikh Vladimir, Pulupa Marc, Magdalenic Jasmina, Bale Stuart D

KustantajaIOP Publishing Ltd

Julkaisuvuosi2023

JournalAstrophysical Journal Letters

Tietokannassa oleva lehden nimiASTROPHYSICAL JOURNAL LETTERS

Lehden akronyymiASTROPHYS J LETT

Artikkelin numero L20

Vuosikerta955

Numero1

Sivujen määrä11

ISSN2041-8205

DOIhttps://doi.org/10.3847/2041-8213/acf857

Verkko-osoitehttps://iopscience.iop.org/article/10.3847/2041-8213/acf857

Rinnakkaistallenteen osoitehttps://research.utu.fi/converis/portal/detail/Publication/181421789


Tiivistelmä
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. Observational limitations, such as a lack of sufficient spectral and temporal resolution, have hindered a full comprehension of the emission process, especially in the hectokilometric wavelengths. Of particular difficulty is the ability to detect the harmonics of type III radio bursts. Here we report the first detailed observations of type III fundamental-harmonic pairs in the hectokilometric wavelengths, observed by the Parker Solar Probe. We present a statistical analysis of the spectral characteristics and polarization measurements of the fundamental-harmonic pairs. Additionally, we quantify various characteristics of the fundamental-harmonic pairs, such as the time delay and time profile asymmetry. Our report concludes that fundamental-harmonic pairs constitute a majority of all type III radio bursts observed during close encounters when the probe is in close proximity to the source region and propagation effects are less pronounced.

Ladattava julkaisu

This is an electronic reprint of the original article.
This reprint may differ from the original in pagination and typographic detail. Please cite the original version.





Last updated on 2024-26-11 at 20:36