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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

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

... and coronal mass ejections are the most powerful explosions in the ...a coronal mass ...the coronal three-dimensional magnetic fi ...

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

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

... which mass measurements are derived from white light coronagraph images is based on theory first developed by Minnaert (1930) in which the scatter- ing geometry of a single electron at a particular point in the ...

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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

... Figure 7 shows the magnetic fi eld, radiation data and solar wind velocity measured by Rosetta at comet 67P at 3.1 AU from the Sun. Figures 7a and 7b show the magnetic fi eld components and magnitude, respectively, as ...

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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

... [10] Yashiro, S., Gopalswamy, N., Michalek, G., St. Cyr, O.C., Plunkett, S.P., Rich, N.B. and Howard, R.A. (2004) A Catalog of White Light Coronal Mass Ejections Ob- served by the SOHO Spacecraft. Journal ...

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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

... dependence of CMEs geoeffectiveness on the polarity of magnetic clouds [Zhang and Burlaga, 1988; Fenrich and Luhmann, 1998; Li and Luhmann, 2004; Wu and Lepping, 2002, 2005]. However, a relation between CME magnetic ...

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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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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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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

... CMEs are intrinsically multiscale features, making their detection using wavelets and other multiscale techniques an attractive proposition. Stenborg & Cobelli (2003) were the first to apply a wavelet-based technique ...

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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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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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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

... This CME–flare system was observed over more than 4 hr using a multitude of instruments. Figure 3 shows the evolution of the system and Figure 4 explicitly shows the motion of both the CME and SXR loop-top sources ...

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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

... Coronal mass ejections (CMEs) cause disturbances in the environment of the Earth when they arrive at the Earth. However, the prediction of the arrival of CMEs still remains a challenge. We have developed an ...

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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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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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Evolution of magnetic helicity during eruptive flares and coronal mass ejections

Evolution of magnetic helicity during eruptive flares and coronal mass ejections

... a coronal mass ejection) and typically produce a two-ribbon flare, with two separating Hα ribbons joined by a rising arcade of flare ...some coronal mass ejections are associated with ...

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Statistical Relation Of Coronal Mass Ejections And Solar Wind Disturbances With Radio Bursts Related Geomagnetic Storms

Statistical Relation Of Coronal Mass Ejections And Solar Wind Disturbances With Radio Bursts Related Geomagnetic Storms

... solar coronal mass ejection (CME) sources for selected major geomagnetic storms in the geomagnetic field of ...halo coronal mass ejections (HCMEs) originating from ...

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