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Coronal Mass Ejection (CME)

Interplanetary coronal mass ejection observed at STEREO A, Mars, comet 67P/Churyumov Gerasimenko, Saturn, and New Horizons en route to Pluto  Comparison of its Forbush decreases at 1 4, 3 1 and 9 9 AU:Interplanetary coronal mass ejection

Interplanetary coronal mass ejection observed at STEREO A, Mars, comet 67P/Churyumov Gerasimenko, Saturn, and New Horizons en route to Pluto Comparison of its Forbush decreases at 1 4, 3 1 and 9 9 AU:Interplanetary coronal mass ejection

... The study presented here was motivated by the analysis of Mars Express data acquired during the flyby of the Siding-Spring comet on 19 October 2014 [e.g. Svedhem et al., 2014; Gurnett et al., 2015]. A preliminary ...

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The eruption of a small scale emerging flux rope as the driver of an M class flare and of a coronal mass ejection

The eruption of a small scale emerging flux rope as the driver of an M class flare and of a coronal mass ejection

... motion, convergence fl ow, magnetic reconnection, and magnetic cancellation ( van Ballegooijen & Martens 1989; Moore et al. 2001; Fan 2009; Priest & Longcope 2017 ) . Recently, more and more observational evidence ...

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Simultaneous interplanetary scintillation and Heliospheric Imager observations of a coronal mass ejection

Simultaneous interplanetary scintillation and Heliospheric Imager observations of a coronal mass ejection

... (IPS) and STEREO Heliospheric Imager (HI) observations of a coronal mass ejection (CME) on 16 May 2007. Strong CME signatures were present throughout the IPS observation. The IPS raypath lay within ...

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Identification Of Interplanetary Coronal Mass Ejection With Magnetic Cloud In Year 2005 At 1 AU

Identification Of Interplanetary Coronal Mass Ejection With Magnetic Cloud In Year 2005 At 1 AU

... Abstract: Coronal mass ejection (CMEs) propagate in to the interplanetary medium are called as Interplanetary Coronal Mass Ejection ...

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Geomagnetic effects of high density plasma with southward magnetic field in the interplanetary coronal mass ejection observed on May 2–3, 1998

Geomagnetic effects of high density plasma with southward magnetic field in the interplanetary coronal mass ejection observed on May 2–3, 1998

... interplanetary coronal mass ejection (ICME) observed during the May 2–3, 1998 geomagnetic ...of coronal helmet ...of coronal helmet ...of coronal helmet ...

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Interplanetary coronal mass ejection observed at STEREO A, Mars, comet 67P/Churyumov Gerasimenko, Saturn, and New Horizons en route to Pluto  Comparison of its Forbush decreases at 1 4, 3 1 and 9 9 AU:Interplanetary coronal mass ejection

Interplanetary coronal mass ejection observed at STEREO A, Mars, comet 67P/Churyumov Gerasimenko, Saturn, and New Horizons en route to Pluto Comparison of its Forbush decreases at 1 4, 3 1 and 9 9 AU:Interplanetary coronal mass ejection

... CME ejection on 14 October at 18:30 UT and an extended period with high level of irradiance in both fi lters are clearly ...Connection Coronal and Heliospheric Investigation (SECCHI)/Extreme Ultraviolet ...

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Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations

Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations

... Solar wind and coronal mass ejections (CMEs) some- times cause geospace disturbances when they arrive at the Earth. These disturbances are closely related to social infrastructures such as radio ...

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Evidence for internal tether cutting in a flare/coronal mass ejection observed by Messenger, Rhessi, and Stereo

Evidence for internal tether cutting in a flare/coronal mass ejection observed by Messenger, Rhessi, and Stereo

... The relationship between eruptive flares and coronal mass ejections (CMEs) is a topic of ongoing debate, especially regarding the possibility of a common initiation mechanism. We studied the kinematic and ...

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Coronal Mass Ejection Detection using Wavelets, Curvelets and Ridgelets: Applications for Space Weather Monitoring

Coronal Mass Ejection Detection using Wavelets, Curvelets and Ridgelets: Applications for Space Weather Monitoring

... Coronal mass ejections (CMEs) are large-scale eruptions of plasma and magnetic field that can produce adverse space weather at Earth and other lo- cations in the ...

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Magnetospheric preconditioning under northward IMF: evidence from the study of coronal mass ejection and corotating interaction region geoeffectiveness

Magnetospheric preconditioning under northward IMF: evidence from the study of coronal mass ejection and corotating interaction region geoeffectiveness

... magnetosphere (as indicated by the Dst index) to the passage of coronal mass ejections (CMEs) and corotating interaction regions (CIRs). We first focused on the difference between the measured Dst signature ...

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Coronal mass ejection mass, energy, and force estimates using STEREO

Coronal mass ejection mass, energy, and force estimates using STEREO

... The mass development of core and front with time is shown in Fig- ure ...two mass measurements are subject to an observational effect of apparent exponential mass growth, however by the time the CME ...

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The Storm Time Response of the Inner Magnetosphere During Coronal Mass Ejection and
        Corotating Interaction Region Driven Storms, Samuel Bingham

The Storm Time Response of the Inner Magnetosphere During Coronal Mass Ejection and Corotating Interaction Region Driven Storms, Samuel Bingham

... THE RADIATION BELT RESPONSE TO CHORUS WAVE ACTIVITY AND SEED ELECTRON DEVELOPMENT DURING CME- OR CIR-DRIVEN STORMS.. 161.[r] ...

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Characterizing Coronal Mass Ejections in Solar Cycle Analysis

Characterizing Coronal Mass Ejections in Solar Cycle Analysis

... flares, coronal mass ejections (CMEs), and solar ...the coronal mass ejection, its trend during solar cycle 23 and gives significance to the statistical nature in the form of normality ...

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Effect of Coronal Mass Ejection on Earth’s Magnetic Field during Ascending Phase of  Solar Cycles 23 24

Effect of Coronal Mass Ejection on Earth’s Magnetic Field during Ascending Phase of Solar Cycles 23 24

... the coronal mass ejections (CMEs) play a central role in the enhancing of interplanetary and geomagnetic activity [1] [2] ...[7]. Coronal mass ejections (CMEs) are identified in the images of ...

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GUMICS 4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds

GUMICS 4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds

... Abstract. We study the response of the Earth’s magneto- sphere to fluctuating solar wind conditions during interplane- tary coronal mass ejections (ICMEs) using the Grand Unified Magnetosphere-Ionosphere ...

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Energetic particle precipitation into the middle atmosphere triggered by a coronal mass ejection

Energetic particle precipitation into the middle atmosphere triggered by a coronal mass ejection

... Experimental Setup [9] This paper combines data from subionospheric VLF radio wave receivers, the high-altitude MINIS balloons, riometers, and pulsation magnetometers to describe the geo[r] ...

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The geospace response to variable inputs from the lower atmosphere: a review of the progress made by Task Group 4 of CAWSES-II

The geospace response to variable inputs from the lower atmosphere: a review of the progress made by Task Group 4 of CAWSES-II

... CME: coronal mass ejection; COSMIC: Constellation Observing System for Meteorology; CTIPe: Coupled Thermosphere Ionosphere Plasmasphere Electrodynamics Model; CTMT: Climatological Tidal Model of the ...

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Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection

Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection

... Abstract. We present a comprehensive statistical analysis of mirror mode waves and the properties of their plasma sur- roundings in sheath regions driven by interplanetary coro- nal mass ejection (ICME). We ...

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Evolution of magnetic helicity during eruptive flares and coronal mass ejections

Evolution of magnetic helicity during eruptive flares and coronal mass ejections

... or coronal mass ejection is that, after the slow buildup of magnetic helicity in a magnetic structure, the eruption is triggered and drives three-dimensional reconnection which adds energy to ...

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Machine Learning Classification of Interplanetary Coronal Mass Ejections Using Satellite Accelerometers

Machine Learning Classification of Interplanetary Coronal Mass Ejections Using Satellite Accelerometers

... Space weather phenomena is a complex area of research. An eruption of energy on the sur- face of the Sun sends high-energy particles towards Earth, a signature of the beginning of an event known as an Interplanetary ...

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