activity
20082026
most citedCME-CME Interactions as Sources of CME Geo-effectiveness: The Formation of the Complex Ejecta and Intense Geomagnetic Storm in Early September 2017

112 citations · 1.2k across the 62 of their papers we have counts for

collaborators
Showing 2019Show all

11 papers · 1 filter

astro-ph.SR2019★ 112 cited

CME-CME Interactions as Sources of CME Geo-effectiveness: The Formation of the Complex Ejecta and Intense Geomagnetic Storm in Early September 2017

Camilla Scolini, Emmanuel Chané, Manuela Temmer +9

Coronal mass ejections (CMEs) are the primary sources of intense disturbances at Earth, where their geo-effectiveness is largely determined by their dynamic pressure and internal m…

astro-ph.SR2019★ 11 cited

Comprehensive Characterization of Solar Eruptions With Remote and In-Situ Observations, and Modeling: The Major Solar Events on 4 November 2015

Iver H. Cairns, Kamen A. Kozarev, Nariaki V. Nitta +12

Solar energetic particles (SEPs) are an important product of solar activity. They are connected to solar active regions and flares, coronal mass ejections (CMEs), EUV waves, shocks…

astro-ph.SR2019★ 50 cited

Testing the background solar wind modelled by EUHFORIA

J. Hinterreiter, J. Magdalenic, M. Temmer +10

In order to address the growing need for more accurate space weather predictions, a new model named EUHFORIA (EUropean Heliospheric FORecasting Information Asset) was recently deve…

physics.space-ph2019★ 5 cited

Spreading protons in the heliosphere: a note on cross-field diffusion effects

Nicolas Wijsen, Angels Aran, Jens Pomoell +1

We study how a high-speed solar wind stream embedded in a slow solar wind affects the transport and energy changes of solar energetic protons in interplanetary space, assuming diff…

astro-ph.SR2019★ 45 cited

Reconstructing coronal hole areas with EUHFORIA and adapted WSA model: optimising the model parameters

Eleanna Asvestari, Stephan G. Heinemann, Mannuela Temmer +4

The adopted WSA model embedded in EUHFORIA (EUropean Heliospheric FORecasting Information Asset) is compared to EUV observations. According to the standard paradigm coronal holes a…

astro-ph.SR2019★ 16 cited

Probing the effect of cadence on the estimates of photospheric energy and helicity injections in eruptive active region NOAA AR 11158

E. Lumme, M. D. Kazachenko, G. H. Fisher +3

In this work we study how the input data cadence affects the photospheric energy and helicity injection estimates in eruptive NOAA active region 11158. We sample the novel 2.25-min…

astro-ph.SR2019★ 26 cited

Multipoint study of successive coronal mass ejections driving moderate disturbances at 1 AU

Erika Palmerio, Camilla Scolini, David Barnes +10

We analyse in this work the propagation and geoeffectiveness of four successive coronal mass ejections (CMEs) that erupted from the Sun during 21--23 May 2013 and that were detecte…

physics.space-ph2019★ 34 cited

FORESAIL-1 cubesat mission to measure radiation belt losses and demonstrate de-orbiting

FORESAIL collaboration, M. Palmroth, J. Praks +57

Today, the near-Earth space is facing a paradigm change as the number of new spacecraft is literally sky-rocketing. Increasing numbers of small satellites threaten the sustainable…

astro-ph.SR2019★ 94 cited

Observation-based modelling of magnetised Coronal Mass Ejections with EUHFORIA

Camilla Scolini, Luciano Rodriguez, Marilena Mierla +2

Coronal Mass Ejections (CMEs) are the primary source of strong space weather disturbances at Earth. Their geoeffectiveness is largely determined by their dynamic pressure and inter…

physics.space-ph2019★ 18 cited

Interplanetary spread of solar energetic protons near a high-speed solar wind stream

Nicolas Wijsen, Angels Aran, Jens Pomoell +1

We study how a high-speed solar wind stream embedded in a slow solar wind influences the spread of solar energetic protons in interplanetary space. To model the energetic protons,…

physics.space-ph2019★ 55 cited

Modelling three-dimensional transport of solar energetic protons in a corotating interaction region generated with EUHFORIA

N. Wijsen, A. Angels, J. Pomoell +1

We introduce a new solar energetic particle (SEP) transport code that aims at studying the effects of different solar wind configurations on SEP events. We focus on the influence o…