Results 81 to 90 of about 438 (164)
Refraction and scattering of radio emission from a solar source due to coronal inhomogeneities [PDF]
Alexander N. Afanasiev, A. T. Altyntsev
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Measuring the Magnetic Field of a Coronal Mass Ejection from the Low to Middle Corona
A major challenge in understanding the initiation and evolution of coronal mass ejections (CMEs) is measuring the magnetic field of the magnetic flux ropes (MFRs) that drive CMEs.
Xingyao Chen +46 more
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Highly Polarized Type III Storm Observed with Parker Solar Probe
The Parker Solar Probe (PSP) spacecraft observed a large coronal mass ejection (CME) on 2022 September 5, shortly before closest approach during the 13th PSP solar encounter.
Marc Pulupa +4 more
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Polarimetric radio observations of the Sun can provide rich information about emission mechanisms and the propagation medium. For the past five decades, solar polarimetric studies at low radio frequencies have almost always assumed the absence of linear ...
Soham Dey +3 more
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The solar corona is much hotter than the photosphere and chromosphere, but the physical mechanism responsible for heating the coronal plasma remains unidentified. The thermal microwave emission, which is produced in a strong magnetic field above sunspots,
Alexey A. Kuznetsov +3 more
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We traced the origin of very-long-periodic pulsations (VLPs) in type-I burst chains on 2024 February 14. Seven successive and repetitive pulsation structures appeared in radio dynamic spectra in the metric waveband, which were simultaneously measured by ...
Dong Li +7 more
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Low-frequency radio emission in the form of type II and III bursts is a direct indicator of plasma motion in the solar corona and interplanetary medium.
Ivey Davis +48 more
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Angular scattering of solar radio emission by coronal turbulence
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Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]
Martinez Oliveros JC +8 more
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