activity
20192022
most citedObservation-based modelling of the energetic storm particle event of 14 July 2012

37 citations · 139 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202237 cited

CMEs and SEPs During November-December 2020: A Challenge for Real-Time Space Weather Forecasting

Erika Palmerio, Christina O. Lee, M. Leila Mays +20

Predictions of coronal mass ejections (CMEs) and solar energetic particles (SEPs) are a central issue in space weather forecasting. In recent years, interest in space weather predi…

astro-ph.SR202210 cited

In-situ Measurement of the Energy Fraction in Supra-thermal and Energetic Particles at ACE, Wind, and PSP Interplanetary Shocks

Liam David, Federico Fraschetti, Joe Giacalone +3

The acceleration of charged particles by interplanetary shocks (IPs) can drain a non-negligible fraction of the plasma pressure. In this study, we have selected 17 IPs observed in-…

astro-ph.SR202225 cited

Direct First PSP Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in November 2020

Teresa Nieves-Chinchilla, Nathalia Alzate, Hebe Cremades +18

We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 Novem…

physics.space-ph202237 cited

Observation-based modelling of the energetic storm particle event of 14 July 2012

Nicolas Wijsen, Angels Aran, Camilla Scolini +6

We model the energetic storm particle (ESP) event of 14 July 2012 using the energetic particle acceleration and transport model named PARADISE, together with the solar wind and cor…

physics.space-ph2021

Energy Balance at Interplanetary Shocks: In-situ Measurement of the Fraction in Supra-thermal and Energetic Particles with ACE and Wind

Liam David, Federico Fraschetti, Joe Giacalone +3

The acceleration of charged particles by interplanetary shocks can drain a non-negligible fraction of the upstream ram pressure. For a sample of shocks observed in-situ at 1 AU by…

physics.space-ph202130 cited

A Self-consistent Simulation of Proton Acceleration and Transport Near a High-speed Solar Wind Stream

Nicolas Wijsen, Evangelia Samara, Àngels Aran +3

Solar wind stream interaction regions (SIRs) are often characterized by energetic ion enhancements. The mechanisms accelerating these particles, as well as the locations where the…