Results 41 to 50 of about 295,213 (157)

Multiwavelength Study on Solar and Interplanetary Origins of the Strongest Geomagnetic Storm of Solar Cycle 23

open access: yes, 2011
We study the solar sources of an intense geomagnetic storm of solar cycle 23 that occurred on 20 November 2003, based on ground- and space-based multiwavelength observations.
B. Schmieder   +34 more
core   +1 more source

Effects of St. Patrick's Day Geomagnetic Storm of March 2015 and of June 2015 on Low‐Equatorial D Region Ionosphere

open access: yesJournal of Geophysical Research: Space Physics, 2018
D region effects of the 17–19 March 2015, a St Patrick's Day super geomagnetic storm (Dst = −223 nT), using a navigational transmitter very low frequency (VLF) signal (NWC, 19.8 kHz) recorded at a low‐latitude Indian station, Allahabad (geomag.
A. Maurya   +5 more
semanticscholar   +1 more source

Midlatitude ionospheric F2-layer response to eruptive solar events-caused geomagnetic disturbances over Hungary during the maximum of the solar cycle 24: a case study [PDF]

open access: yesAdv.Space.Res.61:1230-1243,2018, 2018
In our study we analyze and compare the response and behavior of the ionospheric F2 and of the sporadic E-layer during three strong (i.e., Dst <-100nT) individual geomagnetic storms from years 2012, 2013 and 2015, winter time period. The data was provided by the state-of the art digital ionosonde of the Sz\'echenyi Istv\'an Geophysical Observatory ...
arxiv   +1 more source

Studying Ionosphere Responses to a Geomagnetic Storm in June 2015 with Multi-Constellation Observations

open access: yesRemote Sensing, 2018
The Global Navigation Satellite System (GNSS) observations with global coverage and high temporal and spatial resolution, provide abundant and high-quality Earth-ionosphere observations.
Yang Liu   +3 more
semanticscholar   +1 more source

Satellite Drag Analysis During the May 2024 Gannon Geomagnetic Storm [PDF]

open access: yesJournal of Spacecraft and Rockets 2024 61:5, 1412-1416
Between May 10-12, 2024, Earth saw its largest geomagnetic storm in over 20 years. Since the last major storm in 2003, the population of satellites in low Earth orbit has surged following the commercialization of space services and the ongoing establishment of proliferated LEO constellations.
arxiv   +1 more source

Characterization of G -Semigroup by Intuitionistic N-Fuzzy Set (INFS) and its level set [PDF]

open access: yes, 2017
Some characterizations of G -Semigroup by intuitionistic N-fuzzy sets have been given here. The concept of intuitionistic N-fuzzy set (INFS) and its level set has been applied to G -semigroup.
Iqbal, Zaffar   +2 more
core   +1 more source

Observations of Low‐Latitude Red Aurora in Mexico During the 1859 Carrington Geomagnetic Storm

open access: yesSpace Weather, 2018
One of the most intense geomagnetic storm that has been documented in recent history occurred on 1 September 1859. This storm is known as the Carrington Event.
J. A. Gonzalez-Esparza   +1 more
semanticscholar   +1 more source

A Machine Learning and Computer Vision Approach to Geomagnetic Storm Forecasting [PDF]

open access: yesarXiv, 2022
Geomagnetic storms, disturbances of Earth's magnetosphere caused by masses of charged particles being emitted from the Sun, are an uncontrollable threat to modern technology. Notably, they have the potential to damage satellites and cause instability in power grids on Earth, among other disasters.
arxiv  

The Influence of Internal Atmospheric Variability on the Ionosphere Response to a Geomagnetic Storm

open access: yes, 2018
The Whole Atmosphere Community Climate Model eXtended is used to investigate the extent to which neglecting the realistic day‐to‐day lower atmospheric variability introduces uncertainty in the ionosphere response to an idealized geomagnetic storm.
N. Pedatella, H. Liu
semanticscholar   +1 more source

Geoelectric Field Evaluation During the September 2017 Geomagnetic Storm: MA.I.GIC. Model

open access: yesSpace Weather, 2019
The space environment near Earth is constantly subjected to changes in the solar wind flow generated at the Sun. Examples of this variability are the occurrence of powerful solar disturbances, such as coronal mass ejections (CMEs).
Mirko Piersanti   +4 more
semanticscholar   +1 more source

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