The Global Response of the Terrestrial Magnetosphere During Storms and Substorms is an upcoming RAS discussion meeting to be held on 08 February 2019 at the Royal Astronomical Society at Burlington House. This meeting will include an invited talk from Elena Kronberg (Max-Planck Institute for Solar System Research).
If you are interested in attending, you can visit the page for the meeting on the RAS's website. The programme and list of abstracts are available here on the MIST website.
The meeting is co-convened by Jasmine Sandhu (MSSL/UCL), Hayley Allison (BAS/Cambridge), Maria-Theresia Walach (Lancaster) and Clare Watt (Reading), and the the description of the meeting is as follows:
The magnetosphere is a highly variable environment, and the occurrence of storms and substorms result in the dramatic reconfiguration and redistribution of energy within the system. Understanding the conditions under which these events take place, the response of the magnetosphere, and the causes of the high variability observed is an area of active research.
This meeting aims to further our understanding of how internal and external factors combine to shape the global structure of the magnetosphere and the plasma stored therein during active times. We aim to integrate our collective knowledge of global changes in the magnetic field structure and of plasma behaviour across a wide range of energies, from cold plasmaspheric plasma through to the high energy populations in the plasma sheet, ring current, and outer radiation belt. In addition to bringing together observations from throughout the magnetosphere and ionosphere (e.g., Van Allen, Cluster, and the SuperDARN network), new modelling and simulation results will also provide insight into the response of the terrestrial magnetosphere to a wide range of geomagnetic activity.
There is a scientific discussion meeting to be held at the Royal Society on 21–22 January 2018, organised by Professor Jonathan Tennyson FRS, Professor Benjamin McCall, and Professor Steven Miller. The webpage for the meeting is available on the Royal Society's website.
This meeting will highlight recent developments in theoretical, laboratory and astronomical studies of the molecular ion H3+ and its hydrogenated cousin H5+. These developments include the first models of H5+, high-resolution studies of H3+ deuterated isotopologues, ultra-cold chemistry studies, new chemical models of the Galactic Centre, and data from the space missions Cassini (Saturn) and JUNO (Jupiter).