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]
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]
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
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]
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]
The British Geological Survey (BGS) is part of the Natural Environment Research Council and is its principal supplier of national capability in geoscience.
core
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
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
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
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]
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

