Imaging spectroscopy of type U and J solar radio bursts with LOFAR
Context. Radio U-bursts and J-bursts are signatures of electron beams propagating along
magnetic loops confined to the corona. The more commonly observed type III radio bursts …
magnetic loops confined to the corona. The more commonly observed type III radio bursts …
Solar Type J Radio Bursts and the Associated Coronal Loop
SW Feng, HX Xie, H Misawa - The Astrophysical Journal, 2024 - iopscience.iop.org
The solar type J radio burst is a variant of type III bursts, which are a probe for understanding
solar energetic electrons and local electron density. This study investigates a type J burst …
solar energetic electrons and local electron density. This study investigates a type J burst …
Imaging a large coronal loop using type U solar radio burst interferometry
J Zhang, HAS Reid, E Carley, L Lamy… - The Astrophysical …, 2024 - iopscience.iop.org
Solar radio U-bursts are generated by electron beams traveling along closed magnetic
loops in the solar corona. Low-frequency (< 100 MHz) U-bursts serve as powerful diagnostic …
loops in the solar corona. Low-frequency (< 100 MHz) U-bursts serve as powerful diagnostic …
Decameter U-burst harmonic pair from a high loop
The results of the first observations of solar sporadic radio emission within 10–70 MHz by
the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in …
the Giant Ukrainian Radio Telescope (GURT) are presented and discussed. Observations in …
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 …
between the solar wind and the low solar corona. However, their plasma properties are ill …
Observation of a metric type N solar radio burst
Type III and type-III-like radio bursts are produced by energetic electron beams guided along
coronal magnetic fields. As a variant of type III bursts, Type N bursts appear as the letter" N" …
coronal magnetic fields. As a variant of type III bursts, Type N bursts appear as the letter" N" …
The frequency ratio and time delay of solar radio emissions with fundamental and harmonic components
Solar radio bursts generated through the plasma emission mechanism produce radiation
near the local plasma frequency (fundamental emission) and double the plasma frequency …
near the local plasma frequency (fundamental emission) and double the plasma frequency …
Narrowband frequency-drift structures in solar type IV bursts
Y Nishimura, T Ono, F Tsuchiya, H Misawa… - Earth, Planets and …, 2013 - Springer
We have established the Zao Solar Radiospectrograph (ZSR), a new solar radio observation
system, at the Zao observatory of Tohoku University, Japan. We observed narrowband fine …
system, at the Zao observatory of Tohoku University, Japan. We observed narrowband fine …
[PDF][PDF] Imaging Spectroscopy of Type U and J Solar Radio Bursts with
Context. Radio U-bursts and J-bursts are signatures of electron beams propagating along
magnetic loops confined to the corona. The more commonly observed type III radio bursts …
magnetic loops confined to the corona. The more commonly observed type III radio bursts …