Abstract Solar Energetic Particle (SEP) events are interesting from a scientific perspective as
they are the product of a broad set of physical processes from the corona out through the …

After decades of observations of solar energetic particles from space-based observatories,
relevant questions on particle injection, transport, and acceleration remain open. To address …

Solar energetic particle (SEP) events are related to both solar flares and coronal mass
ejections (CMEs) and they present energy spectra that span from a few keV up to several …

Solar eruptions are the main driver of space-weather disturbances at Earth. Extreme events
are of particular interest, not only because of the scientific challenges they pose, but also …

Aims. We model the energetic storm particle (ESP) event of 14 July 2012 using the energetic
particle acceleration and transport model named 'PArticle Radiation Asset Directed at …

We present an event observed by Parker Solar Probe (PSP) at∼ 0.2 au on 2022 March 2 in
which imaging and in situ measurements coincide. During this event, PSP passed through …

Aims. We introduce a new solar energetic particle (SEP) transport code that aims at studying
the effects of different background solar wind configurations on SEP events. In this work, we …

Capabilities to predict onset and time profiles of solar‐driven events, including solar X‐ray
flares; solar energetic particles (SEP); coronal mass ejections; and high‐speed streams, are …

Understanding the transport of solar energetic particles (SEPs) from acceleration sites at the
Sun into interplanetary space and to the Earth is an important question for forecasting space …

The solar corona between below 10 solar radii is an important region for early acceleration
and transport of solar energetic particles (SEPs) by coronal mass ejection-driven shock …