[PDF] Top 20 The kinematics and morphology of solar coronal mass ejections
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The kinematics and morphology of solar coronal mass ejections
... In the magnetic breakout model the CME eruption is triggered by reconnection between the overlying field and a neighbouring flux system through the shearing of a multipolar topology, illustrated in Figure 1.14 (Antiochos ... See full document
265
Automatic detection and tracking of coronal mass ejections II Multiscale filtering of coronagraph images
... CME morphology, the scattering effects and non-linear intensity profile of the surrounding corona, the presence of coro- nal streamers, and the addition of noise due to cosmic rays and solar energetic ... See full document
18
The kinematics of coronal mass ejections using multiscale methods
... analysing solar active region evo- lution (Hewett et al. 2008), and enhancing solar coronal images (Stenborg & Cobelli 2003; Stenborg et ...its morphology (width, orientation) and kine- ... See full document
10
Large scale Bright Fronts in the Solar Corona: A Review of "EIT waves"
... the coronal scale-height of 50–100 Mm for quiet Sun tem- peratures of 1–2 MK, and typical of what is expected for the propagation of a fast-mode MHD wave in the quiet solar ...EUV coronal waves have ... See full document
34
Coronal mass ejections and Jump in solar wind plasma temperature in association with shock related geomagnetic storms
... in solar wind plasma temperature (JSWT) events which are associated with shock related geomagnetic storms and studied statistical behavior of these events with coronal mass ... See full document
6
Radial and azimuthal oscillations of halo coronal mass ejections in the Sun
... We present the first observational detection of radial and azimuthal oscil- lations in full halo coronal mass ejections (HCMEs). We analyze nine HCMEs well-observed by the Large Angle and ... See full document
14
Aspects of the relationship between active regions and coronal mass ejections
... 2 solar radii from disc centre (below ...0.1 solar radii above the ...observe coronal features on the limb and the ARs in this study include a range of longitudes and have not been selected to meet ... See full document
163
Coronal Mass Ejections during Geomagnetic Storms on Earth
... It also showed up during the events of 2000 and 2001, there are multiple entries relating great geomagnetic events as compared to other years because this was the time where the Sun has reached its peaked and NASA ... See full document
6
Relation between Solar Flares, Halo and Partial Halo Coronal Mass Ejections, and Solar Energetic Particle Events
... Above two paragraphs indicate the impact of the two CME parameters called linear speed and angular width. It is necessary to study the impact of the flare parameters also. Flare class is a major parameter of the ... See full document
18
Statistical Study of Interplanetary Coronal Mass Ejections with Strong Magnetic Fields
... of solar flare strength and the Solar Dynamics Observatory (SDO) spacecraft which has the Helioseismic and Magnetic Imager (HMI) instrument on ...the solar source magnetic ... See full document
123
Uncertainties in polarimetric 3D reconstructions of coronal mass ejections
... The analysis reported here also demonstrates that halo CME can be well characterized unless their projected altitude ρ is too small. In particular, even if it is possible to provide images of the inner part of the ... See full document
8
Evolution of magnetic helicity during eruptive flares and coronal mass ejections
... eruptive solar flares and coronal mass ejections, a non-potential mag- netic arcade with much excess magnetic energy goes unstable and ... See full document
20
Study Of Symmetric And Asymmetric Short Term Cosmic Ray Intensity Decreases From 1997 To 2013
... with coronal mass ejections ...x-ray solar flares of different ...x-ray solar flare and most of the symmetric cosmic ray intensity decreases are found to be associated with C class ... See full document
9
The spectroscopic imprint of the pre eruptive configuration resulting into two major coronal mass ejections
... Following the observations, CME initiation models can also be divided into two broad categories: models with pre- existing FRs and models with FR formation during the erup- tion. Most models that form twisted magnetic ... See full document
14
Machine Learning Classification of Interplanetary Coronal Mass Ejections Using Satellite Accelerometers
... to solar storms, can be derived using the on-board accelerometer of GRACE, is it possible to see similar changes and fluctuations in the raw, unprocessed data, that could be used for space weather monitoring ... See full document
129
The Analysis of Interplanetary Shocks Associated with Six Major Geo Effective Coronal Mass Ejections during Solar Cycle 24
... In this section of observation, we obtained the arrival time using second-order speed of CMEs instead of linear speed reported in the LASCO/SOHO catalogue. So here we are estimating transit time from Equation (3) by ... See full document
9
Space Weather Association with Sunspots and Geomagnetic Storms for Solar Cycle 23 (1996-2007) and Solar Cycle 24 (2008-2016)
... that coronal mass ejections (CMEs) and solar flares are also responsible for geomagnetic storms and a good correlation between sunspot number and coronal mass ejections ... See full document
6
THE SURVEY OF PARKER SOLAR PROBE
... Parker Solar Probe is the only imaging instrument aboard the ...and solar wind before the spacecraft flies through ...like coronal mass ejections, or CMEs, jets and other ejecta from ... See full document
11
Observational study of interplanetary coronal mass ejections and flare in the solar corona
... Interplanetary Coronal Mass Ejections (ICMEs) are the region of light scattered due to the electron densities in solar ...of Coronal the purpose of establishing the relationship between ... See full document
6
Statistical Relation Of Coronal Mass Ejections And Solar Wind Disturbances With Radio Bursts Related Geomagnetic Storms
... the solar center could cause intense geomagnetic ...halo coronal mass ejections and concluded that the geoeffectiveness of partial halo CMEs is lower because they are of low speed and likely ... See full document
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