Timo Laitinen
Timo Laitinen
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magnetic fields
3D propagation of relativistic solar protons through interplanetary space
Context. Solar energetic particles (SEPs) with energy in the GeV range can propagate to Earth from their acceleration region near the …
S. Dalla
,
G. A. de Nolfo
,
A. Bruno
,
J. Giacalone
,
T. Laitinen
,
S. Thomas
,
M. Battarbee
,
M. S. Marsh
Cite
DOI
arXiv
Early propagation of energetic particles across the mean field in turbulent plasmas
Propagation of energetic particles across the mean field direction in turbulent magnetic fields is often described as spatial …
T. Laitinen
,
S. Dalla
,
D. Marriott
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DOI
arXiv
Energetic Particle Transport across the Mean Magnetic Field: Before Diffusion
Current particle transport models describe the propagation of charged particles across the mean field direction in turbulent plasmas as …
T. Laitinen
,
S. Dalla
Cite
DOI
arXiv
Solar energetic particle access to distant longitudes through turbulent field-line meandering
Context. Current solar energetic particle (SEP) propagation models describe the effects of interplanetary plasma turbulence on SEPs as …
T. Laitinen
,
A. Kopp
,
F. Effenberger
,
S. Dalla
,
M. S. Marsh
Cite
DOI
arXiv
Drift-induced Deceleration of Solar Energetic Particles
We investigate the deceleration of solar energetic particles (SEPs) during their propagation from the Sun through interplanetary space, …
S. Dalla
,
M. S. Marsh
,
T. Laitinen
Cite
DOI
arXiv
Energetic Particle Cross-field Propagation Early in a Solar Event
Solar energetic particles (SEPs) have been observed to easily spread across heliographic longitudes, and the mechanisms responsible for …
T. Laitinen
,
S. Dalla
,
M. S. Marsh
Cite
DOI
arXiv
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