Conveners
Open parallel session
- David Themens (University of Birmingham)
- Adur Pastor Yabar (Institute for Solar Physics, Department of Astronomy, Stockholm University)
- Anna Morozova (University of Coimbra, IA-UC)
- Kseniia Golubenko (Oulu University)
Description
This session welcomes submissions on topics not covered under the remaining sessions. These submissions can be on any topic as long as they relate to Space Weather and Space Climate.
Interaction of Coronal Mass Ejection (CMEs) with High-Speed Streams (HSSs) could alter their plasma and magnetic field properties. The properties of the interaction should be encoded in the in situ plasma and magnetic field observations. To characterise the properties of the interaction, we analyse the in situ signatures of 30 interplanetary coronal mass ejections (ICMEs) interacting with...
Forbush decreases (FDs) are one of the very common in-situ signatures of interplanetary coronal mass ejections (ICMEs) throughout the heliosphere. These short-term reductions in the galactic cosmic ray flux are measured by ground-based instruments at Earth and Mars, as well as various spacecraft throughout the heliosphere (most recently by Solar Orbiter). We recently developed an analytical...
Due to geomagnetic dipole tilt, the solar zenith angles and the resultant ionospheric conductivities at the same geomagnetic (GM) latitude and local time are highest in the tilt direction, which are the North American sector in the northern hemisphere and the Australian-New Zealand sector in the southern hemisphere. As a result, the geomagnetic disturbances at observatories in the tilt...
One of the key aspects of the mission of the World Meteorological Organization (WMO), to facilitate worldwide cooperation on monitoring and predicting changes in weather, climate, water and other environmental conditions, is to promote globally coordinated observations and enable global exchange of observation data.
The WMO framework for these activities is called the WMO Integrated Global...
Space weather can adversely affect the operation of satellites in Earth orbit and consequently exacerbate the problem of debris generation in space. The associated effects are more probable around the peak of a solar cycle. As we approach the peak of the 25th solar cycle, we leverage on our institute’s cross-program capabilities in model-driven assessment and prediction of LEO objects’...
The Spacecraft Anomaly Resolution Knowledgebase (SPARK), developed under a NASA SBIR Phase I and built upon an US Air Force SBIR Phase II technology, includes a coupled anomaly database, a powerful analytics software package, and an intuitive user interface -- all hosted in a secure cloud-native infrastructure. It builds on past, current, and new anomaly databases (e.g., NASA SOARS and...
