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Magnetic Storm

Electrodynamics in the duskside inner magnetosphere and plasmasphere during a super magnetic storm on March 13–15, 1989

Electrodynamics in the duskside inner magnetosphere and plasmasphere during a super magnetic storm on March 13–15, 1989

... the magnetic storm appear outside the plasmapause again as shown in the left panels M and ...the magnetic storm, the electric field intensity in the outer region of L > 4 ...

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Magnetic Storm Effects on The Ionospheric F2-Layer Over Czech Republic

Magnetic Storm Effects on The Ionospheric F2-Layer Over Czech Republic

... the magnetic storm was observed to be a moderate storm with a minimum decrease of Dst -73nT, during this storm, a maximum increase of 83% in the electron density of the F2- layer (NmF2) was ...

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Application of the Fengyun 3 C GNSS occultation sounder for assessing the global ionospheric response to a magnetic storm event

Application of the Fengyun 3 C GNSS occultation sounder for assessing the global ionospheric response to a magnetic storm event

... strong magnetic storm event in March 2015 were ana- lyzed using GNOS results supported by ionosonde observa- ...The magnetic storm caused a significant disturbance in NmF2 ...geomagnetic ...

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The frequency variation of Pc5 ULF waves during a magnetic storm

The frequency variation of Pc5 ULF waves during a magnetic storm

... the magnetic storm on July 15, 2000 is studied using ground-based magnetometer data and particle observations by the LANL ...the storm, the frequency drop of the Pc5 in the IMAGE chain around the MLT ...

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Ionospheric irregularity behavior during the September 6–10, 2017 magnetic storm over Brazilian equatorial–low latitudes

Ionospheric irregularity behavior during the September 6–10, 2017 magnetic storm over Brazilian equatorial–low latitudes

... two-step magnetic storm was caused by an X9 solar flare followed by a ...the storm was caused by a B z southward incursion on day 07. The magnetic index K p reached 08, and the Sym-H ...

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The strong Pc5 geomagnetic pulsations in the initial phase of the great magnetic storm of March 24, 1991

The strong Pc5 geomagnetic pulsations in the initial phase of the great magnetic storm of March 24, 1991

... To summarize, the main pecularities of the pulsations analysed above are 1) the latitude independency of their spectrum, in both regimes, quasi-noisy as well as nearly monochromatic, and 2) the sudden disappearance of ...

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Time scale of the largest imaginable magnetic storm

Time scale of the largest imaginable magnetic storm

... ton” storm of September 1859 (Tsurutani et ...imaginable magnetic storm: “the largest depression of the geomagnetic field that could possibly occur” as the result of interaction with the solar wind, ...

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April 2000 magnetic storm: Solar wind driver and magnetospheric response

April 2000 magnetic storm: Solar wind driver and magnetospheric response

... onboard SOHO first observed a halo CME on 4 April 2000 at 1632 UT. This CME caused a strong magnetic storm at the Earth 2 days later. The initial observations were made after a 90 min data gap, when the ...

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Equatorial sporadic E layer abnormal density enhancement during the recovery phase of the December 2006 magnetic storm: A case study

Equatorial sporadic E layer abnormal density enhancement during the recovery phase of the December 2006 magnetic storm: A case study

... variation of this parameter. This also occurred during the recovery phase of the magnetic storm analyzed. The peak explored in the present work was associated with the pres- ence of a sporadic layer type ...

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A large scale traveling ionospheric disturbance during the magnetic storm of 15 September 1999

A large scale traveling ionospheric disturbance during the magnetic storm of 15 September 1999

... suggested in this paper on the basis of the LSTID observation and model calculation. The number preceding each comment indicates the order of occurrence. The poleward neutral wind is generated as a gravity wave probably ...

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The low latitude ionospheric effects of the April 2000 magnetic storm near the longitude 120°E

The low latitude ionospheric effects of the April 2000 magnetic storm near the longitude 120°E

... 2000 storm by the model of Fejer and Scherliess (1997) and Scherliess and Fejer ...2000 storm, the E × B plasma drifts of storm origin are the cause of the near simultaneity of height disturbances at ...

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Prediction of magnetic storm events using the

Prediction of magnetic storm events using the

... new storm onset given that there was no storm in the previ- ous k − 1 periods in a k-string setting, for example, the event 000000000001 in a ...of storm onsets such as 000000000001 would normally ...

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Variation of Total Ozone during 24 August 2005  Magnetic Storm: A Case Study

Variation of Total Ozone during 24 August 2005 Magnetic Storm: A Case Study

... considered storm occurred after a relatively quiet geomagnetic period and it is not superposed by another perturbation, which permit us to identify clearly the effects of the geomagnetic storm on total ...

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The nonlinear coupling of electromagnetic ion cyclotron and lower hybrid waves in the ring current region: the magnetic storm 1–7 May 1998

The nonlinear coupling of electromagnetic ion cyclotron and lower hybrid waves in the ring current region: the magnetic storm 1–7 May 1998

... the magnetic field line, longitudinal and radial drifts of the wave pack- ets are ...dipole magnetic field and Kp depen- dent Volland-Stern convection field are adopted in these stud- ...

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Magnetic storm free ULF analysis in relation with earthquakes in Taiwan

Magnetic storm free ULF analysis in relation with earthquakes in Taiwan

... quake magnitude. Thus, seismo-magnetic anomalies would be related to timings, location, and magnitude of forthcom- ing earthquakes. Although Chen et al. (2011b) reported that earthquake-related stress changes can ...

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Magnetic storm effects at equatorial electrojet stations

Magnetic storm effects at equatorial electrojet stations

... Earth’s magnetic field was suggested by Stewart (1882) as due to the movement of the conducting upper atmosphere across the vertical component of the earth’s magnetic field arising by the regular atmo- ...

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Equatorial enhancement of Pc5–6 magnetic storm time geomagnetic pulsations

Equatorial enhancement of Pc5–6 magnetic storm time geomagnetic pulsations

... Shinohara et al. (1998) while analyzing geomagnetic data from latitudinally dense network of stations in Brazilian sec- tor have shown that the phases of Pi2 and Pc4–5 pulsations lag at the dip equator (obscure) than ...

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Statistical analysis of the mid latitude trough position during different categories of magnetic storms and different storm intensities

Statistical analysis of the mid latitude trough position during different categories of magnetic storms and different storm intensities

... to magnetic storm, ...the storm peak and then slowly recovers to initial ...During magnetic storms, the longitudinal effect of the trough position can be ...the storm sequence ...

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Storm time magnetic field variations observed by the ETS VI satellite

Storm time magnetic field variations observed by the ETS VI satellite

... a magnetic storm is the growth and recovery of the ring current flow- ing in the inner ...a magnetic storm occurs, charged particles in the magnetotail are injected by an increase of the ...

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Storm Door Hazards

Storm Door Hazards

... The apparent increase’ of injuries to children by broken glass in doors may well require in- creased attention by safety-minded pediatri- cians.. The problem stems from the use of ordi- [r] ...

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