Posters

ST1.3

The solar wind is an uninterrupted flow of highly ionised plasma that fills interplanetary space and is crossed by strong transient perturbations such as coronal mass ejections (CMEs). These phenomena, in addition to corotating density structures and solar energetic particles (SEPs), drive a large range of disturbances to planetary atmospheres. Their properties and arrival times are, however, difficult to predict with reasonable accuracy. Observations from multiple vantage points, in-situ measurements from multiple positions and modelling efforts have been employed systematically to study the properties of the solar wind plasma and of CMEs, from their formation to their arrival at Earth and at planets throughout the inner heliosphere.

The recently launched Parker Solar Probe, the imminent launch of Solar Orbiter, as well as potential future missions at L1 and L5, and planetary missions that will measure the solar wind during their cruise phase (e.g. BepiColombo), will provide us with the perfect opportunity to test, validate, and refine the current knowledge of these physical phenomena and their interactions. Accordingly, the aim of this session is to showcase the latest observational and modelling efforts regarding the evolution of the solar wind and CMEs during their propagation throughout the heliosphere as seen from multiple vantage points, and to foresee future developments. Potential improvements to our current space weather forecasting capabilities will be highlighted.

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Convener: David Barnes | Co-conveners: Erika Palmerio, Rui Pinto
Orals
| Tue, 09 Apr, 16:15–18:00
 
Room 1.61
Posters
| Attendance Wed, 10 Apr, 14:00–15:45
 
Hall X4

Attendance time: Wednesday, 10 April 2019, 14:00–15:45 | Hall X4

Chairperson: Rui Pinto
X4.123 |
EGU2019-17510
A Catalogue of Coronal Mass Ejections Observed by the Heliospheric Imagers throughout the STEREO Mission
(withdrawn)
David Barnes, Jackie Davies, and Richard Harrison and the The HELCATS Team
X4.124 |
EGU2019-7373
Tanja Amerstorfer, Jürgen Hinterreiter, Christian Möstl, Jackie A. Davies, Ute V. Amerstorfer, Martin A. Reiss, Manuela Temmer, Rachel L. Bailey, and Richard A. Harrison
X4.125 |
EGU2019-3535
Iuliia Zagainova, Victor Fainshtein, Ludmila Gromova, and Sergei Gromov
X4.126 |
EGU2019-9132
Jürgen Hinterreiter, Tanja Amerstorfer, Manuela Temmer, Christian Möstl, Martin Reiss, Ute Amerstorfer, and Rachel Bailey
X4.127 |
EGU2019-9366
Jingnan Guo, Manuela Temmer, Astrid Veronig, Miho Janvier, Stefan Hofmeister, Robert Wimmer-Schweingruber, and Jasper Halekas
X4.128 |
EGU2019-9578
Manuela Temmer, Lukas Holzknecht, Mateja Dumbovic, and Bojan Vrsnak
X4.129 |
EGU2019-11158
Vratislav Krupar, Milan Maksimovic, Adam Szabo, Ondrej Santolik, and Oksana Kruparova
X4.130 |
EGU2019-11217
Oksana Kruparova, Vratislav Krupar, Jana Safrankova, Zdenek Nemecek, and Ondrej Santolik
X4.131 |
EGU2019-11873
Phillip Hess and Robin Colaninno
X4.132 |
EGU2019-17133
Athanasios Papaioannou, Anatoly Belov, Angelos Vourlidas, and Anastasios Anastasiadis
X4.133 |
EGU2019-6185
Benjamin Lynch, Erika Palmerio, Jens Pomoell, C. Richard DeVore, Maria Kazachenko, and Emilia Kilpua
X4.135 |
EGU2019-13712
Dario Del Moro, Francesco Berrilli, Alice Cristaldi, Roberta Forte, Luca Giovannelli, Gianluca Napoletano, and Ermanno Pietropaolo
X4.136 |
EGU2019-17497
Simon Good, Emilia Kilpua, Adrian LaMoury, Robert Forsyth, Jonathan Eastwood, and Christian Möstl
X4.137 |
EGU2019-1210
Dana-Camelia Talpeanu, Francesco P. Zuccarello, Emmanuel Chané, Stefaan Poedts, Elke D'Huys, Marilena Mierla, and Ilia Roussev
X4.138 |
EGU2019-3954
Matti Ala-Lahti, Emilia Kilpua, Jan Souček, Tuija Pulkkinen, and Andrew Dimmock
X4.139 |
EGU2019-8305
Johan von Forstner, Jingnan Guo, Robert F. Wimmer-Schweingruber, Manuela Temmer, Mateja Dumbović, Astrid Veronig, Christian Möstl, Donald M. Hassler, Cary J. Zeitlin, and Bent Ehresmann