[PDF] Top 20 Observation of solar energetic particle (SEP) events associated with narrow CMEs
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Observation of solar energetic particle (SEP) events associated with narrow CMEs
... other hand, Kallenrode (1996) suggested that a CME-driven shock may not itself accelerate significant numbers of parti- cles out of the ambient solar wind to high energies, but it can confine and re-accelerate ... See full document
5
Major solar eruptions and high energy particle events during solar cycle 24
... major solar eruptions that occurred on the frontside of the Sun during the rise to peak phase of cycle 24 (first 62 months) in order to understand the key factors affecting the occurrence of large solar ... See full document
15
Relation between Solar Flares, Halo and Partial Halo Coronal Mass Ejections, and Solar Energetic Particle Events
... cause, solar flares and CMEs. Only Halo and Partial Halo CMEs are considered for this study as they are directed towards Earth and hence are likely to cause SEPs measured at 1 ...control ... See full document
18
Differences between CME driven storms and CIR driven storms
... 1999a]. Energetic-particle events are also produced by CIRs (by CIR shocks in the helio- sphere beyond 2 AU, with the energetic particles traveling back to 1 AU) [Reames, 1999b], but their ... See full document
17
Interplanetary particle transport simulation for warning system for aviation exposure to solar energetic particles
... four SEP events on 27 January 2012, 13 March 2012, 17 May 2012, and 6 January 2014 that were recorded by the GOES P6 and P7 chan- nels, the square error of the fitting was minimized using the simplex ...the ... See full document
13
The solar energetic particle event of 2010 August 14: connectivity with the solar source inferred from multiple spacecraft observations and modeling
... This SEP event was associated with a fast halo CME observed by the Large Angle and Spectrometric Coronagraph ( LASCO ) on board SOHO ( Brueckner et ...The SEP event was also associated with a ... See full document
24
Observational study of interplanetary coronal mass ejections and flare in the solar corona
... remote solar observations at the Earth. The identified CMEs are measured and their basic attributes are catalogued in a data base known as the e have investigated some properties of all the fast and slow ... See full document
6
Synthesis of 3-D coronal-solar wind energetic particle acceleration modules
... 3. Energetic particles are accelerated over a broad latitudinal and longitudinal spread from the CME released following destabilization shown in Figure ...conditions, CMEs and associated shocks, and ... See full document
8
History and development of coronal mass ejections as a key player in solar terrestrial relationship
... of CMEs (Howard et ...halo CMEs are regular CMEs but viewed head- on (Gopalswamy et ...observe CMEs much closer to the Sun (see ...(HIs). CMEs were tracked in three dimensions (Mierla ... See full document
18
Photometric and Statistical Analysis of Solar Energetic Particle (SEP) for the Peak of Solar Cycle 24
... of solar cycle (24) (2012-2015) have been ...of solar eruptions by tracking SEP associated with CME for the peak of solar cycle (24) (2012-2015), on this basis the most important ... See full document
13
Solar Energetic Particles (SEP) and Galactic Cosmic Rays (GCR) as tracers of solar wind conditions near Saturn:event lists and applications
... 46 SEP events. Most events last more than two weeks and have their lowest occurrence rate around the extended solar minimum between 2008 and 2010, suggesting that they are associated to ... See full document
64
Observation of shocks associated with CMEs in 2007
... of CMEs with the solar wind can lead to the formation of interplanetary ...the solar energetic protons observed in the vicinity of the ...shocks associated with Co-rotating Interaction ... See full document
9
Frequency distributions: from the sun to the earth
... treme events? Basically, there are two approaches that are used for this purpose: “case by case” or “applying statis- ...individual solar flares using multi- wavelength observations. Such single-case ... See full document
15
Observation of the Internal Structure of Energetic Particle-Driven MHD Modes in a Large Helical Device
... of energetic particle-driven MHD instabilities, such as toroidal Alfv´en eigenmodes, is ...the energetic particles are measured in the plasma core region, and the measured values are consistent with ... See full document
5
THE SURVEY OF PARKER SOLAR PROBE
... A corona (Latin, 'crown') is an aura of plasma that surrounds the Sun and other stars. The Sun's corona extends millions of kilometers into outer space and is most easily seen during a total solar eclipse, but it ... See full document
11
Study Of Long-Term And Storm-Time Variations In Earth’S Magnetic Field And Morphology Of Geomagnetic Storms
... 2007. A catalogue of large geomagnetic storms (Table 1) has been compiled. Different types of solar, interplanetary and geomagnetic indices data are available through different world-wide situated solar and ... See full document
15
Propagation of coronal mass ejections in the inner heliosphere
... assumptions about the propagation direction can allow accurate kinematics to be derived for selected events, especially those on the limb. Even then, care must be taken in their interpretation (Byrne et al., ... See full document
242
An investigation of energetic particle injections associated with magnetospheric substorms
... the solar wind speed can double without warning and the interplanetary magnetic field can chaotically spin and ...the solar wind can disable terrestrial electrical networks such as power systems and ... See full document
235
Coronal mass ejections and Jump in solar wind plasma temperature in association with shock related geomagnetic storms
... earth solar wind, magnetic field and plasma data of omni data set, which consists of one hour resolution near earth, solar wind magnetic field and plasma data, energetic proton fluxes and geomagnetic ... See full document
6
Modelling cosmic ray ground level enhancements
... Conclusion The ground level response to solar particle events can be successfully modelled using functional representations of particle pitch angle distributions and rigidity spectra, co[r] ... See full document
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