A Royal Astronomical Society discussion meeting entitled Transitioning Research and Instrument Expertise in Heliophysics into Space Weather Monitoring Capabilities at L1 and L5 is to be held at Burlington House on 8 March, convened by Richard Harrison (STFC), Jackie Davies (STFC), and Jonny Rae (MSSL). This meeting specifically targets the exploitation of our research and instrumentation for space weather applications, in particular, associated with the ESA Lagrange mission and the associated NASA L1 mission. The RAS page for the meeting is here, and the programme is available here.
The online abstract submission system for the 2019 Royal Astronomical Society National Astronomy Meeting is now open. The deadline for abstract submissions is 15 March and abstracts can be submitted through the NAM 2019 website.
NAM 2019 will be held at Lancaster University between 30 June–4 July. Further information and a full list of parallel sessions is available on the event website. Additional practical information will be added to the site prior to registration opening on Mon 25 February, and it is not necessary to register to submit an abstract.
Further to the initial announcement, more details are now available on the 2019 International EISCAT Symposium. It will be held alongside the 46th Annual European Meeting on Atmospheric Studies (46AM) at the University of Oulu, Finland, from 19–23 August 2019.
The joint meeting will be immediately preceded by the International EISCAT Incoherent Scatter Radar School, at Pikku Syote (150 km east of Oulu), from 12–17 August 2019.
Registration information for both meetings will be published in February, but in the meantime, please visit the EISCAT Symposium and 46AM webpage and the EISCAT Radar School webpage for more information.
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).