Space and planetary physics
Lead Research Organisation:
Imperial College London
Department Name: Dept of Physics
Abstract
We propose to carry out a broad series of research projects which will answer important questions about our solar system and the planets within it. We will also study the links between the Sun and interplanetary space through the solar wind, as well as how they affect space around the Earth. Space is filled with small amounts of hot charged particles, called a plasma, along with a magnetic field, so much of the work we do is fundamental plasma physics applied to space.
In our work we will study some fundamental processes that occur in plasmas, including the release of magnetic energy by reconnection and the acceleration of particles at shock waves. We will look at how the solar wind is created by the Sun and how it evolves towards the Earth, as well as how different monitoring locations can be used to predict conditions at Earth. We will pursue our quantitative assessment of the plasma processes and complexity at comet 67P/Churyumov-Gerasimenko, linking our models with data from the Rosetta spacecraft flying alongside. We will use data from the Cassini spacecraft as it travels closer to Saturn than ever before to learn about the giant planet's internal magnetic field. We will study the magnetic field of the smallest planet in the solar system, Mercury, as well as considering how energy is transferred from the solar wind to the giant planets and how this is different from the Earth.
These are important topics to study not just because they provide new insight into fundamental physical processes which we do not fully understand, but also because of their effects on our lives, on other areas of science and of what they tell us about our Universe. Our work on plasma physics is related to both laboratory work on the Earth as well as many astrophysical objects such as stars and the space between the galaxies. Our work on giant planets and moons helps us to better characterise the processes that occur on and around exoplanets.
In all this work we will use theoretical models and computer simulations as well as measurements from spacecraft in deep space or in orbit around planets. In many of these cases, the measurements are made by instruments that we have built here at Imperial College. Most of these measure the magnetic field in space. The magnetic field is important in all plasmas, and space is filled with plasma - but it is also important in telling us about the interiors of planets and moons. Measuring the magnetic fields in space is very difficult because they are so small, so our science is greatly helped by working closely with the engineers who design, build and run the instruments.
As part of this proposal, we will also develop the next generation of miniature magnetic field instruments, which we hope to fly on future, small missions around the Earth or other planets. This development is important so that we can take advantage of new technologies that have become available to make the smallest, lightest, lowest power and most accurate instruments possible. In this way, we lay the groundwork for the science of the future.
In our work we will study some fundamental processes that occur in plasmas, including the release of magnetic energy by reconnection and the acceleration of particles at shock waves. We will look at how the solar wind is created by the Sun and how it evolves towards the Earth, as well as how different monitoring locations can be used to predict conditions at Earth. We will pursue our quantitative assessment of the plasma processes and complexity at comet 67P/Churyumov-Gerasimenko, linking our models with data from the Rosetta spacecraft flying alongside. We will use data from the Cassini spacecraft as it travels closer to Saturn than ever before to learn about the giant planet's internal magnetic field. We will study the magnetic field of the smallest planet in the solar system, Mercury, as well as considering how energy is transferred from the solar wind to the giant planets and how this is different from the Earth.
These are important topics to study not just because they provide new insight into fundamental physical processes which we do not fully understand, but also because of their effects on our lives, on other areas of science and of what they tell us about our Universe. Our work on plasma physics is related to both laboratory work on the Earth as well as many astrophysical objects such as stars and the space between the galaxies. Our work on giant planets and moons helps us to better characterise the processes that occur on and around exoplanets.
In all this work we will use theoretical models and computer simulations as well as measurements from spacecraft in deep space or in orbit around planets. In many of these cases, the measurements are made by instruments that we have built here at Imperial College. Most of these measure the magnetic field in space. The magnetic field is important in all plasmas, and space is filled with plasma - but it is also important in telling us about the interiors of planets and moons. Measuring the magnetic fields in space is very difficult because they are so small, so our science is greatly helped by working closely with the engineers who design, build and run the instruments.
As part of this proposal, we will also develop the next generation of miniature magnetic field instruments, which we hope to fly on future, small missions around the Earth or other planets. This development is important so that we can take advantage of new technologies that have become available to make the smallest, lightest, lowest power and most accurate instruments possible. In this way, we lay the groundwork for the science of the future.
Planned Impact
In addition to academics, other beneficiaries of the proposed work include:
Policy makers: Space weather, the effect on technological systems of solar activity, has been recognised by the UK Government as a significant risk to national infrastructure resilience. Some of our proposed work (project P1.4) directly addresses the basic scientific rationale of sending a spacecraft to the L5 libration point, a possible location for a future early warning mission. In this way, basic research will ultimately inform the policy decision as to whether to support the future funding of such a mission. Our research into the underpinning processes which control space weather (projects P1.1, 1.2, 1.3, 2.3, 2.4) will in the longer term have the potential to improve forecasting accuracy by providing data that can be integrated into e.g. physics-based magnetospheric models. We actively collaborate with the UK Met Office, who are responsible in the UK for real-time space weather forecasting, as a route to apply our research outputs to this field.
Enhancing the nation's quality of life: Space is a universally engaging subject. Our work encompasses some of the most exciting areas in this most exciting of scientific endeavours: rendezvous with a comet; jets of water and organics from a moon of Saturn; the Sun's dynamic atmosphere; the giant outer planets. We actively engage with Imperial's communications team to work with the media, from press releases, print and broadcast interviews and social media to public engagement in schools, clubs, societies and large meetings in order to maximise the public impact of our work.
Enhancing the nation's wealth: our interactions with industry via our hardware programme have resulted in a licensing arrangement with a UK company and several sales of magnetometers. This license has now expired and as part of our ongoing proposed work (project P3.1) we are seeking new commercial partners within the UK: in this way, our blue skies research results in commercial benefit for UK companies. In addition, the researchers we train move on into jobs where the technical, scientific and analytic skills they have learned are applied to a wide range of fields.
Policy makers: Space weather, the effect on technological systems of solar activity, has been recognised by the UK Government as a significant risk to national infrastructure resilience. Some of our proposed work (project P1.4) directly addresses the basic scientific rationale of sending a spacecraft to the L5 libration point, a possible location for a future early warning mission. In this way, basic research will ultimately inform the policy decision as to whether to support the future funding of such a mission. Our research into the underpinning processes which control space weather (projects P1.1, 1.2, 1.3, 2.3, 2.4) will in the longer term have the potential to improve forecasting accuracy by providing data that can be integrated into e.g. physics-based magnetospheric models. We actively collaborate with the UK Met Office, who are responsible in the UK for real-time space weather forecasting, as a route to apply our research outputs to this field.
Enhancing the nation's quality of life: Space is a universally engaging subject. Our work encompasses some of the most exciting areas in this most exciting of scientific endeavours: rendezvous with a comet; jets of water and organics from a moon of Saturn; the Sun's dynamic atmosphere; the giant outer planets. We actively engage with Imperial's communications team to work with the media, from press releases, print and broadcast interviews and social media to public engagement in schools, clubs, societies and large meetings in order to maximise the public impact of our work.
Enhancing the nation's wealth: our interactions with industry via our hardware programme have resulted in a licensing arrangement with a UK company and several sales of magnetometers. This license has now expired and as part of our ongoing proposed work (project P3.1) we are seeking new commercial partners within the UK: in this way, our blue skies research results in commercial benefit for UK companies. In addition, the researchers we train move on into jobs where the technical, scientific and analytic skills they have learned are applied to a wide range of fields.
Organisations
- Imperial College London, United Kingdom (Lead Research Organisation)
- Catholic University of Louvain, Belgium (Collaboration)
- The University of Iowa, United States (Collaboration)
- Max Planck Society (Collaboration)
- University of Arizona, United States (Collaboration)
- Hungarian Academy of Sciences (MTA) (Collaboration)
- West Virginia University (Collaboration)
- Braunschweig University of Technology (Collaboration)
- University of California Los Angeles, United States (Collaboration)
- University of Michigan, United States (Collaboration)
- University of Colorado Boulder (Collaboration)
- National Aeronautics and Space Administration (NASA) (Collaboration)
- Southwest Research Institute (SWRI) (Collaboration)
- University of Leicester, United Kingdom (Collaboration)
- Johns Hopkins University, United States (Collaboration)
Publications

Wilder F
(2016)
Observations of large-amplitude, parallel, electrostatic waves associated with the Kelvin-Helmholtz instability by the magnetospheric multiscale mission KELVIN-HELMHOLTZ ELECTROSTATIC WAVES
in Geophysical Research Letters

Eriksson S
(2016)
Magnetospheric Multiscale Observations of the Electron Diffusion Region of Large Guide Field Magnetic Reconnection.
in Physical review letters

Fuselier S
(2016)
Ion chemistry in the coma of comet 67P near perihelion
in Monthly Notices of the Royal Astronomical Society

Mallet A
(2016)
Measures of three-dimensional anisotropy and intermittency in strong Alfvénic turbulence
in Monthly Notices of the Royal Astronomical Society

Broiles T
(2016)
Characterizing cometary electrons with kappa distributions
in Journal of Geophysical Research: Space Physics

Stawarz J
(2016)
Observations of turbulence in a Kelvin-Helmholtz event on 8 September 2015 by the Magnetospheric Multiscale mission OBSERVATIONS OF TURBULENCE BY MMS
in Journal of Geophysical Research: Space Physics

Mandt K
(2016)
RPC observation of the development and evolution of plasma interaction boundaries at 67P/Churyumov-Gerasimenko
in Monthly Notices of the Royal Astronomical Society

Ergun R
(2016)
Magnetospheric Multiscale observations of large-amplitude, parallel, electrostatic waves associated with magnetic reconnection at the magnetopause Waves Associated With Reconnection
in Geophysical Research Letters

Arridge C
(2016)
Cassini observations of Saturn's southern polar cusp
in Journal of Geophysical Research: Space Physics

Wilder F
(2016)
Observations of whistler mode waves with nonlinear parallel electric fields near the dayside magnetic reconnection separatrix by the Magnetospheric Multiscale mission
in Geophysical Research Letters


Vigren E
(2016)
SUPRATHERMAL ELECTRONS IN TITAN'S SUNLIT IONOSPHERE: MODEL-OBSERVATION COMPARISONS
in The Astrophysical Journal

Hunt G
(2016)
Field-aligned currents in Saturn's magnetosphere: Local time dependence of southern summer currents in the dawn sector between midnight and noon
in Journal of Geophysical Research: Space Physics

Lai H
(2016)
Transport of magnetic flux and mass in Saturn's inner magnetosphere
in Journal of Geophysical Research: Space Physics

Vigren E
(2016)
MODEL-OBSERVATION COMPARISONS OF ELECTRON NUMBER DENSITIES IN THE COMA OF 67P/CHURYUMOV-GERASIMENKO DURING 2015 JANUARY
in The Astronomical Journal

Masters A
(2016)
SUPRATHERMAL ELECTRONS AT SATURN'S BOW SHOCK
in The Astrophysical Journal

Galand M
(2016)
Ionospheric plasma of comet 67P probed by Rosetta at 3 au from the Sun
in Monthly Notices of the Royal Astronomical Society

Franci L
(2016)
PLASMA BETA DEPENDENCE OF THE ION-SCALE SPECTRAL BREAK OF SOLAR WIND TURBULENCE: HIGH-RESOLUTION 2D HYBRID SIMULATIONS
in The Astrophysical Journal


Mejnertsen L
(2016)
Global MHD simulations of Neptune's magnetosphere
in Journal of Geophysical Research: Space Physics

Provan G
(2016)
Planetary period oscillations in Saturn's magnetosphere: Coalescence and reversal of northern and southern periods in late northern spring
in Journal of Geophysical Research: Space Physics

Russell C
(2016)
Ion cyclotron waves at Titan
in Journal of Geophysical Research: Space Physics

Stansby D
(2016)
EXPERIMENTAL DETERMINATION OF WHISTLER WAVE DISPERSION RELATION IN THE SOLAR WIND
in The Astrophysical Journal

Ergun RE
(2016)
Magnetospheric Multiscale Satellites Observations of Parallel Electric Fields Associated with Magnetic Reconnection.
in Physical review letters

Øieroset M
(2016)
MMS observations of large guide field symmetric reconnection between colliding reconnection jets at the center of a magnetic flux rope at the magnetopause
in Geophysical Research Letters
Description | We made progress in several areas of space and planetary science which have important implications for how we under space plasmas and the ways that planets, monos and comets interact with their environments. We published ground-breaking results about magnetic reconnection, which controls how the Earth's magnetosphere stores and releases energy, and the way in which the solar wind interacts with the magnetosphere. We used data from Magnetospheric Multiscale to shed new light on the processes controlling reconnection which has stimulated considerable further research and discovery [Burch et al., Science, 2016; Torbert et al., Science, 2019]. We also used MMS to discover the existence of small-scale electron-only reconnection, which has opened up a new area of space physics research at the interface between turbulence and reconnection [Phan et al., Nature, 2028; Stawarz et al., Ap. J. 2019; Gingell et al., GRL, 2019]. We studied the magnetic field of Saturn. The unexpected confirmation of Saturn's extremely small dipole tilt, requires a rethink of the planetary dynamo process (Dougherty et al., 2018); can be described if there are 2 dynamos, the usual deep one which generates the planetary field with its usual dipole tilt and then a shallower one that masks the tilt effect (Hao et al., 2020). We studied measurements of the solar wind near the Sun. We discovered (Horbury et al., 2018) a class of events, now called "switchbacks," which last only a few minutes but can reach 1000 km/s in speed. These have proved to be very common near to the Sun and are now recognised as a fundamental aspect of the solar wind flow. We studied the physics of how comets interact with the solar wind using a combination of modelling and data form the Rosetta spacecraft. We saw how competing processes, such as solar radiation and the impact of the solar wind, can change the ionisation rates of gas emanating from comets, and the dynamics of how that material is carried away from the comet. |
Exploitation Route | Our results on reconnection and switchbacks help us to understand how the solar wind is produced, how it evolves and how it interacts with the Earth's magnetic field; these, collectively, can drive "space weather" which can impact satellites and ground-based assets. In this way, our work helps to underpin the science behind future space weather predictions. Beyond this, our work informs the research of other groups worldwide and many of our published papers are highly cited in the field. |
Sectors | Aerospace, Defence and Marine |
Title | Helios ion data re-analysis |
Description | A full re-analysis of proton core measurement by the Helios spacecraft, 1974-1986 |
Type Of Material | Database/Collection of data |
Year Produced | 2017 |
Provided To Others? | Yes |
Impact | Used in multiple scientific papers. |
URL | http://helios-data.ssl.berkeley.edu/data/E1_experiment/New_proton_corefit_data_2017/cdf/ |
Description | Cassini Magnetometer Team |
Organisation | Braunschweig University of Technology |
Country | Germany |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | Hungarian Academy of Sciences (MTA) |
Department | Wigner Research Centre for Physics |
Country | Hungary |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | Johns Hopkins University |
Department | Applied Physics Laboratory (APL) |
Country | United States |
Sector | Charity/Non Profit |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | Max Planck Society |
Department | Max Planck Institute for Nuclear Physics |
Country | Germany |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | Max Planck Society |
Department | Max Planck Institute for Solar System Research |
Country | Germany |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | National Aeronautics and Space Administration (NASA) |
Department | Goddard Space Flight Center |
Country | United States |
Sector | Public |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | National Aeronautics and Space Administration (NASA) |
Department | Jet Propulsion Laboratory |
Country | United States |
Sector | Public |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | Southwest Research Institute (SwRI) |
Department | Space Research |
Country | United States |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | University of Arizona |
Department | Lunar and Planetary Laboratory |
Country | United States |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | University of California, Los Angeles (UCLA) |
Country | United States |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | University of Colorado Boulder |
Department | Laboratory for Atmospheric and Space Physics (LASP) |
Country | United States |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | University of Iowa |
Country | United States |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | University of Leicester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Cassini Magnetometer Team |
Organisation | University of Michigan |
Department | Space Research Building (SRB) |
Country | United States |
Sector | Academic/University |
PI Contribution | I am the Principal Investigator of the Cassini Magnetometer Team |
Collaborator Contribution | helped to build the instruments, and science collaboration |
Impact | Numerous high profile research papers based on Cassini data, and a working instrument still flying on Cassini |
Description | Reconnection Goldman |
Organisation | Catholic University of Louvain |
Country | Belgium |
Sector | Academic/University |
PI Contribution | Spacecraft data analysis of magnetic reconnection |
Collaborator Contribution | Performance of computer simulations and subsequent data analysis of magnetic reconnection |
Impact | Carr et al., Phys. Plasmas, 2013, Goldman et al., Phys. Rev. Lett., 2014 Eastwood et al., J. Geophys. Res., 2015 Innocenti et al., Geophys. Res. Lett., 2017 Goldman et al., J. Geophys. Res., 2020 Eastwood et al., Phys. Rev. Lett., 2020 Goldman et al. Phys. Plasmas, 2021 Multi-disciplinary - space science and laboratory plasma physics |
Start Year | 2011 |
Description | Reconnection Goldman |
Organisation | University of Colorado Boulder |
Country | United States |
Sector | Academic/University |
PI Contribution | Spacecraft data analysis of magnetic reconnection |
Collaborator Contribution | Performance of computer simulations and subsequent data analysis of magnetic reconnection |
Impact | Carr et al., Phys. Plasmas, 2013, Goldman et al., Phys. Rev. Lett., 2014 Eastwood et al., J. Geophys. Res., 2015 Innocenti et al., Geophys. Res. Lett., 2017 Goldman et al., J. Geophys. Res., 2020 Eastwood et al., Phys. Rev. Lett., 2020 Goldman et al. Phys. Plasmas, 2021 Multi-disciplinary - space science and laboratory plasma physics |
Start Year | 2011 |
Description | Reconnection Goldman |
Organisation | West Virginia University |
Country | United States |
Sector | Academic/University |
PI Contribution | Spacecraft data analysis of magnetic reconnection |
Collaborator Contribution | Performance of computer simulations and subsequent data analysis of magnetic reconnection |
Impact | Carr et al., Phys. Plasmas, 2013, Goldman et al., Phys. Rev. Lett., 2014 Eastwood et al., J. Geophys. Res., 2015 Innocenti et al., Geophys. Res. Lett., 2017 Goldman et al., J. Geophys. Res., 2020 Eastwood et al., Phys. Rev. Lett., 2020 Goldman et al. Phys. Plasmas, 2021 Multi-disciplinary - space science and laboratory plasma physics |
Start Year | 2011 |
Title | HelioPhy - software for heliophysics research |
Description | Public software in Python which faciliates downloading and analysis of data in heliosphysic physics. |
Type Of Technology | Software |
Year Produced | 2018 |
Open Source License? | Yes |
Impact | Used in several papers |
URL | https://docs.heliopy.org/en/stable/index.html |
Title | QSAS - Science Analysis Software for Space Plasmas |
Description | Analysis and display software targeted at space physics data. See documentation at https://qsas.sourceforge.io/QSAShelp/QSAS_help_index.html Features Optimised for Space Physics data Multi-spacecraft and Multi-instrument analysis Extensible through plugins Robust Analysis and Plotting Graphical Calculator interface Import/Export data in various formats Save/Restore Sessions, calculations and plot designs Understands units, coordinate frames Join performed on the fly Nanosecond accuracy with leap seconds |
Type Of Technology | Software |
Year Produced | 2019 |
Open Source License? | Yes |
Impact | QSAS is used in the analysis of data form multiple space missions, including Cluster, MMS and Rosetta. |
URL | https://sourceforge.net/projects/qsas/ |
Description | , "Hold a comet in your hand", Imperial Fringe: A Space Odyssey |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Public/other audiences |
Results and Impact | Demonstrated in front of the public how to make a comet with supporting material, posters and slide show to illustrate Rosetta achievements and scientific outcomes. Experiment redone 5 times, each time about 20-30 people watched, asked questions and interacted with us. In addition, we interacted with the public through informal chats and supporting material between the experiments with smaller groups (2-5 people for each of us at a given time). It took place in the premises of Imperial College London one evening. The attendance included the general public as well as high school kids, undergraduate and graduated students. |
Year(s) Of Engagement Activity | 2017 |
Description | BBC Sky at Night feature |
Form Of Engagement Activity | A broadcast e.g. TV/radio/film/podcast (other than news/press) |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Public/other audiences |
Results and Impact | BBC Sky at Night broadcast, subject the Sun, featured Solar Orbiter and had extended interview with Tim Horbury and discussion of the science and engineering of the Solar Orbiter magnetometer, built at Imperial College. |
Year(s) Of Engagement Activity | 2018 |
URL | https://www.bbc.co.uk/programmes/p06hbgkf |
Description | Exhibit at the Royal Society Summer Science Exhibition (London, 2016) |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | As part of the Royal Society Summer Exhibition, we co-organised an exhibit about "A comet revealed" in order to introduce the ESA/Rosetta mission to the public and share with them the exciting, science findings. The whole week we were present to interact with the public, students and pupils. Some had already heard about the mission and were not aware of the motivation behind and outcomes, others did not know anything about it. All enjoyed "smelling" a comet and were very excited to learn more about space exploration. Many mentioned that they would keep informed about it and were keen to check the weblink we passed on to obtain further insights. |
Year(s) Of Engagement Activity | 2016 |
URL | https://royalsociety.org/science-events-and-lectures/2016/summer-science-exhibition/exhibits/rosetta... |
Description | Multiple interviews on national TV (Sky, BBC World, BBC News at 10pm) |
Form Of Engagement Activity | A press release, press conference or response to a media enquiry/interview |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Multiple interviews with media during launch activities for NASA's Parker Solar Probe mission. |
Year(s) Of Engagement Activity | 2018 |
Description | NY Times Interview |
Form Of Engagement Activity | A press release, press conference or response to a media enquiry/interview |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Interviewed for an article in the New York Times about space weather. |
Year(s) Of Engagement Activity | 2019 |
URL | https://www.nytimes.com/2019/02/06/science/northern-lights-southern-lights.html |
Description | National Geographic (2018) |
Form Of Engagement Activity | A magazine, newsletter or online publication |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Interviewed for an article in National Geographic relating to space weather. |
Year(s) Of Engagement Activity | 2018 |
URL | https://www.nationalgeographic.com/science/2018/11/why-space-weather-is-being-made-in-lab-solar-wind... |
Description | Newsweek (2018) |
Form Of Engagement Activity | A magazine, newsletter or online publication |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Quoted in article reporting work published as a result of the funded research. |
Year(s) Of Engagement Activity | 2018 |
URL | http://www.newsweek.com/nasa-discovers-strange-new-magnetic-phenomenon-earths-turbulent-outer-922012 |
Description | Pint of Science (2018) |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Public/other audiences |
Results and Impact | Science communication event as part of Pint of Science to ~80 audience members. |
Year(s) Of Engagement Activity | 2018 |
URL | https://pintofscience.co.uk/event/hazards-from-space-to-core |
Description | School visit (Sutton) |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Schools |
Results and Impact | Attended a school to talk to year 5 pupils about space science. Teachers reported that it was very interesting and timely based on the work they had been doing in the curriculum. |
Year(s) Of Engagement Activity | 2019 |
Description | The Royal Institution Discourse |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Presentation by Prof. Michele Dougherty at the Royal Insitution. |
Year(s) Of Engagement Activity | 2018 |