FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3017151508> ?p ?o ?g. }

• W3017151508 endingPage "951" @default.
• W3017151508 startingPage "931" @default.
• W3017151508 abstract "Abstract. Recently, it has been established that interplanetary coronal mass ejections (ICMEs) can dramatically affect both trapped electron fluxes in the outer radiation belt and precipitating electron fluxes lost from the belt into the atmosphere. Precipitating electron fluxes and energies can vary over a range of timescales during these events. These variations depend on the initial energy and location of the electron population and the ICME characteristics and structures. One important factor controlling electron dynamics is the magnetic field orientation within the ejecta that is an integral part of the ICME. In this study, we examine Van Allen Probes (RBSPs) and Polar Orbiting Environmental Satellites (POESs) data to explore trapped and precipitating electron fluxes during two ICMEs. The ejecta in the selected ICMEs have magnetic cloud characteristics that exhibit the opposite sense of the rotation of the north–south magnetic field component (BZ). RBSP data are used to study trapped electron fluxes in situ, while POES data are used for electron fluxes precipitating into the upper atmosphere. The trapped and precipitating electron fluxes are qualitatively analysed to understand their variation in relation to each other and to the magnetic cloud rotation during these events. Inner magnetospheric wave activity was also estimated using RBSP and Geostationary Operational Environmental Satellite (GOES) data. In each event, the largest changes in the location and magnitude of both the trapped and precipitating electron fluxes occurred during the southward portion of the magnetic cloud. Significant changes also occurred during the end of the sheath and at the sheath–ejecta boundary for the cloud with south to north magnetic field rotation, while the ICME with north to south rotation had significant changes at the end boundary of the cloud. The sense of rotation of BZ and its profile also clearly affects the coherence of the trapped and/or precipitating flux changes, timing of variations with respect to the ICME structures, and flux magnitude of different electron populations. The differing electron responses could therefore imply partly different dominant acceleration mechanisms acting on the outer radiation belt electron populations as a result of opposite magnetic cloud rotation." @default.
• W3017151508 created "2020-04-24" @default.
• W3017151508 creator A5006591924 @default.
• W3017151508 creator A5007535974 @default.
• W3017151508 creator A5008520842 @default.
• W3017151508 creator A5009475272 @default.
• W3017151508 creator A5020163516 @default.
• W3017151508 creator A5021348886 @default.
• W3017151508 creator A5053663225 @default.
• W3017151508 creator A5087195287 @default.
• W3017151508 date "2020-08-28" @default.
• W3017151508 modified "2023-10-12" @default.
• W3017151508 title "Outer Van Allen belt trapped and precipitating electron flux responses to two interplanetary magnetic clouds of opposite polarity" @default.
• W3017151508 cites W1571696717 @default.
• W3017151508 cites W1578289780 @default.
• W3017151508 cites W1585557767 @default.
• W3017151508 cites W1588383312 @default.
• W3017151508 cites W1615413734 @default.
• W3017151508 cites W1626272402 @default.
• W3017151508 cites W1889533513 @default.
• W3017151508 cites W1899519118 @default.
• W3017151508 cites W1906361797 @default.
• W3017151508 cites W1938807356 @default.
• W3017151508 cites W1962829677 @default.
• W3017151508 cites W1965883346 @default.
• W3017151508 cites W1969316888 @default.
• W3017151508 cites W1974669404 @default.
• W3017151508 cites W1978673845 @default.
• W3017151508 cites W1979752318 @default.
• W3017151508 cites W1982916298 @default.
• W3017151508 cites W1987495055 @default.
• W3017151508 cites W1997935893 @default.
• W3017151508 cites W1998709248 @default.
• W3017151508 cites W2019173865 @default.
• W3017151508 cites W2020192861 @default.
• W3017151508 cites W2022853993 @default.
• W3017151508 cites W2022883321 @default.
• W3017151508 cites W2024621340 @default.
• W3017151508 cites W2039776955 @default.
• W3017151508 cites W2041936080 @default.
• W3017151508 cites W2042271521 @default.
• W3017151508 cites W2047312950 @default.
• W3017151508 cites W2056431769 @default.
• W3017151508 cites W2057993361 @default.
• W3017151508 cites W2058817053 @default.
• W3017151508 cites W2066067534 @default.
• W3017151508 cites W2071983443 @default.
• W3017151508 cites W2074805056 @default.
• W3017151508 cites W2076616463 @default.
• W3017151508 cites W2078743489 @default.
• W3017151508 cites W2086292892 @default.
• W3017151508 cites W2087353542 @default.
• W3017151508 cites W2090693627 @default.
• W3017151508 cites W2097615993 @default.
• W3017151508 cites W2100718824 @default.
• W3017151508 cites W2104248815 @default.
• W3017151508 cites W2104503686 @default.
• W3017151508 cites W2127112787 @default.
• W3017151508 cites W2128527697 @default.
• W3017151508 cites W2136001518 @default.
• W3017151508 cites W2140839232 @default.
• W3017151508 cites W2142227531 @default.
• W3017151508 cites W2144212043 @default.
• W3017151508 cites W2154353907 @default.
• W3017151508 cites W2162326489 @default.
• W3017151508 cites W2163990113 @default.
• W3017151508 cites W2168857545 @default.
• W3017151508 cites W2169054245 @default.
• W3017151508 cites W2243118106 @default.
• W3017151508 cites W2323064125 @default.
• W3017151508 cites W2429376441 @default.
• W3017151508 cites W2474499982 @default.
• W3017151508 cites W2594699752 @default.
• W3017151508 cites W2607972703 @default.
• W3017151508 cites W2617688903 @default.
• W3017151508 cites W2735189374 @default.
• W3017151508 cites W2737089961 @default.
• W3017151508 cites W2755331818 @default.
• W3017151508 cites W2760476843 @default.
• W3017151508 cites W2770563800 @default.
• W3017151508 cites W2773245711 @default.
• W3017151508 cites W2792061377 @default.
• W3017151508 cites W2794427626 @default.
• W3017151508 cites W2795877741 @default.
• W3017151508 cites W2891768774 @default.
• W3017151508 cites W2891845492 @default.
• W3017151508 cites W2905686039 @default.
• W3017151508 cites W2910817225 @default.
• W3017151508 cites W2924153241 @default.
• W3017151508 cites W2942801002 @default.
• W3017151508 cites W2947477807 @default.
• W3017151508 cites W2955576273 @default.
• W3017151508 cites W2961415522 @default.
• W3017151508 cites W2971190011 @default.
• W3017151508 cites W2986157780 @default.
• W3017151508 cites W2989885852 @default.
• W3017151508 cites W4251409017 @default.
• W3017151508 doi "https://doi.org/10.5194/angeo-38-931-2020" @default.

• next