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Spectral Characteristics of Fundamental–Harmonic Pairs of Interplanetary Type III Radio Bursts Observed

4 months ago astro.gla.ac.uk astronomy

Magnetic Field Geometry and Anisotropic Scattering Effects to Explain Puzzling LOFAR Solar Radio Burst Observations

4 months ago astro.gla.ac.uk astronomy

Temporally resolved Type III solar radio bursts in the frequency range 3-13 MHz

6 months ago astro.gla.ac.uk astronomy

Radio wave scattering observations suggest that the energy deposition rates due to ion-sound wave damping are comparable to the rates available from a turbulent cascade of Alfvénic waves at large scales; suggesting a coherent picture of energy transfer and coronal heating.

11 months ago astro.gla.ac.uk astronomy

Solar electron beam velocities that grow Langmuir waves in the inner heliosphere

22 months ago astro.gla.ac.uk astronomy

Imaging preflare broadband pulsations in the decimetric-metric wavelengths

24 months ago astro.gla.ac.uk astronomy

Electron acceleration efficiency during the impulsive phase of a solar flare: X-ray and microwave observations

24 months ago astro.gla.ac.uk astronomy

Solar Radio Spikes and Type IIIb Striae Manifestations Triggered by a Coronal Mass Ejection

2 years ago astro.gla.ac.uk astronomy

Automated Detection and Statistical Study of Solar Radio Spikes

2 years ago astro.gla.ac.uk astronomy

The Radial Variation of the Solar Wind Turbulence Spectra near the Kinetic Break Scale from Parker Solar Probe Measurements

2 years ago astro.gla.ac.uk astronomy

The First Flare Observation with a New Solar Microwave Spectrometer Working in 35–40 GHz

2 years ago astro.gla.ac.uk astronomy

Langmuir wave motion observed in the most intense radio sources in the sky

3 years ago astro.gla.ac.uk

First imaging spectroscopy observations of puzzling solar drift pair bursts

5 years ago astro.gla.ac.uk

Fragmented radio emission reveals a shock passing through solar active region loops by Silja Pohjolainen, Jens Pomoell and Rami Vainio

8 years ago astro.gla.ac.uk

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Spectral Characteristics of Fundamental–Harmonic Pairs of Interplanetary Type III Radio Bursts Observed

Magnetic Field Geometry and Anisotropic Scattering Effects to Explain Puzzling LOFAR Solar Radio Burst Observations

Temporally resolved Type III solar radio bursts in the frequency range 3-13 MHz

Radio wave scattering observations suggest that the energy deposition rates due to ion-sound wave damping are comparable to the rates available from a turbulent cascade of Alfvénic waves at large scales; suggesting a coherent picture of energy transfer and coronal heating.

Solar electron beam velocities that grow Langmuir waves in the inner heliosphere

Imaging preflare broadband pulsations in the decimetric-metric wavelengths

Electron acceleration efficiency during the impulsive phase of a solar flare: X-ray and microwave observations

Solar Radio Spikes and Type IIIb Striae Manifestations Triggered by a Coronal Mass Ejection

Automated Detection and Statistical Study of Solar Radio Spikes

The Radial Variation of the Solar Wind Turbulence Spectra near the Kinetic Break Scale from Parker Solar Probe Measurements

The First Flare Observation with a New Solar Microwave Spectrometer Working in 35–40 GHz

Langmuir wave motion observed in the most intense radio sources in the sky

First imaging spectroscopy observations of puzzling solar drift pair bursts

Fragmented radio emission reveals a shock passing through solar active region loops by Silja Pohjolainen, Jens Pomoell and Rami Vainio

All the news that's fit to scrape

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