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[PDF] Top 20 A study of relativistic electron flux enhancements in the Earth's outer radiation belt

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A study of relativistic electron flux enhancements in the Earth's outer radiation belt

A study of relativistic electron flux enhancements in the Earth's outer radiation belt

... maximum flux enhancement occurring at L > ...the radiation belt, which are then transported inward while conserving the first two adiabatic ...the outer radiation belt ... See full document

198

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

... this study is to identify the development of chorus wave activity, the seed electron population, and the radiation belt response as a function of storm phase, the superposed epoch analysis ... See full document

274

Processes in auroral oval and outer electron radiation belt

Processes in auroral oval and outer electron radiation belt

... of relativistic electrons during the storms for which the electron fluxes before and after the storm are almost ...of electron fluxes is observed during the 30 September 2012 storm: The fluxes at L = ... See full document

11

Modeling inward diffusion and slow decay of energetic electrons in the Earth's outer radiation belt

Modeling inward diffusion and slow decay of energetic electrons in the Earth's outer radiation belt

... the Earths inner magnetosphere [Mauk et ...the radiation belt particle spectra with excellent energy and pitch angle ...Magnetic Electron Ion Spectrometer (MagEIS) instrument [Blake ... See full document

11

Butterfly pitch angle distribution of relativistic electrons in the outer radiation belt: Evidence of nonadiabatic scattering

Butterfly pitch angle distribution of relativistic electrons in the outer radiation belt: Evidence of nonadiabatic scattering

... this study we demonstrated the alternative approach for probing the magnetic field configuration with measurements of near-equatorial distributions of high-energy ...certain electron energies should directly ... See full document

20

Relative positions of the polar boundary of the outer electron radiation belt and the equatorial boundary of the auroral oval

Relative positions of the polar boundary of the outer electron radiation belt and the equatorial boundary of the auroral oval

... trapped radiation region of electrons with energy > 35 ...low-energy electron precipitation. However, this study was done using the data obtained for only 21 orbits, and was not widely ...auroral ... See full document

10

The problem of the acceleration of electrons of the outer radiation belt and magnetospheric substorms

The problem of the acceleration of electrons of the outer radiation belt and magnetospheric substorms

... high-energy electron fluxes filling a new radiation belt is an endeavor being carried out by physicists studying the ...high-energy electron fluxes that appeared during the recovery phase was ... See full document

8

Comparative study on earthquake and ground based transmitter induced radiation belt electron precipitation at middle latitudes

Comparative study on earthquake and ground based transmitter induced radiation belt electron precipitation at middle latitudes

... (peak-to-background flux ratio p/b > 20) energetic electron bursts in the presence of VLF activity, as observed from the DEMETER satellite at low al- titudes ( ∼ 700 ...inner radiation belts in ... See full document

13

Energetic, relativistic and ultra-relativistic electrons: Comparison of long-term VERB code simulations with Van Allen Probes measurements

Energetic, relativistic and ultra-relativistic electrons: Comparison of long-term VERB code simulations with Van Allen Probes measurements

... this study, we used the VERB code to model the dynamics of the outer electron radiation belt during a long period of time, which included various levels of geomagnetic ...the ... See full document

16

Main phase creation of “seed” electrons in the outer radiation belt

Main phase creation of “seed” electrons in the outer radiation belt

... producing relativistic electrons? Possible ones are following; ring current (Dst) effect and a wave-particle ...the flux variation of the energetic electrons in the outer belt and concluded ... See full document

7

Quantifying the relative contributions of substorm injections and chorus waves to the rapid outward extension of electron radiation belt

Quantifying the relative contributions of substorm injections and chorus waves to the rapid outward extension of electron radiation belt

... We study the rapid outward extension of the electron radiation belt on a timescale of several hours during three events observed by Radiation Belt Storm Probes and Time History ... See full document

20

James van Allen and his namesake NASA mission

James van Allen and his namesake NASA mission

... highly relativistic electrons ( E = 4.0– 5.0 million electron volts (MeV)) confined in the Earth’s magnetic ...the Relativistic Electron- Proton Telescope A ( REPT-A) and REPT-B measured ... See full document

5

Pc5 geomagnetic fluctuations in response to solar wind excitation and their relationship with relativistic electron fluxes in the outer radiation belt

Pc5 geomagnetic fluctuations in response to solar wind excitation and their relationship with relativistic electron fluxes in the outer radiation belt

... tron flux at geosynchronous orbit with the Pc5 power in the magnetosphere and at high and low latitude, at a time delay of approximately 2 days, in agreement with previous studies at auroral and middle latitudes ... See full document

9

What Fraction of the Outer Radiation Belt Relativistic Electron Flux at L approximate to 3 4 5 Was Lost to the Atmosphere During the Dropout Event of the St  Patrick's Day Storm of 2015?

What Fraction of the Outer Radiation Belt Relativistic Electron Flux at L approximate to 3 4 5 Was Lost to the Atmosphere During the Dropout Event of the St Patrick's Day Storm of 2015?

... What fraction of the outer radiation belt relativistic electron flux at L≈3-4.5 was lost to the atmosphere during the dropout event of the St Patrick’s Day storm of 2015?.. British Antar[r] ... See full document

47

Response of the equatorial electrojet to solar flare related X ray flux enhancements

Response of the equatorial electrojet to solar flare related X ray flux enhancements

... presented in detail the implications of such observations in relation to the lunar phase. Several studies on solar flare events occurring in the presence of a counter electrojet have been reported earlier (Srivastava, ... See full document

12

Modelling the outer radiation belt as a complex system in a self-organised critical state

Modelling the outer radiation belt as a complex system in a self-organised critical state

... For this work the solar wind velocity frequency distribu- tion was also fitted by a power-law and the results are shown in Fig. 9. The fit is not so good for the 1995 solar wind data and you can clearly see two ... See full document

9

Simulations of inner magnetosphere dynamics with an expanded RAM-SCB model and comparisons with Van Allen Probes observations

Simulations of inner magnetosphere dynamics with an expanded RAM-SCB model and comparisons with Van Allen Probes observations

... to Earth, the intensified westward ring current weakens the magnetic field especially across the ...and electron trajectories in the near-Earth region, leading to adiabatic redistribution and ... See full document

10

Cooling of relativistic electron beams in intense laser pulses : chirps and radiation

Cooling of relativistic electron beams in intense laser pulses : chirps and radiation

... esting study on the radiation spectra predicted by the clas- sical Landau–Lifshitz theory [27] where they found that negative chirps led to an increased rate of electron energy loss and a stronger ... See full document

6

Study of the Oceanic Heat Budget Components over the Arabian Sea during the Formation and Evolution of Super Cyclone, Gonu

Study of the Oceanic Heat Budget Components over the Arabian Sea during the Formation and Evolution of Super Cyclone, Gonu

... The Indian peninsula splits the north Indian Ocean into two basins, the Arabian Sea in the west and Bay of Ben- gal in the east. In 2007, an organized convection was formed on 28th May near southeastern Arabian Sea. ... See full document

9

Chorus acceleration of radiation belt relativistic electrons during March 2013 geomagnetic storm

Chorus acceleration of radiation belt relativistic electrons during March 2013 geomagnetic storm

... current study focuses on whether chorus waves can produce efficient accel- eration of relativistic electrons but is not intended to identify the relative contributions of in situ acceleration and radial ...of ... See full document

10

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