Results 61 to 70 of about 295,213 (157)
AN EXTENSION OF THE CHAPMAN-FERRARO THEORY OF GEOMAGNETIC STORMS [PDF]
Extension of chapman-ferraro theory of geomagnetic ...
Kern, J. W., Vestine, E. H.
core +1 more source
Effects of electrojet turbulence on a magnetosphere‐ionosphere simulation of a geomagnetic storm
, 2017 Ionospheric conductance plays an important role in regulating the response of the magnetosphere‐ionosphere system to solar wind driving. Typically, models of magnetosphere‐ionosphere coupling include changes to ionospheric conductance driven by extreme ...
M. Wiltberger +10 more
semanticscholar +1 more source
Brain Emotional Learning-based Prediction Model For the Prediction of Geomagnetic Storms [PDF]
arXiv, 2020 This study suggests a new data-driven model for the prediction of geomagnetic storm. The model which is an instance of Brain Emotional Learning Inspired Models (BELIMs), is known as the Brain Emotional Learning-based Prediction Model (BELPM). BELPM consists of four main subsystems; the connection between these subsystems has been mimicked by the ...
arxiv
, 2007 International audienceUsing 8-year global ionosphere maps (GIMs) of TEC products from the Jet Propulsion Laboratory (JPL), we make a statistical study on the morphology of the global ionospheric behaviors with respect to the geomagnetic disturbances ...
Biqiang, Zhao +3 more
core +2 more sources
A Study of the Morphology of Magnetic Storms Great Magnetic Storms [PDF]
, 1958 Average characteristics are determined for 74 great magnetic storms with sudden commencements that occurred in 1902-1945. The storm field is resolved for different epochs of storm time into tv;o parts: (i) Dst, which is independent of local time, that
Chapman, Sydney, Sugiura, Masahisa
core
Ionosphere-thermosphere global time response to geomagnetic storms [PDF]
arXiv, 2017 In this study, we investigate thermospheric neutral mass density heating associated with 168 CME-driven geomagnetic storms in the period of May 2001 to September 2011. We use neutral density measured by two low-Earth orbit satellites: CHAMP and GRACE.
arxiv
The structure of the solar plasma flow generated by solar flares [PDF]
Geomagnetic storm characteristics for two-dimensional configuration of solar plasma flow generated by solar ...
Akasofu, S.-I., Yoshida, S.
core +1 more source
SAMI3‐RCM simulation of the 17 March 2015 geomagnetic storm
, 2017 We present a self‐consistent modeling study of the ionosphere‐plasmasphere system response to the 17 March 2015 geomagnetic storm using the coupled SAMI3‐RCM code. The novel feature of this work is that we capture the important storm time dynamics of the
J. Huba, S. Sazykin, A. Coster
semanticscholar +1 more source
Wavelet analysis of the ionospheric response at mid-latitudes during the April 200 storm using magnetograms and vTEC from GPS [PDF]
, 2013 In this work we pursue the idea of computing a parameter that allows us to estimate the local ionospheric response to a geospheric event that triggers an ionospheric storm. For that, wavelet technique has been chosen because of its ability to analyze non-
Fernandez, Laura Isabel +2 more
core
, 2016 The main purpose of this paper is to investigate the effects of rapid assimilation‐forecast cycling on the performance of ionospheric data assimilation during geomagnetic storm conditions.
Chia-Hung Chen +7 more
semanticscholar +1 more source