Results 151 to 160 of about 2,802,659 (186)

Outstanding Questions and Future Research on Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev
Nakamura R   +24 more
europepmc   +1 more source

Psyche Mission Description and Design Rationale. [PDF]

open access: yesSpace Sci Rev
Polanskey CA   +29 more
europepmc   +1 more source

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Probing the transient and time-variable sky. [PDF]

open access: yesOpen Res Eur
Orlowski-Scherer J   +27 more
europepmc   +1 more source

Observations of the Coronal Dynamics Associated With Solar Radio Spike Burst Emission [PDF]

open access: yesAstronomy and Astrophysics, 2006
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]

open access: yesSolar Physics, 2011
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]

open access: yesAstrophysical Journal, 2014
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

Solar Radio Emission as a Prediction Technique for Coronal Mass Ejections’ Detection

Proceedings of the International Astronomical Union, 2017
AbstractIn 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

Prediction of Type II Solar Radio Bursts by Three-Dimensional MHD Coronal Mass Ejection and Kinetic Radio Emission Simulations

open access: yesAstrophysical Journal Letters, 2013
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

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