FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3092693503> ?p ?o ?g. }

• W3092693503 abstract "&lt;p align=&quot;justify&quot;&gt;The pitch-angle distribution of electron intensities is an essential piece of information in order to understand the transport processes undergone by the particles in their journey from their acceleration sites to the spacecraft and, to infer properties of the particle sources such as their intensity and duratio&lt;span&gt;n&lt;/span&gt;.&lt;/p&gt; &lt;p align=&quot;justify&quot;&gt;&lt;span&gt;In a previous work, we modelled fifteen solar relativistic electron events observed at different heliocentric radial distances by the Helios spacecraft (Pacheco et al. 2019). We used a Monte-Carlo transport model and an inversion procedure to fit the in-situ observations, and inferred both the electron mean free path in the interplanetary space and the injection histories of the electrons at two solar radii from the Sun. We applied a full inversion procedure, that is, we considered both the angular and the energetic responses of the Helios/E6 particle experiment in the modelling of the electron events. &lt;/span&gt;&lt;/p&gt; &lt;p align=&quot;justify&quot;&gt;&lt;span&gt;By using the same methodology as previously employed for ACE/EPAM, STEREO/SEPT and Helios/E6 instruments, we have modelled the angular response of the Electron Proton Telescope (EPT) of the Energetic Particle Detector (EPD) on board Solar Orbiter. Here, we present the study of the modelled angular response and its application to several of the solar energetic particle (SEP) events previously modelled as if Solar Orbiter were located at the Helios position. We compare the pitch-angle distributions measured by Solar Orbiter and Helios at different phases of the intensity-time profile of the SEP events, that is, near the particle onset, peak and on the decay of the event, and for different interplanetary magnetic field orientations provided by the Helios measurements. &lt;/span&gt;&lt;/p&gt; &lt;p align=&quot;justify&quot;&gt;We found that despite Helios were spinning spacecraft which gathered electron information from eight angular sectors, the four Solar Orbiter/EPD/EPT fields of view will often offer similar angular coverage. We also found that, under specific circumstances, EPT can obtain better pitch angle distribution information than Helios, specifically when the interplanetary magnetic field points away from the ecliptic.&lt;/p&gt; &lt;p align=&quot;justify&quot;&gt;&lt;span&gt;We expect, then, that Solar Orbiter will provide us with numerous and valuable observations that will permit us to untangle the transport effects that electrons, protons and ions suffer in their journey through interplanetary space. &lt;/span&gt;&lt;/p&gt;" @default.
• W3092693503 created "2020-10-22" @default.
• W3092693503 creator A5002111617 @default.
• W3092693503 creator A5007972896 @default.
• W3092693503 creator A5010540726 @default.
• W3092693503 creator A5030266079 @default.
• W3092693503 creator A5055430033 @default.
• W3092693503 creator A5062579977 @default.
• W3092693503 creator A5073440177 @default.
• W3092693503 creator A5073451062 @default.
• W3092693503 creator A5088103676 @default.
• W3092693503 date "2020-03-10" @default.
• W3092693503 modified "2023-10-18" @default.
• W3092693503 title "Seeing Helios electron data through the eyes of Solar Orbiter: modelling the angular response of EPD/EPT and its application to the full inversion of Helios events" @default.
• W3092693503 doi "https://doi.org/10.5194/egusphere-egu2020-21407" @default.
• W3092693503 hasPublicationYear "2020" @default.
• W3092693503 type Work @default.
• W3092693503 sameAs 3092693503 @default.
• W3092693503 citedByCount "0" @default.
• W3092693503 crossrefType "posted-content" @default.
• W3092693503 hasAuthorship W3092693503A5002111617 @default.
• W3092693503 hasAuthorship W3092693503A5007972896 @default.
• W3092693503 hasAuthorship W3092693503A5010540726 @default.
• W3092693503 hasAuthorship W3092693503A5030266079 @default.
• W3092693503 hasAuthorship W3092693503A5055430033 @default.
• W3092693503 hasAuthorship W3092693503A5062579977 @default.
• W3092693503 hasAuthorship W3092693503A5073440177 @default.
• W3092693503 hasAuthorship W3092693503A5073451062 @default.
• W3092693503 hasAuthorship W3092693503A5088103676 @default.
• W3092693503 hasConcept C121332964 @default.
• W3092693503 hasConcept C1276947 @default.
• W3092693503 hasConcept C147120987 @default.
• W3092693503 hasConcept C184779094 @default.
• W3092693503 hasConcept C185544564 @default.
• W3092693503 hasConcept C2776481522 @default.
• W3092693503 hasConcept C29829512 @default.
• W3092693503 hasConcept C30475298 @default.
• W3092693503 hasConceptScore W3092693503C121332964 @default.
• W3092693503 hasConceptScore W3092693503C1276947 @default.
• W3092693503 hasConceptScore W3092693503C147120987 @default.
• W3092693503 hasConceptScore W3092693503C184779094 @default.
• W3092693503 hasConceptScore W3092693503C185544564 @default.
• W3092693503 hasConceptScore W3092693503C2776481522 @default.
• W3092693503 hasConceptScore W3092693503C29829512 @default.
• W3092693503 hasConceptScore W3092693503C30475298 @default.
• W3092693503 hasLocation W30926935031 @default.
• W3092693503 hasOpenAccess W3092693503 @default.
• W3092693503 hasPrimaryLocation W30926935031 @default.
• W3092693503 hasRelatedWork W10665211 @default.
• W3092693503 hasRelatedWork W14496336 @default.
• W3092693503 hasRelatedWork W16425120 @default.
• W3092693503 hasRelatedWork W29461076 @default.
• W3092693503 hasRelatedWork W33433787 @default.
• W3092693503 hasRelatedWork W33667252 @default.
• W3092693503 hasRelatedWork W34087262 @default.
• W3092693503 hasRelatedWork W36769147 @default.
• W3092693503 hasRelatedWork W46096731 @default.
• W3092693503 hasRelatedWork W917765 @default.
• W3092693503 isParatext "false" @default.
• W3092693503 isRetracted "false" @default.
• W3092693503 magId "3092693503" @default.
• W3092693503 workType "article" @default.