Results 91 to 100 of about 2,928 (232)

Automated real time detection of solar wind shocks and consequences for the identification of SSC and SI events [PDF]

open access: yes, 2005
Algorithms have been developed to automatically detect Earth bound shocks in the solar wind as measured by the ACE satellite. These involve simple threshold techniques and wavelet analysis.
Baillie, O.   +4 more
core  

Understanding GIC in the UK and French high-voltage transmission systems during severe magnetic storms [PDF]

open access: yes, 2017
The measurement and collection of digital magnetic field data in Europe extends back to the 1970s, providing over 30 years of data for the analysis of severe space weather.
A. Viljanen   +26 more
core   +1 more source

Automated Detection of Equatorial Plasma Bubbles From the Magnetic Measurements of Macau Science Satellite‐1 Using Machine Learning

open access: yesSpace Weather, Volume 24, Issue 4, April 2026.
Abstract Equatorial plasma bubbles (EPBs) are plasma density depletion structures that produce magnetic field perturbations through the diamagnetic effect and therefore need to be identified and excluded in high‐precision geomagnetic field modeling. Traditional EPB detection methods typically rely on in situ electron density or total electron content ...
Xinyi Rang   +3 more
wiley   +1 more source

Revised prediction of LDEF exposure to trapped protons [PDF]

open access: yes
The Long Duration Exposure Facility (LDEF) spacecraft flew in a 28.5 deg inclination circular orbit with an altitude in the range from 319.4 to 478.7 km.
Armstrong, T. W.   +2 more
core   +1 more source

British Geological Survey Annual Science Review 2012-13 [PDF]

open access: yes, 2013
The British Geological Survey (BGS) is part of the Natural Environment Research Council and is its principal supplier of national capability in geoscience.

core  

Global Impacts of Ultra‐Low‐Frequency Waves: 1. Thermospheric Responses and Traveling Atmospheric Disturbances

open access: yesGeophysical Research Letters, Volume 53, Issue 6, 28 March 2026.
Abstract Ultra‐low‐frequency (ULF) waves cause local Thermosphere‐Ionosphere (T‐I) perturbations, but their impacts on the global T‐I system including the generation of Traveling Atmospheric Disturbances (TADs) have never been evaluated. The mechanisms responsible for the TAD generation and propagation, whether through dynamic or thermal process, are ...
Haonan Wu   +6 more
wiley   +1 more source

Automated Coronal Hole Identification via Multi-Thermal Intensity Segmentation

open access: yes, 2017
Coronal holes (CH) are regions of open magnetic fields that appear as dark areas in the solar corona due to their low density and temperature compared to the surrounding quiet corona.
Gallagher, Peter T.   +2 more
core   +1 more source

Mesospheric and Lower Thermospheric Responses to the May 2024 Geomagnetic Storm in the Antarctic Peninsula

open access: yesGeophysical Research Letters, Volume 53, Issue 6, 28 March 2026.
Abstract We analyze the response of mean winds and semidiurnal tides (SDTs) in the mesosphere and lower thermosphere (MLT; ∼70–110 km altitude) to the May 2024 geomagnetic super storm, based on meteor radar (MR) observations from King Sejong Station (KSS; geographic: 62.22°S, 58.78°W; geomagnetic: 53.27°S, 10.88°E) in the Antarctic Peninsula.
Byeong‐Gwon Song   +8 more
wiley   +1 more source

Influence of Pipeline Insulation Leakage Points on the Distribution of Geomagnetically Induced Current and Pipe-Soil Potential

open access: yesIEEE Access, 2019
During geomagnetic storms, geomagnetically induced currents (GIC) and pipe-soil potential (PSP) generated in a pipeline present a risk to the safe operation of the pipeline.
Chenglian Ma, Chunming Liu
doaj   +1 more source

Future directions for LDEF ionizing radiation modeling and assessments [PDF]

open access: yes
A calculational program utilizing data from radiation dosimetry measurements aboard the Long Duration Exposure Facility (LDEF) satellite to reduce the uncertainties in current models defining the ionizing radiation environment is in progress. Most of the
Armstrong, T. W., Colborn, B. L.
core   +1 more source

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