Results 11 to 20 of about 1,884,795 (348)
Classification of Solar Radio Spectrum Based on Swin Transformer [PDF]
Solar radio observation is a method used to study the Sun. It is very important for space weather early warning and solar physics research to automatically classify solar radio spectrums in real time and judge whether there is a solar radio burst. As the
Jian Chen +5 more
doaj +2 more sources
Auto Recognition of Solar Radio Bursts Using the C-DCGAN Method
Solar radio bursts can be used to study the properties of solar activities and the underlying coronal conditions on the basis of the present understanding of their emission mechanisms. With the construction of observational instruments, around the world,
Weidan Zhang +7 more
doaj +2 more sources
Incoherent Solar Radio Emission [PDF]
Incoherent solar radio radiation comes from the free-free, gyroresonance, and gyrosynchrotron emission mechanisms. Free-free is primarily produced from Coulomb collisions between thermal electrons and ions. Gyroresonance and gyrosynchrotron result from the acceleration of low-energy electrons and mildly relativistic electrons, respectively, in the ...
A. Nindos
openaire +5 more sources
LSTM neural network for solar radio spectrum classification [PDF]
A solar radio spectrometer records solar radio radiation in the radio waveband. Such solar radio radiation spanning multiple frequency channels and over a short time period could provide a solar radio spectrum which is a two dimensional image.
Long Xu +5 more
openalex +2 more sources
Performance assessment of GPS receivers during the September 24, 2011 solar radio burst event
The sudden outburst of in-band solar radio noise from the Sun is recognized as one of the potential Radio Frequency Interference (RFI) sources that directly impact the performance of Global Navigation Satellite System (GNSS) receivers.
Muhammad Bilal +4 more
doaj +2 more sources
Imaging spectroscopy of solar radio burst fine structures. [PDF]
Solar radio observations provide a unique diagnostic of the outer solar atmosphere. However, the inhomogeneous turbulent corona strongly affects the propagation of the emitted radio waves, so decoupling the intrinsic properties of the emitting source ...
Kontar EP +8 more
europepmc +3 more sources
Low Altitude Solar Magnetic Reconnection, Type III Solar Radio Bursts, and X-ray Emissions. [PDF]
Type III solar radio bursts are the Sun’s most intense and frequent nonthermal radio emissions. They involve two critical problems in astrophysics, plasma physics, and space physics: how collective processes produce nonthermal radiation and how magnetic ...
Cairns IH +41 more
europepmc +2 more sources
Exploring the Circular Polarisation of Low–Frequency Solar Radio Bursts with LOFAR [PDF]
The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio wavelengths. Low frequency radio bursts have recently been brought back to light with the advancement of novel radio interferometers.
D. Morosan +11 more
semanticscholar +1 more source
New Insights from Imaging Spectroscopy of Solar Radio Emission
Newly available high-resolution imaging of solar radio emission at many closely spaced frequencies and times provides new physical insight into the processes, structure, and dynamics of the solar atmosphere.
D. Gary
semanticscholar +1 more source
A Broadband Solar Radio Dynamic Spectrometer Working in the Millimeter-wave Band
Most solar radio telescopes operate below ∼18 GHz and cannot realize a complete frequency coverage of the microwave spectrum, especially in the optically thin regime during solar bursts, which can provide unique information about the magnetic field in ...
Ziqian Shang +9 more
semanticscholar +1 more source

