Combined Radio and Space-based Solar Observations: From Techniques to New Results
arXiv:1806.05919 · doi:10.1007/s11207-018-1309-2
Abstract
The phenomena observed at the Sun have a variety of unique radio signatures that can be used to diagnose the processes in the solar atmosphere. The insights provided by radio obervations are further enhanced when they are combined with observations from space-based telescopes. This special issue demonstrates the power of combination methodology at work and provides new results on i) type I solar radio bursts and thermal emission to study active regions; ii) type II and IV bursts to better understand the structure of coronal mass ejections; iii)~non-thermal gyro-synchrotron and/or type III bursts to improve characterization of particle acceleration in solar flares. The ongoing improvements in time, frequency, and spatial resolutions of ground-based telescopes reveal new levels of solar phenomena complexity and pose new questions.
References in corpus (10)
- Imaging Spectroscopy of Solar Radio Burst Fine Structures
- Strength of the Solar Coronal Magnetic field - A Comparison of Independent Estimates Using Contemporaneous Radio and White-light Observations
- 4D Data Cubes from Radio-Interferometric Spectroscopic Snapshot Imaging
- The Wind/EPACT proton event catalog (1996-2016)
- A Statistical Analysis of the Solar Phenomena Associated with Global EUV Waves
- Solar prominence modelling and plasma diagnostics at ALMA wavelengths
- Flare SOL2012-07-06: on the origin of the circular polarization reversal between 17 GHz and 34 GHz
- Solar plasma radio emission in the presence of imbalanced turbulence of kinetic-scale Alfvén waves
- Decameter Type IV Burst Associated with a behind-the-limb CME Observed on 7 November 2013
- Observations of a Radio-quiet Solar Preflare