Name: STCE Annual Meeting
Start: 2024-06-27T09:30:00+02:00
End: 2024-06-27T14:40:00+02:00
Location: Royal Meteorological Institute

STCE Annual Meeting

Thursday, 27 June 2024 - 09:30

Monday, 24 June 2024
Tuesday, 25 June 2024
Wednesday, 26 June 2024
Thursday, 27 June 2024

09:30 Arrival with coffee and tea
Arrival with coffee and tea
09:30 - 10:00
Room: Director's house, room Stratus
10:00 Welcome to the attendees and special guests from Belgian defence. - Ronald Van der Linden
Welcome to the attendees and special guests from Belgian defence.
- Ronald Van der Linden
10:00 - 10:10
Room: Director's house, room Stratus We welcome Dries Van Baelen, radio engineer and Emilien Juckler from MeteoWing, both at Belgian defence.
10:10 Assessing long-term changes in stratospheric water vapour observed from space - Daan Hubert (BIRA-IASB)
Assessing long-term changes in stratospheric water vapour observed from space
- Daan Hubert (BIRA-IASB)
10:10 - 10:20
Room: Director's house, room Stratus Changes in water vapour have an impact on surface climate, but are not well constrained due to differences between observations. In this study we quantify and compare variability and long-term changes in three merged satellite Climate Data Records of vertically resolved water vapour in the stratosphere.
10:20 ICME impact on plasma turbulence and complexity at Venus, Earth and Mars. - Marius Echim (IASB)
ICME impact on plasma turbulence and complexity at Venus, Earth and Mars.
- Marius Echim (IASB)
10:20 - 10:30
Room: Director's house, room Stratus We investigate the effects of ICME on the properties of turbulence and intermittency detected in the magnetosheath of Venus and Mars and compare with properties detected in the Earth’s magnetosheath when impacted by the same interplanetary event. We select two Interplanetary Coronal Mass Ejection (ICME) events, one in January 2009 which hit Venus and Earth and the second one in 2018 which hit Earth and Mars. We use magnetic field and plasma data provided by Venus Express, Cluster and MAVEN on which we apply a full set of analysis methods including computation of Power Spectral Density (PSD), Probability Density Functions (PDFs) and the flatness. We compare the spectral index and the intermittent range of scales (where we observe scale dependent/increasing flatness) obtained for the non-magnetized planets with the same turbulence descriptors obtained for the Earth. We also compare planetary magnetosheath turbulence and intermittency properties observed during space weather events with quiet times results, for each planetary system.
10:30 Mother's Day Storm - part 1
Mother's Day Storm - part 1
10:30 - 11:30
Room: Director's house, room Stratus Sabrina, David, Marie, Christophe, Antonio - Solar Observations Viviane, Tobias, Hervé, Dani - Near Earth Observations Erwin, Nicolas, Jean-Marie, Yana - Sources of Space Weather Impacts Dries - Impacts in HF operations seen by users

11:30 Break
Break
11:30 - 11:45
Room: Director's house, room Stratus

11:45 Mother's Day Storm, part 2
Mother's Day Storm, part 2
11:45 - 12:45
Room: Director's house, room Stratus Sabrina, David, Marie, Christophe, Antonio - Solar Observations Viviane, Tobias, Hervé, Dani - Near Earth Observations Erwin, Nicolas, Jean-Marie, Yana - Sources of Space Weather Impacts Dries - Impacts in HF operations seen by users
12:45 STCE structure & future - Ronald Van der Linden
STCE structure & future
- Ronald Van der Linden
12:45 - 13:00
Room: Director's house, room Stratus
13:00 Announcement STCE 20 years
Announcement STCE 20 years
13:00 - 13:05
Room: Director's house, room Stratus

13:05 Lunch: veggie sandwiches + lactose-free salad
Lunch: veggie sandwiches + lactose-free salad
13:05 - 14:00
Room: Director's house, room Stratus