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[PDF] Top 20 On the radiation belt location during the 23rd and 24th solar cycles

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On the radiation belt location during the 23rd and 24th solar cycles

On the radiation belt location during the 23rd and 24th solar cycles

... the solar minimum was ap- ...degrees) during the declin- ing phase of the 24th solar cycle compared with its loca- tion during the 23rd solar ...observed during 2 ... See full document

14

On the radiation belt location in the solar cycles

On the radiation belt location in the solar cycles

... indicate latitudes of the maximum and inner edge of the outer radiation belt, respectively.. The same as Figure 4 but for the inner edge of the outer radiation belt[r] ... See full document

35

Analysis of the Heliosphere During Major Solar Energetic Particle Events of the 23rd Solar cycle

Analysis of the Heliosphere During Major Solar Energetic Particle Events of the 23rd Solar cycle

... that during solar events particle acceleration can happen in three different ...first location is at the hot flare ...second location is at the shocks when they are propagating at in the outer ... See full document

59

The cusp: a window for particle exchange between the radiation belt and the solar wind

The cusp: a window for particle exchange between the radiation belt and the solar wind

... A set of test particle simulations in the T96 model are pre- sented to prove these results. To make a better prediction, a more accurate magnetic model in the cusp region is required. Acknowledgements. We are grateful to ... See full document

7

Average profiles of the solar wind and outer radiation belt during the extreme flux enhancement of relativistic electrons at geosynchronous orbit

Average profiles of the solar wind and outer radiation belt during the extreme flux enhancement of relativistic electrons at geosynchronous orbit

... of solar wind parame- ters and geomagnetic activities superposed at 17:00 UT of the day of maximum flux at ...days during the storm recovery phase, as indicated by two vertical dahsed ... See full document

5

The relativistic electron response in the outer radiation belt during magnetic storms

The relativistic electron response in the outer radiation belt during magnetic storms

... the solar wind must also be ...the solar wind speed was first reported by Williams and Smith (1965) and Williams (1966) and later by Paulikas and Blake ...up-stream solar wind conditions and found ... See full document

9

The global statistical response of the outer radiation belt during geomagnetic storms

The global statistical response of the outer radiation belt during geomagnetic storms

... outer radiation belt is a toroidal region of the magnetosphere between ~2 and 7 Earth radii from the cen- ter of the Earth populated by trapped electrons with energies from hundreds of 100s of keV to ... See full document

12

Variation of proton radiation belt deduced from solar cell degradation of Akebono satellite

Variation of proton radiation belt deduced from solar cell degradation of Akebono satellite

... the solar cells of the Akebono satellite due to various space radiations, and found a signature of a deformed proton radiation belt in ...the solar cells decreased slowly from 13A in 1989 to ... See full document

5

Measurement of the Direct Flux of Solar Radiation During Operation of a Big Solar Furnace

Measurement of the Direct Flux of Solar Radiation During Operation of a Big Solar Furnace

... measuring solar radiation are considered and long-term data obtained by actinometric measurements of solar radiation at the location of the big solar furnace of the Academy of ... See full document

8

Multi-satellite simultaneous observations of magnetopause and atmospheric losses of radiation belt electrons during an intense solar wind dynamic pressure pulse

Multi-satellite simultaneous observations of magnetopause and atmospheric losses of radiation belt electrons during an intense solar wind dynamic pressure pulse

... and to investigate the underlying physical processes of loss during an intense solar wind dynamic pressure pulse. Basi- cally, adoption of electron fluxes cannot rule out the adia- batic effect that mixes ... See full document

17

A density-temperature description of the outer electron radiation belt during geomagnetic storms

A density-temperature description of the outer electron radiation belt during geomagnetic storms

... electron radiation belt suddenly decreases to very low levels (essen- tially to instrument-background ...magnetosphere during the storm [Denton and Borovsky, 2008, ...not) solar wind in the ... See full document

20

Characteristic of Ionospheric foF2 and Solar Indices during the 23rd Solar Cycle over High Latitude Station, Syowa, Antarctica

Characteristic of Ionospheric foF2 and Solar Indices during the 23rd Solar Cycle over High Latitude Station, Syowa, Antarctica

... the solar parameters as well as the (foF2) show two maxima, with the second maximum higher than the first ...from location to location, indicating that direct linear relationship of foF2 with ... See full document

9

Spatial Distribution of Radiation Belt Protons Deduced from Solar Cell Degradation of the Arase Satellite

Spatial Distribution of Radiation Belt Protons Deduced from Solar Cell Degradation of the Arase Satellite

... The signature of a large flux of energetic protons can be seen as contamination in the particle detectors on board the Arase satellite. However, we did not see any abrupt change in the estimated Voc (Figure 2) or ... See full document

17

The atmospheric implications of radiation belt remediation

The atmospheric implications of radiation belt remediation

... “Radiation Belt Remediation” ...artificial radiation belt in- jected by a Starfish Prime-type HANE over either 1 or 10 days, assuming a space-based system operating over all local ... See full document

17

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

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

... It should be mentioned that a least squares Gaussian fit to the observed chorus spectral intensity is per- formed over a specific 3 min period 17:13:00–13:16:00 UT on 17 March, corresponding to the maximum amplitude and ... See full document

10

Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm

Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm

... dynamics during the 17 March 2013 storm, when energetic electrons experienced very ef fi cient acceleration within ~12 ...peak location at L ...peak location, which indicates that chorus waves play a ... See full document

15

Influences of Solar Cycles on Earthquakes

Influences of Solar Cycles on Earthquakes

... of solar cycles on earthquakes through of statistical ...earthquakes during solar ...events during approximately four hundred years (1600- ...of Solar cycle, and also de- pends ... See full document

8

Simulation of solar radiation during a total eclipse: a challenge for radiative transfer

Simulation of solar radiation during a total eclipse: a challenge for radiative transfer

... with location but varies of course in the case of a solar ...for solar eclipse simula- ...each location in the TOA reference plane to the ra- diance/irradiance at the ... See full document

12

Simulation of solar radiation during a total eclipse: a challenge for radiative transfer

Simulation of solar radiation during a total eclipse: a challenge for radiative transfer

... with location but varies of course in the case of a solar ...for solar eclipse simula- ...each location in the TOA reference plane to the ra- diance/irradiance at the ... See full document

13

Energetic electron enhancements under the radiation belt (L 
            Energetic electron enhancements under the radiation belt (L 
        
        
            
                Energetic electron enhancements under the radiation belt (L 

Energetic electron enhancements under the radiation belt (L  Energetic electron enhancements under the radiation belt (L  Energetic electron enhancements under the radiation belt (L  Energetic electron enhancements under the radiation belt (L  Alla V Suvorova et al

... the solar wind should trigger some processes in the magnetosphere–ionosphere system that might result in the electron injections into the forbidden ...fore during weak geomagnetic ...chain during ... See full document

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