Results 151 to 160 of about 2,802,659 (186)
Outstanding Questions and Future Research on Magnetic Reconnection. [PDF]
Nakamura R +24 more
europepmc +1 more source
Psyche Mission Description and Design Rationale. [PDF]
Polanskey CA +29 more
europepmc +1 more source
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Probing the transient and time-variable sky. [PDF]
Orlowski-Scherer J +27 more
europepmc +1 more source
Different Behavior of Density Perturbations Between Dayside and Nightside in the Martian Thermosphere and the Ionosphere Associated With Atmospheric Gravity Waves. [PDF]
Nakagawa H +8 more
europepmc +1 more source
Observations of the Coronal Dynamics Associated With Solar Radio Spike Burst Emission [PDF]
We present the results of an analysis of multi-wavelength data for a solar radio spike burst event which was observed on 1997 November 14 by the Solar Radio Spectrometers of the Astrophysikalisches Institut Potsdam (AIP).
H Aurass, J I Khan
exaly +3 more sources
The Connection of Solar Wind Parameters With Radio and UV Emission From Coronal Holes [PDF]
This paper presents the results of a comparison between observations of coronal holes in UV (SOHO EIT) and radio emission (17, 5.7 GHz, 327 and 150.9 MHz, from NoRH, SSRT and Nancay radioheliographs), and solar wind parameters, from ACE spacecraft data over the period 12 March – 31 May 2007.
I N Myagkova
exaly +4 more sources
A Model for Radio Emission From Solar Coronal Shocks [PDF]
Solar coronal shocks are very common phenomena in the solar atmosphere and are believed to be the drivers of solar type II radio bursts. However, the microphysical nature of these emissions is still an open problem. This paper proposes that electron cyclotron maser (ECM) emission is responsible for the generation of radiations from the coronal shocks ...
Ling Chen, G Q Zhao, D J Wu
exaly +3 more sources
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Solar Radio Emission as a Prediction Technique for Coronal Mass Ejections’ Detection
Proceedings of the International Astronomical Union, 2017AbstractIn this report we present a possible scheme of short-term CME detection forecasting developed on the basis of statistical analysis of solar radio emission regularities prior to “isolated” solar Coronal Mass Ejections registered in 1998, 2003, 2009-2013.
Olga A Sheiner
exaly +2 more sources
Type II solar radio bursts are the primary radio emissions generated by shocks and they are linked with impending space weather events at Earth. We simulate type II bursts by combining elaborate three-dimensional MHD simulations of realistic coronal mass ejections (CMEs) at the Sun with an analytic kinetic radiation theory developed recently.
Iver H. Cairns, Joachim M. Schmidt
exaly +2 more sources

