[HTML][HTML] New Insights from Imaging Spectroscopy of Solar Radio Emission
DE Gary - Annual Review of Astronomy and Astrophysics, 2023 - annualreviews.org
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 …
frequencies and times provides new physical insight into the processes, structure, and …
Magnetic diagnostics of the solar corona: synthesizing optical and radio techniques
In this contribution we review the current state-of-the-art of coronal magnetometry, in both
optical and radio domains. We address the achievable objectives and the challenges of …
optical and radio domains. We address the achievable objectives and the challenges of …
[HTML][HTML] Tight asteroseismic constraints on core overshooting and diffusive mixing in the slowly rotating pulsating B8. 3V star KIC 10526294
Context. KIC 10526294 was recently discovered to be a very slowly rotating and slowly
pulsating late B-type star. Its 19 consecutive dipole gravity modes constitute a series with …
pulsating late B-type star. Its 19 consecutive dipole gravity modes constitute a series with …
[HTML][HTML] Imaging spectroscopy of solar radio burst fine structures
Solar radio observations provide a unique diagnostic of the outer solar atmosphere.
However, the inhomogeneous turbulent corona strongly affects the propagation of the …
However, the inhomogeneous turbulent corona strongly affects the propagation of the …
Multiple regions of shock-accelerated particles during a solar coronal mass ejection
The Sun is an active star that can launch large eruptions of magnetized plasma into the
heliosphere, known as coronal mass ejections (CMEs). These can drive shocks that …
heliosphere, known as coronal mass ejections (CMEs). These can drive shocks that …
The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT
A Konovalenko, L Sodin, V Zakharenko, P Zarka… - Experimental …, 2016 - Springer
The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio
telescope) together with its VLBI system called URAN is described in detail. By …
telescope) together with its VLBI system called URAN is described in detail. By …
Science with the Murchison Widefield Array: Phase i results and Phase II opportunities
The Murchison Widefield Array (MWA) is an open access telescope dedicated to studying
the low-frequency (80–300 MHz) southern sky. Since beginning operations in mid-2013, the …
the low-frequency (80–300 MHz) southern sky. Since beginning operations in mid-2013, the …
[HTML][HTML] Spatially resolved radio signatures of electron beams in a coronal shock
Context. Type II radio bursts are a type of solar radio bursts associated with coronal shocks.
Type II bursts usually exhibit fine structures in dynamic spectra that represent signatures of …
Type II bursts usually exhibit fine structures in dynamic spectra that represent signatures of …
Magnetic reconnection null points as the origin of semirelativistic electron beams in a solar jet
Magnetic reconnection, the central engine that powers explosive phenomena throughout the
universe, is also perceived to be one of the principal mechanisms for accelerating particles …
universe, is also perceived to be one of the principal mechanisms for accelerating particles …
[HTML][HTML] A review of recent solar type III imaging spectroscopy
HAS Reid - Frontiers in Astronomy and Space Sciences, 2020 - frontiersin.org
Solar type III radio bursts are the most common impulsive radio signatures from the Sun,
stimulated by electron beams traveling through the solar corona and solar wind. Type III …
stimulated by electron beams traveling through the solar corona and solar wind. Type III …