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441
Large Geomagnetically Induced Currents at Equator Caused by an Interplanetary Magnetic Cloud
Published 2022-06-01“…The responsible physical mechanisms were examined through magneto‐hydrodynamic model simulations and found that a prompt penetration of strong westward‐overshielding electric fields and ionospheric currents at the equator play a dominant role. …”
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442
Multilayered Sporadic‐E Response to the Annular Solar Eclipse on June 21, 2020
Published 2021-03-01“…Abstract A moon shadow of annular solar eclipse passed through East Asia in the afternoon on June 21, 2020, which was a good opportunity to study the rapid ionospheric response to the solar radiation variations. …”
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443
A Generalized Oblique Projection Filter with Flexible Parameter for Interference Suppression
Published 2015-01-01“…Further, an application of GOP filter in ionospheric clutter cancellation in a high frequency surface wave radar (HFSWR) system is given. …”
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444
Determination of Auroral Electrodynamic Parameters From AMPERE Field‐Aligned Current Measurements
Published 2021-04-01“…The electric fields are then used with the conductances to calculate horizontal ionospheric currents. We validate the results by simulating the SuperMAG magnetic indices for 30 geomagnetically active days. …”
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445
A Method to Mitigate the Effects of Strong Geomagnetic Storm on GNSS Precise Point Positioning
Published 2022-01-01“…To mitigate the adverse effects of strong geomagnetic storms, we propose to establish the geometry‐free (GF) cycle slip threshold model based on ionospheric disturbance index rate of total electron content index to reduce the false detection rate of cycle slip in GNSS precise point positioning (PPP) during strong storm periods, thus improving the accuracy and reliability of GNSS PPP. …”
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446
A Cycle Slip Detection and Repair Method Using BDS Triple-Frequency Optimization Combination with Wavelet Denoising
Published 2022-01-01“…The dual-frequency phase ionospheric residual (PIR) method has the ability to detect sensitive small cycle slips, but its detection results have multivalue problems. …”
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447
GA-ARMA Model for Predicting IGS RTS Corrections
Published 2017-01-01“…For precise positioning, users should correct for GNSS error components such as satellite orbit and clock errors as well as ionospheric delay. The international GNSS service (IGS) real-time service (RTS) can be used to correct orbit and clock errors in real-time. …”
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448
The Flare Irradiance Spectral Model‐Version 2 (FISM2)
Published 2020-12-01“…FISM2 is also improved to 0.1‐nm spectral bins across the same 0‐ to 190‐nm spectral range and is already being used in research to estimate space weather changes due to solar irradiance variability in planetary thermospheres and ionospheres.…”
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449
Detection of GRBs and OTs by All-Sky Optical and SID Monitors
Published 2010-01-01“…The second method is the GRB detection based on their ionospheric response.…”
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450
Intelligent methods for natural data analysis: application to space weather
Published 2024-02-01“…Using the problem of detecting ionospheric anomalies as an example, the efficiency of combining threshold wavelet filtering with the NARX network is shown. …”
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451
A Proper Use of the Adjacent Land‐Based Observatory Magnetic Field Data to Account for the Geomagnetic Disturbances During Offshore Directional Drilling
Published 2022-12-01“…These measurements are the superposition of the signals from the internal, core and crustal, and external, ionospheric and magnetospheric sources and the noise from magnetic elements in the borehole assembly. …”
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452
Solar EUV‐Enhancement and Thermospheric Disturbances
Published 2021-12-01“…The proposed physical mechanism driving the Dst changes is linked to the increased production of O+ ions of ionospheric origin, which may occur over the EUV‐enhancement period.…”
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453
Upper‐Atmosphere Mass Density Variations From CASSIOPE Precise Orbits
Published 2021-04-01“…In this study, TMD is estimated from the precise orbits of CAScade SmallSat and IOnospheric Polar Explorer (CASSIOPE) at one‐second time step, and the TMD variations following the February 2014 geomagnetic storm are investigated. …”
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454
Recreating the Horizontal Magnetic Field at Colaba During the Carrington Event With Geospace Simulations
Published 2021-05-01“…The mechanism behind this has previously been attributed to magnetospheric processes, ionospheric processes or a combination of both. In this study, we outline our efforts to replicate this low‐latitude magnetic field using the Space Weather Modeling Framework. …”
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455
ROTI‐Based Stochastic Model to Improve GNSS Precise Point Positioning Under Severe Geomagnetic Storm Activity
Published 2022-07-01“…Abstract For global navigation satellite system (GNSS), ionospheric disturbances caused by the geomagnetic storm can reduce the accuracy and reliability of precision point positioning (PPP). …”
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456
Global TEC Map Fusion Through a Hybrid Deep Learning Model: RFGAN
Published 2023-01-01“…For the integrity and continuity of the global observation data, deep learning can obtain a global Ionospheric total electron content (TEC) map by fusing multi‐source TEC maps. …”
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457
Climatological Statistics of Extreme Geomagnetic Fluctuations With Periods From 1 s to 60 min
Published 2021-11-01“…Rates of exceedance are explained by reference to the magneto‐ionospheric processes dominant in different latitude and MLT sectors, including ULF waves, interplanetary shocks, auroral substorm currents, and traveling convection vortices. …”
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458
Nowcasting Solar EUV Irradiance With Photospheric Magnetic Fields and the Mg II Index
Published 2024-04-01“…With daily global photospheric magnetic maps and Mg II index observations, this study provides an improved method of nowcasting EUV & FUV bands used to drive thermospheric and ionospheric modeling.…”
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459
Nighttime Geomagnetic Response to Jumps of Solar Wind Dynamic Pressure: A Possible Cause of Québec Blackout in March 1989
Published 2023-11-01“…Soon after another pair related to the main impulse (MI) appears and travels in the anti‐sunward direction. The horizontal ionospheric current associated with the MI remains strong when propagating to the nightside. …”
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460
Lyman‐alpha Variability During Solar Flares Over Solar Cycle 24 Using GOES‐15/EUVS‐E
Published 2020-07-01“…We also show that increased Lyα flux is closely correlated with induced currents in the ionospheric E‐layer through the detection of the solar flare effect as observed by the Kakioka magnetometer.…”
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