Results 81 to 90 of about 1,264 (121)
A gas-dynamic calculation of type 2 shock propagation through the corona [PDF]
An approximate analytic theory of acoustic shock propagation in nonuniform media is used to determine the motion of a flare-generated shock wave in the corona.
Kopp, R. A.
core +1 more source
Estimating the Total Energy Content in Escaping Accelerated Solar Electron Beams
Quantifying the energy content of accelerated electron beams during solar eruptive events is a key outstanding objective that must be constrained to refine particle acceleration models and understand the electron component of space weather.
Alexander W. James, Hamish A. S. Reid
doaj +1 more source
During solar cycle minimum, polar coronal holes show a prominent radio brightening cap. The analysis of polar microwave enhanced radiation in polar coronal holes is helpful for understanding the magnetic field characteristics and the origin of the solar ...
Jing Huang +6 more
doaj +1 more source
Large scale structure of the corona [PDF]
This is an introduction to this section of the proceedings. In this section is a brief description of some radio results obtained with meter-decameter radioheliograph.
Kundu, M. R.
core +1 more source
Giant Postflare Loops in Active Regions with an Extremely Strong Coronal Magnetic Field
We report for the first time the detection of thermal free–free emission from post-flare loops at 34 GHz in images from the Nobeyama Radioheliograph. We studied eight loops, seven of which were from regions with an extremely strong coronal magnetic field
Costas E. Alissandrakis +4 more
doaj +1 more source
Subsecond Spikes in Fermi GBM X-Ray Flux as a Probe for Solar Flare Particle Acceleration. [PDF]
Knuth T, Glesener L.
europepmc +1 more source
Long-term Solar Activity Studies using Microwave Imaging Observations and Prediction for Cycle 25. [PDF]
Gopalswamy N +3 more
europepmc +1 more source
An 8-cm radioheliograph which has been under construction since 1972 is almost completed. It has a maximum resolving power of 1.5 .arc min. and can be operated in various operational modes combined with the existing high-resolution compound interferometer. The minimum time necessary for taking a map is 40 seconds. A two-dimensional mapping will be used
openaire
Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona. [PDF]
Carley EP +6 more
europepmc +1 more source
On-Disc Observations of Flux Rope Formation Prior to Its Eruption. [PDF]
James AW +8 more
europepmc +1 more source

