A new mailing list for space scientists who use Python has been founded. Angeline Burrell writes:
In the days of yesteryear, there was a MIST forum provided for members of the MIST community to discuss things in a fashion more immediate and informal than email. It has been some years since the fabled MIST forum was a going concern, and in that time, the MIST Council has technically been in violation of the MIST Charter, which states that
MIST will provide an on-line forum to allow ongoing discussions and the formulation of ideas prior to public dissemination. This forum will be private, visible only to registered members; membership is restricted to active MIST scientists and is offered at the discretion of MIST council chair.
“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 keynote talks from Mona Kessel (NASA/GSFC) and 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, and if you would like to submit an abstract there is an online submission form. The deadline for abstract submission is 7 December 2018 (just after Autumn MIST).
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.