From Sun to Interplanetary Space: What is the Pathlength of Solar Energetic Particles?

Solar energetic particles (SEPs), accelerated during solar eruptions, propagate in turbulent solar wind before being observed with in situ instruments. In order to interpret their origin through comparison with remote sensing observations of the solar eruption, we thus must deconvolve the transport...

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Veröffentlicht in:	The Astrophysical journal 2019-12, Vol.887 (2), p.222
Hauptverfasser:	Laitinen, T., Dalla, S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Energetic particles Eruptions Heliosphere Interplanetary physics Interplanetary space Interplanetary turbulence Islands Magnetic fields Magnetic islands Random walk Remote sensing Solar energetic particles Solar wind Sun
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