MIST

Magnetosphere, Ionosphere and Solar-Terrestrial

Latest news

STFC Public Engagement Early-Career Researcher (PEER) Forum

The STFC has issued a call for applications to join their Public Engagement Early-Career Researcher (PEER) Forum, which is designed to support talented scientists and engineers in the early stages of their career in developing their public engagement and outreach goals. This forum is geared towards PhD students and early-career postdocs developing ideas for public engagement with similarly-minded researchers in a context that allows them to feed suggestions for the improvement of STFC's programmes back to STFC itself, and involves meeting twice a year. The deadline for applications is 4pm on 3 June 2019. For more information and more detail on what the scheme involves, you can visit the PEER Forum webpage or This email address is being protected from spambots. You need JavaScript enabled to view it..

The aims of the PEER Forum are as follows:

  • To foster peer learning and peer support between early career scientists and engineers with a passion for public engagement and outreach.
  • To improve understanding of the support STFC provides for public engagement and outreach (including funding mechanisms, evaluation, and reporting) and how to successfully utilise this support.
  • To stimulate discussions that help to develop and influence STFC’s approaches to public engagement.

ESA Science Programme Committee greenlights SMILE

The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) has been given the green light for implementation by ESA's Science Programme Committee. SMILE will explore the Sun-Earth connection in a very novel way, by mapping solar wind-magnetosphere interactions in soft X-rays. SMILE is a joint mission by ESA and the Chinese Academy of Sciences (CSA). The UK is one of many countries contributing to the payload development.

The SMILE payload comprises four instruments: a soft X-ray imager (SXI), a UV auroral imager (UVI) and an in situ measurement package composed of a light ion analyser and a magnetometer. The UK leads SXI, Canada leads UVI, and China leads the ion analyser and magnetometer. SMILE will fly in a highly elliptical polar orbit with an apogee of 20 Earth radii to image the magnetosphere and the Northern Lights for more than 40 hours continuously per orbit. The launch is planned in November 2023.

For more information, visit the European Space Agency, the Chinese Academy of Sciences, or Mullard Space Science Laboratory.

Debye mission proposal for ESA F-class call

We are currently preparing a proposal for the space mission “Debye” in response to ESA’s F-Class call. As the first dedicated electron-astrophysics mission, Debye will use the solar wind as a testbed to study universal small-scale electron processes throughout the universe. The mission's key science question is: “How are electrons heated in astrophysical plasmas?”
 
Debye will consist of up to four spacecraft that will orbit the Lagrange point L2. The main spacecraft will measure electron distribution functions with unprecedented cadence and very high resolution, electric fields, magnetic fields, and plasma ions. The deployable spacecraft will provide multi-point and multi-baseline measurements of the magnetic field to determine the nature of fluctuations on electron scales.
 
Read more ...

RAS Specialist Discussion suggestions invited

The RAS is inviting suggestions from Fellows of the RAS for Specialist Discussion meeting topics in the academic year 2019/20. These meetings are held on the second Friday of the month between October and May in a given academic year; the April meeting will be moved due to the second Friday being Good Friday. 

If you would like to organise one of these meetings, you can do so by submitting a proposal no longer than one A4 page. Geophysics proposals, including MIST science, should be sent to This email address is being protected from spambots. You need JavaScript enabled to view it., and the deadline is 1 March 2019.

Your proposal should include the title of the meeting; the names of the co-convenors (at least one of whom should be a RAS Fellow); the topics you intend to cover; the rationale (including timeliness); suggestions for invited speakers; and the preferred date for the meeting. More information, including detailed guidance, can be found on the RAS website.

 

RAS awards for 2019 announced

MIST Council would like to extend their congratulations to the 2019 Royal Astronomical Society award winners, as well as the recent AGU award winners. In particular, we congratulate the following MIST members recognised for their significant achievements:
  • Margaret Kivelson (UCLA) has been awarded the Gold Medal in Geophysics for a lifetime of outstanding achievement in understanding planetary magnetospheres and their connections to the planets they surround.
  • Tom Stallard (Leicester) has been awarded the Chapman medal in Geophysics for outstanding contributions to understanding planetary upper atmospheres and their interactions with their magnetospheres.
  • The Cluster Science and Operations Team have been awarded the Geophysics Group Award for their continued success ensuring the operations and scientific exploitation of the European Space Agency’s Cluster mission.
  • Mark Clilverd (British Antarctic Survey) has been awarded the James Dungey Lecture for their excellent research on energetic particle precipitation and its effects on the upper atmosphere and climate, and their vast experience delivering outstanding scientific talks to a broad range of audiences.
  • Julia Stawarz (Imperial College London) has been awarded the Basu United States Early Career Award for Research Excellence in Sun-Earth Systems Science for significant contributions in furthering understanding of collisional plasma turbulence and kinetic scale processes. 
MIST Council would also like to congratulate Fran Bagenal (Colorado), who has been awarded the AGU Van Allen Lecture for exceptional work on the understanding of planetary magnetospheres and outstanding contributions to planetary missions.

List of seminar speakers

The following is a list of people who have registered their interest in giving seminars on their research interests at other institutions. The aims of this list are:

  1. To improve the visibility, and awareness, of the work done by different researchers and research groups.
  2. To assist local organisers of regular institutional seminar series with suggestions for speakers, particularly PhD students and postdocs who may be less widely known in the community.
  3. To assist the science organising committees of conferences and meetings, as above.

If you would like to appear on the below list or you would like to edit the details that appear on this page, please fill in this google form. We note that there is no obligation for the people listed below to accept invitations extended by MIST institutions. The list is also available in this spreadsheet.

 (Last updated on 25 February 2019.)

Speakers

  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Numerical experiments of wave-particle interactions in the inner magnetosphere; basic theory of collisionless plasma equilibria and stability (current sheets and flux tubes).
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Dayside magnetospheric dynamics at Earth; transient kinetic phenomena in the foreshock, bow shock and magnetosheath; magnetospheric ULF waves and resonances; magnetospheric variability; novel analysis techniques; sonification of data; public engagement.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — high latitude thermosphere-ionopshere coupling (mainly the effects of ion drag and the timescales on which it acts); the resultant Joule heating; its variations due to multiple criteria (aurora/neutral winds).
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Machine learning; solar wind; radiation belts; space weather; big data techniques.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Interactions with the ionosphere; radar observations; satellite observations; community programming.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Type II solar radio burst band-splitting.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Birkeland currents (aka field-aligned currents); AMPERE observations; substorms; flux transfer events (FTEs); northward IMF.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Heliospheric physics; evolution of coronal mass ejections (CMEs); magnetic clouds; solar wind; solar transients.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Magnetospheric physics; ionospheric physics; space weather; magnetic reconnection; magnetohydrodynamics (MHD); computer simulations
  • This email address is being protected from spambots. You need JavaScript enabled to view it. Field-aligned currents; the Jovian magnetodisc.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Ionosphere; magnetosphere; solar quiet currents; equatorial electrojets; geomagnetic field.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Mars plasma system, ionosphere, space weather.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. Substorms; ring current energisation; Van Allen observations; field line eigenfrequencies.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Electrical current systems of the magnetosphere (field-aligned currents); dynamics of the terrestrial magnetosphere; sub-auroral polarization streams (SAPS); magnetospheric and ionospheric convection.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Solar wind-magnetosphere-ionosphere-thermosphere coupling; response time-scales to solar wind driving; SuperDARN observations; auroral observations.
  • This email address is being protected from spambots. You need JavaScript enabled to view it. — Heliospheric physics; solar wind; plasma turbulence; collisionless heating; non-linear plasma physics; kinetic physics; micro-instabilities; statistical data analysis; hybrid/particle-in-cell simulations.