[PDF] Top 20 Nanodust dynamics during a coronal mass ejection
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Nanodust dynamics during a coronal mass ejection
... a nanodust population near the Sun and an indication of the type and expected magnitude of its ...The mass of the CME as described by the model is about ... See full document
17
Coronal mass ejection mass, energy, and force estimates using STEREO
... and dynamics property esti- mates cannot be carried out when unknown propaga- tion angle hinders an accurate calculation of CME mass, hence adding unacceptable uncertainty to any subse- quent ...as ... See full document
8
Proton beam velocity distributions in an interplanetary coronal mass ejection
... The associated ICME revealed the expected typical signa- tures, such as a magnetic field rotation indicating the mag- netic flux rope of a MC. The solar wind flow speed ranged between 400 and 500 km/s during this ... See full document
7
Propagation of an Earth-directed coronal mass ejection in three dimensions
... trajectory have to be inferred from either its association with a source region on-disk 33 or its trajectory through the COR data 15 , or derived by assuming a constant velocity through the HI fields-of-view 34 . ... See full document
30
An unusual giant spiral arc in the polar cap region during the northward phase of a Coronal Mass Ejection
... from coronal holes reaches the ...By during northward IMF or a deformation of the magnetopause caused by solar wind density fluctuations (maybe in connection with magne- topause surface waves) are possible ... See full document
11
Simultaneous interplanetary scintillation and Heliospheric Imager observations of a coronal mass ejection
... Brown, D. S., D. Bewsher, and C. J. Eyles (2008), Calibrating the pointing and optical parameters of the STEREO Heliospheric Imagers, Sol. Phys., in press. Canals, A. (2002), Interplanetary scintillation studies of the ... See full document
6
Energetic particle precipitation into the middle atmosphere triggered by a coronal mass ejection
... [ 23 ] At L 4, shown by Jyva¨skyla¨ at L = 3.7, the picture appears quite similar with a burst of enhanced ionization at the start of the CME, followed by a relatively flat response until a small absorption event at ... See full document
12
Multi-wavelength study of a flare and burst associated coronal mass ejection
... shock during the enhancement frequency emission between the height range 8 Ro – 42 ...CME during high density solar wind-CME interaction which was driven by the ... See full document
7
From the Sun to the Earth: the 13 May 2005 Coronal Mass Ejection
... distance of ∼ 200 R and is more dominant to the east. In the last scan, the ICME has already moved out of the Earth’s orbit and beyond the Ooty IPS FOV. The Pushchino Radio Astronomy Observatory was used at the ... See full document
79
CORONAL MASS EJECTION SHOCK AND SHEATH STRUCTURES RELEVANT TO PARTICLE ACCELERATION
... 3.1. Computational Mesh The computational domain for the simulation extends over the range defined by192 R < x < 192 R , 48 R < y < 336 R , and 192 R < z < 192 R , with the Sun placed at the ori- gin. The ... See full document
15
Planar magnetic structures in coronal mass ejection-driven sheath regions
... Solar wind and IMF measurements are taken primarily from the Wind spacecraft. Wind was launched in November 1994. It spent its first years at the Lagrangian point L1 and in 1999 it acquired a complex petal-shaped orbit ... See full document
10
Effect of Coronal Mass Ejection on Earth’s Magnetic Field during Ascending Phase of Solar Cycles 23 24
... DOI: 10.4236/ijaa.2017.73017 216 International Journal of Astronomy and Astrophysics Figure 3. Shows the distribution of total CMEs according to Angular width for the as- cending phase of solar cycles 23 and 24. maximum ... See full document
8
Coronal Mass Ejection-driven Shocks and the Associated Sudden Commencements-sudden Impulses
... electrojet (EEJ) currents, is one of the prime contributors of geomagnetic field data to World Data Center (WDC), Kyoto, Japan, for calculating the storm time disturbance index (Dst). It is found that there is not much ... See full document
11
Uncovering the birth of a coronal mass ejection from two viewpoint SECCHI observations
... CME. The time offsets between the SXR and CME acceleration peaks are within 5 min of each other. There is even indication for an earlier acceleration jump associated with a small step in the SXR flux at around 7:00 UT. ... See full document
18
(1)A NUMERICAL STUDY OF THE BREAKOUT MODEL FOR CORONAL MASS EJECTION INITIATION P
... the ejection of the plasmoid represents approximately 80% of the total originally injected into the ...the coronal helicity, a significant fraction remains behind, which implies that some other mechanism ... See full document
14
ANGEO - The response of the magnetosphere to the passage of a coronal mass ejection on March 20−21 1990
... ®rst particle injection event identi®ed by the LANL spacecraft. The response time of Dst to the southward turning at 1314 (5) UT March 21 is again consistent with the maximum high-latitude (67°N) ionospheric response ... See full document
14
The Storm Time Response of the Inner Magnetosphere During Coronal Mass Ejection and Corotating Interaction Region Driven Storms, Samuel Bingham
... enhanced during the storm main phase from the nightside towards dusk due to the main phase enhancement of the cross-tail convection electric field which provides ac- cess to the inner magnetosphere via open drift ... See full document
274
GUMICS 4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds
... Figure 1 shows the arrival of the leading shock at 18:53 UT on 14 July 2012 as the simultaneous abrupt jump in the plasma and magnetic field parameters and the following ICME sheath as irregular directional changes in ... See full document
19
(1)THE CORONAL-DIMMING FOOTPRINT OF A STREAMER-PUFF CORONAL MASS EJECTION: CONFIRMATION OF THE MAGNETIC-ARCH-BLOWOUT SCENARIO Ronald L
... consequent coronal dimming observed in EIT Fe xii images, along with their setting in a registered MDI magnetogram, are shown in Figure ...progress during the GOES X-ray burst; the arrow points to the ... See full document
8
Coronal Mass Ejection Detection using Wavelets, Curvelets and Ridgelets: Applications for Space Weather Monitoring
... These advanced image processing techniques are likely to be of use for real-time space weather operations, and in addition, to the analysis of large data-volumes from future ground- and space-based imagers. For space ... See full document
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