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Found 2 entries in the Bibliography.
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2023 |
Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations Large coronal loops around one solar radius in altitude are an important connection between the solar wind and the low solar corona. However, their plasma properties are ill-defined, as standard X-ray and UV techniques are not suited to these low-density environments. Diagnostics from type J solar radio bursts at frequencies above 10 MHz are ideally suited to understand these coronal loops. Despite this, J-bursts are less frequently studied than their type III cousins, in part because the curvature of the coronal loop makes ... Zhang, Jinge; Reid, Hamish; Krupar, Vratislav; Zucca, Pietro; Dabrowski, Bartosz; Krankowski, Andrzej; Published by: \solphys Published on: jan YEAR: 2023   DOI: 10.1007/s11207-022-02096-0 Parker Data Used; Energetic particles; Electrons; magnetic fields; Corona; Radio emission; Radio bursts; Astrophysics - Solar and Stellar Astrophysics |
Solar Electron Beam Velocities That Grow Langmuir Waves in the Inner Heliosphere Solar accelerated electron beams, a component of space weather, are emitted by eruptive events at the Sun. They interact with the ambient plasma to grow Langmuir waves, which subsequently produce radio emission, changing the electrons motion through space. Solar electron beam-plasma interactions are simulated using a quasilinear approach to kinetic theory to probe the variations in the maximum electron velocity [\ensuremath\Xi ] responsible for Langmuir wave growth between the Sun s surface and 50 R$_\ensuremath\odot$ above ... Lorfing, Camille; Reid, Hamish; Published by: \solphys Published on: apr YEAR: 2023   DOI: 10.1007/s11207-023-02145-2 Electrons; particle emission; Radio radiation; Langmuir waves; space weather |
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