P-212initial Experience With the Abramson Procedure: A New Technique for Treatment of Pectus Carinatum

Rochus, Ine; Coosemans, Willy; Veer, Hans Van

doi:10.1093/icvts/ivx280.212

Cited by 1 publication

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“…by STIX (Krucker et al 2019) and EUI (Rochus et al 2019). The detection of flare accelerated particles close to the Sun will significantly reduce the influence of particle transport on estimates of the particle travel time and then on the particle escape time.…”

Section: Investigations On the Properties And Origin(s) Of Sepsmentioning

confidence: 95%

“…When magnetofrictinonal and MHD simulations are coupled, a pre-eruptive but unstable magnetic configuration is transferred from one another as initial condition and a typical plasma distribution is assumed (Pagano et al 2013b). In this approach, MHD simulations of CMEs can be used to infer the properties of the coronal plasma through the kinematic properties of the CME propagation (Pagano et al 2013a;Rodkin et al 2017), or by means of a more advanced diagnostic when we synthesize remote sensing measurements (Pagano et al 2014(Pagano et al , 2015.…”

Section: Solar Orbiter Contributions To Space Weather Researchmentioning

confidence: 99%

“…Heliophysics is at the dawn of a golden age in observational capabilities. In addition to the on-going space missions like A majority of Solar Orbiter science goals rely on coordinated observations with multiple instruments (Müller et al 2019), from IS instruments (Maksimovic et al 2019;Horbury et al 2019a;Owen & et al 2019;Rodríguez-Pacheco et al 2019) operating continuously along the orbit beginning in cruise phase, to the RS instruments (SPICE Consortium et al 2019;Solanki et al 2019;Krucker et al 2019;Antonucci et al 2019;Rochus et al 2019;Howard et al 2019) observing during three 10-day windows per orbit called Remote Sensing Windows (RSWs). The RSWs will typically be centred around perihelia as well as minimum and maximum heliographic latitudes.…”

Section: General Introductionmentioning

confidence: 99%

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Models and data analysis tools for the Solar Orbiter mission

Rouillard

Pinto

Vourlidas

et al. 2020

A&A

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Context. The Solar Orbiter spacecraft will be equipped with a wide range of remote-sensing (RS) and in-situ (IS) instruments to record novel and unprecedented measurements of the solar atmosphere and the inner heliosphere. To take full advantage of these new datasets, tools and techniques must be developed to ease multi-instrument and multi-spacecraft studies. In particular the currently inaccessible low solar corona below two solar radii can only be observed remotely. Furthermore techniques must be used to retrieve coronal plasma properties in time and in three dimensional (3D) space. Solar Orbiter will run complex observation campaigns that provide interesting opportunities to maximise the likelihood of linking IS data to their source region near the Sun. Several RS instruments can be directed to specific targets situated on the solar disk just days before data acquisition. To compare IS and RS, data we must improve our understanding of how heliospheric probes magnetically connect to the solar disk. Aims. The aim of the present paper is to briefly review how the current modelling of the Sun and its atmosphere can support Solar Orbiter science. We describe the results of a community-led effort by European Space Agency (ESA)'s Modelling and Data Analysis Working Group (MADAWG) to develop different models, tools, and techniques deemed necessary to test different theories for the physical processes that may occur in the solar plasma. The focus here is on the large scales and little is described with regards to kinetic processes. To exploit future IS and RS data fully, many techniques have been adapted to model the evolving 3D solar magneto-plasma from the solar interior to the solar wind. A particular focus in the paper is placed on techniques that can estimate how Solar Orbiter will connect magnetically through the complex coronal magnetic fields to various photospheric and coronal features in support of spacecraft operations and future scientific studies. Methods. Recent missions such as STEREO, provided great opportunities for RS, IS, and multi-spacecraft studies. We summarise the achievements and highlight the challenges faced during these investigations, many of which motivated the Solar Orbiter mission. We present the new tools and techniques developed by the MADAWG to support the science operations and the analysis of the data from the many instruments on Solar Orbiter. Results. This article reviews current modelling and tool developments that ease the comparison of model results with RS and IS data made available by current and upcoming missions. It also describes the modelling strategy to support the science operations and subsequent exploitation of Solar Orbiter data in order to maximise the scientific output of the mission. Conclusions. The on-going community effort presented in this paper has provided new models and tools necessary to support mission operations as well as the science exploitation of the Solar Orbiter data. The tools and techniques will no doubt evolve significantly as we refine our proc...

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Section: Investigations On the Properties And Origin(s) Of Sepsmentioning

confidence: 95%