Meeting the Challenges of Limited Observations for the Global Modelling of the Ionosphere-Thermosphere System

STS-41G earth observations
Credit
NASA ID: 41g-34-036
Start Date
End Date

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Earth’s ionosphere is the boundary between space and the atmosphere. It holds a special importance in models of the Ionosphere-Thermosphere (IT) System because plasma interactions with the magnetic field of the ionosphere become intertwined with the neutral dynamics of the thermosphere and atmosphere. In the context of global whole atmosphere models in particular, the IT system builds the top layer and is responsible for holding the information of solar wind-magnetosphere-ionosphere interactions. At high latitudes, the IT dynamics are driven by the solar wind and magnetospheric responses to solar wind driving, whereas at mid to low latitudes, the electric dynamo interactions and tides dominate. Modelling these interactions and dynamics is challenging, but important to the provision of the boundary conditions for modelling the entire atmosphere. These challenges are compounded by limited observations of the IT system.

The dynamics of the solar wind results in a varying degree of activity in the ionosphere, especially at high- to mid-latitudes. During a geomagnetic storm for example, the energy input into the mesosphere and thermosphere is much higher than during quiet times, which changes atmospheric composition in those regions. It is important to capture these dynamics to advance models for space and/or terrestrial weather and climate purposes. This comes with great challenges due to the varying observations available. The thermosphere, for example, is difficult to measure in-situ due to orbital constraints, and ground-based observations can be sparse due to geographical constraints and lack of vertical resolution. Furthermore, scale-sizes and cadences of observations vary drastically. This makes it difficult to infer physical interactions and build global empirical models, and so challenges model validation efforts.

The aim of this discussion meeting is to bring together modellers and observers of the IT system and the atmosphere, as well as researchers interested in advancing our modelling capabilities, to discuss recent scientific findings, modelling advances and future plans.

 

"How Data Assimilation Advances the Science and Engineering of Forecasting Near-Earth Space Environments” Tomoko Matsuo invited speaker.

 

Please submit abstracts before the 16th February using this form:  https://docs.google.com/forms/d/e/1FAIpQLSdpVTcRUJ9MfHaFuC_2RCRJ8k-cl6MzPGU5RBPIrTfGKqTmGA/viewform

This meeting will take place in person and online.

 

ORGANISERS:

Maria-Theresia Walach (Lancaster University)

Mai Mai Lam (British Antarctic Survey)

David Themens (Birmingham University)

Anasuya Aruliah (University College London)

Andrew Kavanagh (British Antarctic Survey)

 

Book a Fellows March SDM In Person or Online ticket 

Book a Non Fellows March SDM In Person or Online Ticket 

Venue Address

The Royal Astronomical Society,Burlington House

Map

51.5085763, -0.13960799999995