The STFC Solar System Advisory Panel (SSAP) is undertaking a review of the "Roadmap for Solar System Research", to be presented to STFC Science Board later this year. This is expected to be a substantial update of the Roadmap, as the last full review was carried out in 2012, with a light-touch update in 2015.
The current version of the SSAP Roadmap can be found here.
In carrying out this review, we will take into account changes in the international landscape, and advances in instrumentation, technology, theory, and modelling work.
As such, we solicit your input and comments on the existing roadmap and any material we should consider in this revision. This consultation will close on Wednesday 14 July 2021 and SSAP will try to give a preliminary assessment of findings at NAM.
This consultation is seeking the view of all members of our community and we particularly encourage early career researchers to respond. Specifically, we invite:
Short "white papers" on science investigations (including space missions, ground-based experimental facilities, or computing infrastructure) and impact and knowledge exchange (e.g. societal and community impact, technology development). Please use the pro-forma sent to the MIST mailing list and send your response to This email address is being protected from spambots. You need JavaScript enabled to view it..
The Dublin Institute of Advanced Studies (DIAS) will be hosting a seminar by Jesper Gjerloev, Sam Yee, and the entire EZIE Team on 2 June at 3pm (Dublin). Jesper will give an overview of the EZIE mission to study Earth's auroral electrojets. The title and abstract are below; the Zoom link can be found on the MIST mailing list.
EZIE will image the magnetic signature of the ionospheric electrojets using the Zeeman splitting of the O2 thermal emissions originating from around 80km altitude. EZIE’s 3 smallsats each carry a microwave electrojet magnetogram (MEM) instrument for multipoint vector magnetic field measurements proximate to the source current thereby revealing the structure and evolution of the electrojets. In situ measurements of the electrojet region have proved elusive because the altitudes are too high for balloons and too low for satellites. EZIE’s multi-point measurements will provide unprecedented 2D current maps allowing for a separation of spatial and temporal variations of the electrojets.
EZIE will address two primary science questions that have remained elusive because of observation limitations:
EZIE’s science augmentation characterizes the spatiotemporal structure of equatorial electrojets and explores the physical mechanisms of their generation, resulting in EZIE’s third science question:
The presentation will provide an overview of the mission with a focus on science and implementation. We will show results from comprehensive and realistic end-to-end simulations to illustrate the unprecedented observational capabilities of the EZIE mission.
This year’s STFC summer school is provisionally planned to be held in person at Durham University from 22–27 August. However, if the government’s easing of restrictions between now and then changes so that an in-person meeting is not deemed sensible, then the school will instead be held online. The final decision on this will be made by 30 June.
For more information, visit the website for the summer school.
The summer school is intended as an introduction to solar physics and solar-terrestrial interactions, aimed at PhD students starting in Autumn 2021. The five-day course will consist of a number of lectures delivered by experts from across the UK. The lectures will cover a range of topics, from a general introduction to Plasma Physics to more specialised areas such as magnetic topology.
The preliminary programme is currently available. In addition to the core lectures there will be a careers Q&A, a session on surviving a PhD, an interactive introduction to Python/SunPy and a conference dinner on the Thursday evening. Accommodation for students during the week will be in one of Durham's colleges.