Modelling the acceleration, transport and loss of radiation belt electrons to protect satellites from space weather (Rad-Sat)

Lead Research Organisation: British Antarctic Survey
Department Name: Science Programmes

Abstract

Over the last 10 years the number of operational satellites in orbit has grown from 450 to more than 1300. We rely on these satellites more than ever before for a wide range of applications such as mobile phones, TV signals, internet, navigation and financial services. All these satellites must be designed to withstand the harsh radiation environment in space for a design life that can be as long as 15 years or more. Space weather events can increase electron radiation levels by five orders of magnitude in the Earth's Van Allen radiation belts causing satellite charging, disruption to satellite operations and sometimes satellite loss. For example, in 2003 it was estimated that at least 10% of all operational satellites suffered anomalies (malfunctions1) during a large space weather event known as the Halloween storm. It is therefore important to understand how and why radiation levels vary so much so that engineers and business can assess impact and develop mitigation measures. New results from the NASA Van Allen Probes and THEMIS satellite missions show that wave-particle interactions play the major role in the acceleration, transport and loss of high energy electrons and hence the variability of the radiation belts. This proposal brings together scientists from across the UK with stakeholders from the insurance and satellite services sector. We will process data from scientific satellites such as Van Allen Probes and THEMIS to obtain information on four very important type of waves known as magnetosonic waves, and radio-waves known as plasmaspheric hiss, lightning generated whistlers and transmitter waves. We will use data, theory and models to determine the properties of the waves and how they vary during space weather events. We will conduct studies to assess the acceleration, transport and loss of electrons due to each wave type using quasi-linear theory. We will use simulations to test whether nonlinear effects result in more particle acceleration and loss compared to quasi-linear theory. We will analyse compressional magnetosonic waves in the ultra-low frequency range and determine their effectiveness for transporting electrons across the magnetic field, and whether the transport is diffusive or not. We will incorporate the results of these studies into our state-of-the-art global radiation belt model to simulate known space weather events, and compare the results against data to highlight the importance of the waves and improve the model. We will also include local time effects and compare loss rates against data from the ground and other satellites to constrain the model. We will simulate extreme space weather events using our existing radiation belt model, and an MHD model so that we can assess the role of waves in the rapid formation of a radiation belt such as occurred in 1991 in less than 2 minutes. We will develop a stakeholder community consisting of space insurance, satellite operators and forecasters who will provide input to our research and who will use the results for risk assessment, anomaly resolution and operational planning. The project will deliver new processed data, a better forecasting capability and expertise that will support the UK Government assessment of severe space weather for the National Risk Register2 and the growth of the satellite industry.

1. Cannon, P, S., et al. (2013), Extreme Space Weather: Impacts on Engineered Systems and Infrastructure, Royal Academy of Engineering, London, SW1A 2WH.
2. Cabinet Office, (2012), National risk register of civil emergencies, Whitehall, London SW1A 2WH, www.cabinetoffice.gov.uk.

Planned Impact

We have identified the following non-academic users who will benefit from our research:

Space insurance

One of the outputs of our research will be a set of radiation belt models which can be used to re-create the space radiation environment for severe space weather events that damage spacecraft. In their letter of support the Atrium Space Insurance Consortium have listed 4 ways in which they will benefit, including "further information to ensure the Lloyds Realistic Disaster Scenarios are accurate and that sufficient reserves are being made to cover the potential worst case insurance losses". Space insurance may also benefit from an independent assessment of the radiation environment for anomaly resolution.

Satellite construction companies

Satellite designers must protect satellites from the harsh radiation environment in space. They use models of the radiation environment to design for the 'reasonable worst case' but there is a very large uncertainty. Our research will simulate three different types of realistic worst case events, and will provide the radiation environment for medium Earth orbit for any part of the solar cycle. Satellite designers will be able to use our results to assess the amount of shielding needed to protect satellites, particularly for electric orbit raising and medium Earth orbit where there is relatively little radiation data.

Satellite operators

Satellite operators have an interest in the safe and reliable operation of their spacecraft. Space weather events can cause satellite anomalies (malfunctions) resulting in loss of service and in some cases total satellite loss. It can also mean a delay in reaching orbit and lost revenue if an anomaly affects electric orbit raising. Our research will lead to a step-change in space weather forecasting which will provide satellite operators with space weather situation awareness. This will enable them to plan mitigating action, for example, to suspend orbit manoeuvres and software updates, to ensure more staff are available to deal with problems, to have back-up systems immediately available, and when appropriate to inform users that some services may be at risk. Satellite operators will also benefit by using the results of our case studies of particular events to help identify the cause of a satellite anomaly.

Space Weather forecasting

The UK Met Office and the European Space Agency (ESA) are developing a system of forecasting all types of space weather. Our research will include new processes into our state-of-the-art forecasting models which will enable a step-change in our forecasting capability. Subject to further agreement, the Met Office and the ESA will benefit by turning our prototype forecasting system into a fully operational system for the satellite services sector.

General public

It is widely acknowledged that space research attracts young people into Science, Technology, Engineering and Mathematics (STEM subjects). The press coverage of the UK Astronaut Tim Peak and the International Space Station, is compelling evidence of the public's interest in space research. Our dissemination activities to schools and the public will help attract young people into the STEM subjects.

Policy makers

Extreme space weather was put on the UK National Risk Register in 2012 and revised in 2014. The UK Department of Energy and Industrial Strategy (DEIS) 'owns' the risk and is developing contingency plans to mitigate the impact of severe space weather. The Department will benefit from our research which will help define scenarios for severe space weather events, and how long they may last, and will provide the radiation environment needed for further impact assessment by engineers and business. The PI (Richard Horne) is a member of the Space Environment Impacts Expert Group (SEIEG) and will be able to provide advice to Government through this Group at meetings with DEIS.

Publications

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Sandhu J (2019) A global view of storms and substorms in Astronomy & Geophysics

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Meredith N (2019) An Investigation of VLF Transmitter Wave Power in the Inner Radiation Belt and Slot Region in Journal of Geophysical Research: Space Physics

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Walton S (2021) Cross- Coherence of the Outer Radiation Belt During Storms and the Role of the Plasmapause in Journal of Geophysical Research: Space Physics

 
Title Aurora Musicalis 
Description In May 2020 we were involved in the release of an album, Aurora Musicalis, that features the unique 'sounds of space' as recorded by the VLF receiver at Halley VI, Antarctica, captured in one day combined with piano playing from Kim Cunio, also played in one day. 
Type Of Art Composition/Score 
Year Produced 2020 
Impact The music has been played on several radio stations, including Manx Radio, Resonance FM, Skylab Radio and Cambridge 105 Radio. As a result of this album I was guest speaker at an online event organised by ecoartspace, a US-based organisation serving as a platform for artists influenced by the natural world. 
URL https://soundsofspaceproject.bandcamp.com
 
Title Celestial Incantations 
Description Celestial Incantations features a wide variety of space 'sounds' and a huge musical palette, including orchestral instruments, traditional instruments and electronics. The album, which is free to hear and download from bandcamp, takes the listener on a journey from Earth to the largest definitions of cosmic time and space. It invites us to consider the vastness of space, imagining time and space in the grandest sense, and embark on a spectacular journey of sound. Starting off at Earth and moving outwards we hear compositions inspired by and featuring the 'sounds' of our planet, Mars, a comet, Jupiter, Saturn, interstellar space and a galactic pulsar. The album concludes with a track featuring the 'sound' of the merger of two black holes, as evidenced by the first observed gravitational wave, an almost unbelievable ripple in space time that Einstein doubted humans could ever capture! 
Type Of Art Composition/Score 
Year Produced 2021 
Impact 1. 41,783 track plays on bandcamp and 3026 full album downloads 2. Article in the Guardian entitled "'Chirps' in space: new album captures the sound of black holes colliding". The article included a video entitled "New album, Celestial Incantations, captures the 'sounds' of space" featuring music from the album and created by the Guardian Newspaper. This video has had 34,211 views on YouTube. 3. I led an article describing the art, music and science behind Celestial Incantations. The article, entitled "Music of the Spheres", was published as the cover articles in the February 2022 issue of Astronomy and Geophysics. 4. Music from the album has been played on number of radio stations including the Phantom Circuit (#329 & #331), Audionautic Radio (ep. 17 & ep. 20), Space is the Place Radio Show, The Magic Window, Muzak Concrete, The Dark Train (C19#70 & C19#71), and Night Tracks on BBC Radio 3 and features on four ambient compilations Ambient Spring - Orbit IV, Ambient Autumn - Orbit IV, Ambient Winter - Orbit V and Ambient Music for Ambient People: 22 Home. 
URL https://soundsofspaceproject.bandcamp.com/album/celestial-incantations
 
Description Research outputs have been used to support the UK national risk register for space weather. The results have been used to win £20 million funding from the UKRI Strategic Priorities Fund in a project now called SWIMMR. The results here were used to write the business case. The new funding was announced by the Prime Minister on 24 September 2019. See https://stfc.ukri.org/news/20m-project-to-tackle-space-weather-announced/
First Year Of Impact 2020
Sector Aerospace, Defence and Marine,Energy,Environment,Government, Democracy and Justice,Security and Diplomacy
Impact Types Policy & public services

 
Description Input to UK Risk Assessment for Space Weather
Geographic Reach Multiple continents/international 
Policy Influence Type Membership of a guideline committee
Impact Provided advice on the risk to satellites due to severe space weather. This is being used to update and suport the UK risk register. The impact is to help the Government plan and prepare for an extreme space weahter event, and develop better mitigation strategies.
 
Title BAS Radiation Belt Model 
Description The BAS radiation belt model is designed to simulate the variability of the Earth's radiation belt. It is a 3d model and is the equivalent to a global circulation model in atmopsheric physics - but applied to space. It is used as a basic research tool to understand the physical processes governing the acceleration, transport and loss of electrons in the radiation belts. It has also been applied to Jupiter and Saturn. There is a verion of the code that is used to predict the radiation belts for space weather applications. 
Type Of Material Computer model/algorithm 
Year Produced 2014 
Provided To Others? Yes  
Impact The model has been used to show how plasma waves play a major role in the formation of the Earth's radiation belts. 
URL https://www.bas.ac.uk/science/research-models/bas-radiation-belt-model-bas-rbm/
 
Title Data from the figures in 'A 30 year simulation of the outer electron radiation belt' S.A. Glauert et al., 2018 
Description These files contain the data from the figures in "A 30 year simulation of the outer electron radiation belt", S.A. Glauert, et al., Space Weather 2018. The paper describes a 30 year (1 January 1986 - 1 January 2016) reconstruction of the Earth's electron radiation belt from L*=2 to L*=6.1 (approximately geostationary orbit), for energies ranging from 100 keV to 30 MeV at L*=6.1. 
Type Of Material Database/Collection of data 
Year Produced 2018 
Provided To Others? Yes  
 
Title Effects of VLF transmitter waves on the inner belt and slot region 
Description Signals from VLF transmitters can leak from the Earth-ionosphere wave guide into the inner magnetosphere, where they propagate in the whistler mode and contribute to electron dynamics in the inner radiation belt and slot region. Observations show that the waves from each VLF transmitter are highly localised, peaking on the nightside in the vicinity of the transmitter. In this study we use ~5 years of Van Allen probe observations to construct global statistical models of the bounce-averaged pitch angle diffusion coefficients for each individual VLF transmitter, as a function of L*, Magnetic Local Time (MLT) and geographic longitude. We construct a 1D pitch-angle diffusion model with implicit longitude and MLT dependence to show that VLF transmitter waves weakly scatter electrons into the drift loss cone. We find that global averages of the wave power, determined by averaging the wave power over MLT and longitude, capture the long-term dynamics of the loss process, despite the highly localised nature of the waves in space. We use our new model to assess the role of VLF transmitters waves, hiss waves, and Coulomb collisions on electron loss in the inner radiation belt and slot region. At moderate relativistic energies, E~ keV, waves from VLF transmitters reduce electron lifetimes by an order of magnitude or more, down to the order of 200 days near the outer edge of the inner radiation belt. However, VLF transmitter waves are ineffective at removing multi-MeV electrons from either the inner radiation belt or slot region. Funding was provided by the NERC grant NE/P01738X/1. 
Type Of Material Database/Collection of data 
Year Produced 2019 
Provided To Others? Yes  
 
Title Electromagnetic ion cyclotron electron diffusion coefficients calculated from CRRES data using a new approach 
Description The data provided is the underlying data used for creating the plots in Ross et al 2020. The research leading to these results has received funding from the National Environment Research Council Highlight Topic grant NE/P01738X/1 (Rad-Sat), National Environment Research Council grant NE/R016445/1 and NE/R016038/1, and the STFC grant ST/S000496/1 
Type Of Material Database/Collection of data 
Year Produced 2020 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01366
 
Title Electromagnetic ion cyclotron electron diffusion coefficients calculated using Van Allen Probe EMFISIS data for a range of ion compositions 
Description The banded structure of Electromagnetic Ion Cyclotron (EMIC) wave spectra and their resonant interactions with radiation belt electrons depend on the cold ion composition. However, there is a great deal of uncertainty in the composition in the inner magnetosphere due to difficulties in direct flux measurements. Here we determine the sensitivity of electron diffusion by EMIC waves to the cold ion composition. The diffusion coefficients are calculated using collocated EMIC waves spectra and plasma densities observed by Van Allen Probe EMFISIS data, parameterised by Dst, using quasi-linear theory implemented in the PADIE code. Funding was provided by NERC Highlight Topic grant: NE/P01738X/1 (Rad-Sat), NERC grant: NE/V00249X/1 (Sat-Risk) and NERC grant: NE/R016038/1 
Type Of Material Database/Collection of data 
Year Produced 2022 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01654
 
Title Electron Diffusion by Magnetosonic Waves in the Earth's Radiation Belts 
Description We conduct a global survey of magnetosonic waves and compute the associated bounce and drift averaged diffusion coefficients, taking into account co-located measurements of fpe/fce, to assess the role of magnetosonic waves in radiation belt dynamics, where fpe is the plasma frequency and fce is the electron gyrofrequency.. The average magnetosonic wave intensities increase with increasing geomagnetic activity and decreasing relative frequency with the majority of the wave power in the range fcp < f < 0.3fLHR during active conditions, where fcp is the proton gyrofrequency and fLHR is the lower hybrid resonance frequency. In the region 4.0 
Type Of Material Database/Collection of data 
Year Produced 2022 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01628
 
Title Electron Electromagnetic Ion Cyclotron diffusion coefficients calculated from Van Allen Probe observations 
Description Electromagnetic Ion Cyclotron (EMIC) wave are important for the losses of ultra-relativistic electrons from the Earth's radiation belts. In this work, statistical EMIC diffusion coefficients are calculated from Van Allen Probe A observations of EMIC waves from the entire mission. The diffusion coefficient calculations include the observed L* and activity dependent distributions in plasma density and wave spectra so that the wave-particle interactions modelled are representative of those in the radiation belts. These diffusion coefficients can be included into global radiation belt simulations such as the BAS radiation belt model. The study is published in Ross et al 2021, JGR: Space Physics. Funding was provided by National Environment Research Council Highlight Topic grant NE/P01738X/1 (Rad-Sat), National Environment Research Council grant NE/R016445/1 and NE/R016038/1. 
Type Of Material Database/Collection of data 
Year Produced 2021 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01580
 
Title Evaluation of SaRIF high-energy electron reconstructions and forecasts 
Description This data is provided to comply with the AGU's data policy for the publication of Glauert et al., "Evaluation of SaRIF high-energy electron reconstructions and forecasts" in Space Weather, 2021. Each data file corresponds to a figure or table in the paper and covers the period from 1 March 2019 to 1 September 2019. The data sets are as follows: Figure 1 - SaRIF reconstructions of the >800 keV and the >2 MeV flux (in cm-2 s-1 sr-1) measured by the GOES 14 spacecraft. Figure 3 - SaRIF 24-hour forecasts of the >800 keV and the >2 MeV flux (in cm-2 s-1 sr-1) at the location of the GOES 14 spacecraft. Figure 5 - SaRIF reconstructions of the >800 keV and the >2 MeV flux (in cm-2 s-1 sr-1) measured by the GOES 14 spacecraft, with the improvements to the modelling detailed in the paper. Figure 6 - Simulated SaRIF 24-hour forecasts of the >800 keV and the >2 MeV flux (in cm-2 s-1 sr-1) at the location of the GOES 14 spacecraft, with the improvements to the modelling detailed in the paper. Table 6 - Simulated SaRIF 24-hour reconstructions and forecasts of the >800 keV and the >2 MeV flux (in cm-2 s-1 sr-1) at the location of the GOES 14 spacecraft when the outer boundary for the simulation is placed at L* = 6.6. These are the values used to produce the metrics in Table 6. This research was supported by the Natural Environment Research Council (NERC) Highlight Topic Grant NE/P01738X/1 (Rad-Sat), National and Public Good activity grant NE/R016445/1 and ESA contract 4000118861/16/D/MRP (SSA P2-SWE-XIII proto- type) 
Type Of Material Database/Collection of data 
Year Produced 2021 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01567
 
Title Global model of Whistler Mode Chorus in the Near-Equatorial Region (|?|m<18o) 
Description Whistler mode chorus is an important magnetospheric emission, playing fundamental roles in the dynamics of the Earth's outer radiation belt and the production of the Earth's diffuse and pulsating aurora. In this study we extend our existing database of whistler mode chorus by including ~3 years of data from RBSP-A and RBSP-B and an additional ~6 years of data from THEMIS A, D, and E, greatly improving the statistics and coverage in the near-equatorial region (|?|m<18o). We produce new global maps of whistler mode chorus as a function of spatial location and frequency. This work is reported in Meredith et al. [2020] and the data provided here enable reconstruction of all of the figures in the paper. The research leading to these results has received funding from the Natural Environment Research Council (NERC) Highlight Topic grant NE/P01738X/1 (Rad-Sat) and the NERC grant NE/R016038/1. Wen Li and Xiao-Chen Shen received funding from NASA grants NNX17AG07G and 80NSSC19K0845, NSF grant AGS-1847818, and the Alfred P. Sloan Research Fellowship FG-2018-10936. Jacob Bortnik received funding from NASA grants NNX14AI18G, and RBSP-ECT and EMFISIS funding provided by JHU/APL contracts 967399 and 921647 under NASA's prime contract NAS5-01072. 
Type Of Material Database/Collection of data 
Year Produced 2020 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01315
 
Title Global models of the VLF transmitter wave power in the inner radiation belt and slot region 
Description Signals from manmade VLF transmitters, used for communications with submarines, can leak into space and contribute to the dynamics of energetic electrons in the inner radiation belt and slot region. We use ~5 years of plasma wave data from the Van Allen Probe A satellite to construct new models of the observed wave power from VLF transmitters both as a function of L* and MLT and geographic location. This work is reported in Meredith et al. (2019) and the data provided here enable reconstruction of all of the figures in the paper. 
Type Of Material Database/Collection of data 
Year Produced 2019 
Provided To Others? Yes  
 
Title HOTRAY 
Description HOTRAY is a computer program that can trace the path of any type of wave through a hot magnetised plasma. It has been used successfully in the Earth's ionosphere, magnetosphere, Jupiter, Saturn, the solar wind and in lab plasmas, 
Type Of Material Computer model/algorithm 
Provided To Others? Yes  
Impact There are over 100 peer-reviewed research publications using HOTRAY, including collaborations with USA, Japan, and Europe. 
URL https://www.bas.ac.uk/science/research-models/hotray-ray-tracing-model/
 
Title PADIE code 
Description The PADIE code is designed to compute the pitch angle and energy diffusion co-efficients due to the interaction between plasma waves and high energy charged particles in space - in particualr the radiation belts of Earth, Jupiter and Saturn. 
Type Of Material Computer model/algorithm 
Provided To Others? No  
Impact It has been used in many peer reviewed research papers to show how different types of plasma waves can cause acceleration and loss of high energy electrons and protons in space. 
URL https://www.bas.ac.uk/science/research-models/padie-pitch-angle-diffusion-of-ions-and-electrons/
 
Title Pitch angle diffusion coefficients used to calculate electron precipitation from the Earth's radiation belts 
Description This dataset contains two NetCDF files: Chorus_daa.nc (labelled from here as a) which contains the chorus pitch angle diffusion coefficients presented in Figure 1 of Reidy et al (2020) and Combined_daa.nc (labelled from here as b) containing the combined pitch angle diffusion coefficients which can be used to do the analysis presented in the remainder of the Reidy et al (2020) paper. These data sets include: a. A matrix containing the pitch angle diffusion coefficients for chorus waves at the angle of the loss cone for energies of 30, 100 and 300 keV between L*= 2-7.5, a full range of MLT sectors and for low (1 < Kp < 2), moderate (2 < Kp < 3) and high (4 < Kp < 7) geomagnetic activity levels. These were calculated from an average wave model presented in Meredith et al (2020) to capture the effect of wave-particle interactions in the BAS Radiation Belt Model (BAS-RBM). Also the arrays containing the energy, L*, MLT and Kp dependence are also included. b, A matrix containing the combined pitch angle diffusion coefficients for chorus, hiss and EMIC waves and coulomb collisions between alpha = 0.5deg -9.45deg, Energy = 28.18-2511.89 keV , L* = 4.25-7.25, MLT = 0-24 and 6 different activity levels. The arrays containing the pitch angle, energy, L*, MLT and Kp dependence are also included. Funding was provided by NERC Highlight Topic Grant NE/P01738X/1 and NERC National Capability grants NE/R016038/1 and NE/R016445/1 
Type Of Material Database/Collection of data 
Year Produced 2020 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01362
 
Title Rapid electron acceleration in low density regions of Saturn's radiation belt by whistler mode chorus waves 
Description Radiation belts are hazardous regions found around several of the planets in our Solar System. They consist of very hot, electrically charged particles that are trapped in the magnetic field of the planet. At Saturn the most important way to heat these particles has for many years been thought to involve the particles drifting closer towards the planet. This paper adds to the emerging idea at Saturn that a different way to heat the particles is also possible where the heating is done by waves, in a similar way to what we find at the Earth. This work is reported in the paper "Rapid electron acceleration in low density regions of Saturn's radiation belt by whistler mode chorus waves" by E.E. Woodfield et al., 2019. The data provided here enable reconstruction of all the figures in the paper. 
Type Of Material Database/Collection of data 
Year Produced 2019 
Provided To Others? Yes  
 
Title Solutions to BAS-PRO model runs for Modelling 1-10MeV Proton Phase Space Density 
Description This dataset contains solution data produced by the BAS-PRO proton radiation belt model for the study "Modelling Inner Proton Belt Variability at Energies 1 to 10MeV using BAS-PRO". The solution data is in the form of 3D grids describing phase space density computed during dynamic simulations of Earth's proton belt over the modelling period 2014 to 2018. Three model runs are included: SA19, J81 and S16. Files were produced in May 2021. This work was funded by the Natural Environment Research Council (NERC) via Doctoral Training Programme NE/R009457/1. Richard B. Horne and Sarah A. Glauert were supported by NERC National Capability grants NE/R016038/1 and NE/R016445/1, and by NERC grant NE/V00249X/1 (Sat-Risk), and by Highlight Topic Grant NE/P01738X/1 (Rad-Sat). Giulio Del Zanna acknowledges support from STFC (UK) via the consolidated grants to the atomic astrophysics group (AAG) at DAMTP, University of Cambridge (ST/P000665/1 and ST/T000481/1). Seth G. Claudepierre acknowledges support from NASA Grant no. NNX17AF10G and from RBSP-ECT funding provided by JHU/APL Contract 967399 under NASA's Prime Contract NAS5-01072. 
Type Of Material Database/Collection of data 
Year Produced 2021 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01565
 
Title Statistical investigation of the frequency dependence of the chorus source mechanism of plasmaspheric hiss 
Description We use data from eight satellites to statistically examine the role of chorus as a potential source of plasmaspheric hiss. We find that the strong equatorial (|?m| < 6°) chorus wave power in the frequency range 50 < f < 200 Hz does not extend to high latitudes in any MLT sector and is unlikely to be the source of the low frequency plasmaspheric hiss in this frequency range. In contrast, strong equatorial chorus wave power in the medium frequency range 200 < f < 2000 Hz is observed to extend to high latitudes and low altitudes in the pre-noon sector, consistent with ray tracing modelling from a chorus source and supporting the chorus to hiss generation mechanism. At higher frequencies, chorus may contribute to the weak plasmaspheric hiss seen on the dayside in the frequency range 2000 < f < 3000 Hz band, but is not responsible for the weak plasmaspheric hiss on the night-side in the frequency range 3000 < f < 4000 Hz. The research leading to these results has received funding from the Natural Environment Research Council (NERC) Highlight Topic grant NE/P01738X/1 (Rad-Sat) and the NERC grants NE/V00249X/1 (Sat-Risk) and NE/R016038/1. Jacob Bortnik received funding from NASA grant NNX14AI18G, and RBSP-ECT and EMFISIS funding provided by JHU/APL contracts 967399 and 921647 under NASA's prime contract NAS5-01072. Wen Li and Xiao-Chen Shen received funding from NASA grants 80NSSC20K0698 and 80NSSC19K0845, NSF grant AGS-1847818, and the Alfred P. Sloan Research Fellowship FG-2018-10936. 
Type Of Material Database/Collection of data 
Year Produced 2021 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01467
 
Title TS05 and TS07 external magnetic field model L*, LCDS and B field data for the GOES-13, GOES-15 and HIMAWARI-8 satellites for three geomagnetic storm periods 
Description The dataset contains satellite L* values, last closed drift shell (LCDS) model locations and model magnetic field values for three two day periods covering three different magnetic storms. The periods covered are 27-28 February 2014, 22-23 June 2015 and 14-15 December 2015. The L* values are calculated for electrons with a pitch angle of 90 degrees at the locations of the GOES-13, GOES-15 and HIMAWARI-8 geostationary satellites, using the IRBEM library with the TS05 and TS07 external magnetic field models. Magnetic field values from the models are also included for the GOES-13 satellite during the June 2015 event. LCDS values for each of the periods are included, with two LCDS models based on the TS05 and TS07 field models, and a third LCDS model based particle tracing simulations. This material is based upon work supported by the Air Force Office of Scientific Research under award number FA9550-19-1-7039. Richard Horne and Sarah Glauert were supported by the Natural Environment Research Council (NERC) Highlight Topic Grant NE/P01738X/1 (Rad-Sat) and NERC grant NE/V00249X/1 (Sat-Risk) and National and Public Good activity grant NE/R016445/1. Giulio Del Zanna acknowledges support from STFC (UK) via the consolidated grant to the astrophysics group at DAMTP, University of Cambridge (ST/T000481/1). 
Type Of Material Database/Collection of data 
Year Produced 2022 
Provided To Others? Yes  
URL https://data.bas.ac.uk/full-record.php?id=GB/NERC/BAS/PDC/01653
 
Description Analysis of plasma wave data 
Organisation Boston University
Department Centre for Space Physics
Country United States 
Sector Academic/University 
PI Contribution Analysis and interpretation of THEMIS and Van Allen probe plasma wave data
Collaborator Contribution Provision of wave data in a specified format from THEMIS and Van Allen probes for VLF wave database. Interpretation of wave data.
Impact Meredith, N. P., R. B. Horne, A. Sicard-Piet, D. Boscher, K. H. Yearby, W. Li and R. M. Thorne, Global model of lower band and upper band chorus from multiple satellite observations,J. Geophys. Res., 117, A12209, doi:10.1029/2012JA017978, 2012. Meredith, N. P., R. B. Horne, J. Bortnik, R. M. Thorne, L. Chen, W. Li and A. Sicard-Piet, Global statistical evidence for chorus as the embryonic source of plasmaspheric hiss, Geophys. Res. Lett., 40, doi:10.1002/grl.50593, 2013. Horne, R. B., T. Kersten, S. A. Glauert, N. P. Meredith, D. Boscher, A. Sicard-Piet, R. M. Thorne and W. Li, A new diffusion matrix for whistler mode chorus waves, J. Geophys. Res., 118, 6302-6318, doi:10.1002/jgra.50594 , 2013. Meredith, N. P., R. B. Horne, W. Li, R. M. Thorne, and A. Sicard-Piet, Global model of low frequency chorus (fLHR < f < 0.1fce) from multiple satellite observations, Geophys. Res. Lett., 41, doi:10.1002/2013GL059050, 2014.
Start Year 2012
 
Description MICA - South 
Organisation University of New Hampshire
Department Department of Physics
Country United States 
Sector Academic/University 
PI Contribution Operation and provision of data from a seach coil magnetometer at Halley and Rothera in the Antarctic to the international network.
Collaborator Contribution Provision of data from the wider network of search coil magnetometers in the Antarctic.
Impact Numerous research papers listed elsewhere.
Start Year 2015
 
Description Nonlinear wave-particle interactions 
Organisation University of Reading
Department Department of Meteorology
Country United Kingdom 
Sector Academic/University 
PI Contribution Provision of satellite data, computer modelling output, scientific expertese.
Collaborator Contribution Analysis of satellite data
Impact Research paper given at AGU Chapman Conference, Cascais, Portugal, 2018.
Start Year 2017
 
Description Plasma wave data analysis 
Organisation University of Iowa
Department Department of Physics and Astronomy
Country United States 
Sector Academic/University 
PI Contribution Provision of the HOTRAY code, extertese on plasma waves
Collaborator Contribution Analysis of plasma wave data from the Van Allen Probes mission, wave normal angle distribution, ray tracing of plasma waves
Impact Research papers listed separately.
Start Year 2015
 
Description Ray tracing 
Organisation University of Texas at Dallas
Country United States 
Sector Academic/University 
PI Contribution Provision of the HOTRAY ray tracing code, scientific expertese
Collaborator Contribution Research on the origin and propagation of low frequency plasma waves known as plasmaspheric hiss
Impact several research papers
Start Year 2009
 
Description Shock acceleration 
Organisation Imperial College London
Department Space and Atmospheric Physics Group
Country United Kingdom 
Sector Academic/University 
PI Contribution Discussion and expertese on the radiation belts
Collaborator Contribution Computer simulations of particle motion in the Earth's radiation belts in response to rapid compression of the Earth's magnetic field by coronal mass ejections emitted by the Sun
Impact Too early in the project.
Start Year 2017
 
Description Solar wind coupling 
Organisation University of Sheffield
Department Automatic Control and Systems Engineering
Country United Kingdom 
Sector Academic/University 
PI Contribution Provision of satellite data
Collaborator Contribution Data analysis and machine learning which relates variations in the solar wind outside the Earth's magnetic field to the location and amplitude of plasma waves inside the Earth's radiation belts
Impact Research papers under Rad-Sat listed under the University of Sheffield submission.
Start Year 2017
 
Description Space Insurance 
Organisation Atrium Space Insurance Consortium
Country United Kingdom 
Sector Public 
PI Contribution Analysis of particular space weather events of interest to space insurance, looking at the causes of the event and the space radiation environment
Collaborator Contribution Indication of particular space weather events where satellites may have suffered an outage or a malfunction
Impact Member of the Rad-Sat Stakeholder team. Joint meetings to discuss the risks faced by the space insurance industry.
Start Year 2011
 
Description ULF wave diffusion co-efficients 
Organisation University College London
Department Department of Space and Climate Physics (MSSL)
Country United Kingdom 
Sector Academic/University 
PI Contribution Led discussion and provided expertese on radial diffusion in the radiation belts
Collaborator Contribution Analysis of satellite data to calculate radial diffusion coefficients
Impact Research presentation at the AGU Chapman Conference in Cascais, Portugal, 2018
Start Year 2017
 
Title Software license. 
Description The BAS Radiation Belt Model has been licensed to the UK Met Office for forecasting space weather 
IP Reference  
Protection Trade Mark
Year Protection Granted 2019
Licensed Yes
Impact We have licensed our radiation belt model to the UK Met Office so they can develop our prototype space weather forecasting system into a fully operational system run by the Met Office to help protect satelites from space weather.
 
Description "Sounds of Space" on BBC Earth Podcast Looking Up 
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 I talked to Emily Knight about the "sounds of space" in the BBC Earth podcast "Looking Up"
Year(s) Of Engagement Activity 2019
URL https://www.bbcearth.com/podcast
 
Description Armchair Aurora - Making Music with Mother Nature 
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 I took part in a livestream aurora event run by the Disability charity Aerobility. I described the natural radio "sounds" of our planet as recorded at Halley Research Station, Antarctica and how they have been combined with original music on a grand piano to create novel ambient soundscapes, which resulted in the production of a new album, Aurora Musicalis, last year. I also played the music video from Aurora Musicalis which contains sonic highlights of the natural radio 'sounds' from the album, set to the music of the first track and featuring images from the BAS image collection.
Year(s) Of Engagement Activity 2021
URL https://www.youtube.com/watch?v=gmnj682D42s
 
Description Aurora Musicalis on the ABC Radio National Breakfast Show 
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 I spoke to Hamish McDonald about the science behind Aurora Musicalis on the ABC Radio National Breakfast Show.
Year(s) Of Engagement Activity 2020
URL https://www.abc.net.au/radionational/programs/breakfast/collaboration-between-art-and-science-uses-s...
 
Description Cambridge University Astronomical Society - "Celestial Incantations" 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach Local
Primary Audience Undergraduate students
Results and Impact In this presentation, I explored the amazing variety of natural 'sounds' detected at Halley, Antarctica and then embarked on a sound-led, data-driven journey from Earth-orbit to beyond the galaxy! I then described how the "Sounds of Space Project", our art-science collaboration, has woven these mysterious "sounds" into performances that fuse art and science, new music, and short films. I introduced our first album, "Aurora Musicalis", which features recordings from the Halley VLF Receiver accompanied by ambient music on a grand piano. My talk culminated with a presentation of the tracks and track artwork from "Celestial Incantations", our second album, which features the 'sounds of space' from astronomical objects both within and beyond our solar system together with a massive musical palette, including orchestral and traditional instruments and electronics.\
The talks was recorded and is now available on our 'Sounds of Space" YouTube channel here - https://www.youtube.com/watch?v=f33DdOOrqkc.
Year(s) Of Engagement Activity 2022
URL https://talks.cam.ac.uk/talk/index/168926
 
Description Cambridge University Astronomical Society - "Sounds of Space" 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach Local
Primary Audience Undergraduate students
Results and Impact I gave a presentation in which I introduced the amazing variety of natural radio 'sounds' detected at Halley, Antarctica and then embarked on a sound-led, data-driven journey from Earth-orbit to beyond the galaxy! I then described how these remarkable 'sounds' have been used in art-science collaborations to create performances, new music, and short films. Finally, I described how the recordings from Halley had been used to enhance the exploration gameplay in the space simulation video game Elite Dangerous.
Year(s) Of Engagement Activity 2020
URL https://talks.cam.ac.uk/talk/index/136933
 
Description Celestial Incantations on The Moncrieff Show 
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 I talked to Clare McKenna about Celestial Incantations on the Moncrieff Show on Newstalk, a national independent radio station in Ireland.
Year(s) Of Engagement Activity 2021
URL https://www.newstalk.com/podcasts/highlights-from-moncrieff/celestial-incantations
 
Description Elite Dangerous Discovery Channel - Sounds of Space 
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 Other audiences
Results and Impact I took part in a podcast run by Elite Dangerous in which I talked about the 'sounds of space' and how my collaboration with the team at Elite Dangerous resulted in the inclusion of the space 'sounds' in their space simulation video game. The video has currently had 9,695 views on YouTube.
Year(s) Of Engagement Activity 2019
URL https://www.youtube.com/watch?v=JdEvVx8LDs8
 
Description Interview for BBC on space weather 
Form Of Engagement Activity A broadcast e.g. TV/radio/film/podcast (other than news/press)
Part Of Official Scheme? No
Geographic Reach International
Primary Audience Public/other audiences
Results and Impact TV interview on space weather broadcast on BBC Weather channel, more than 10 times over the Christmas and New year period of 2017/18. Reached over 500,000 people.
Year(s) Of Engagement Activity 2017,2018
URL https://www.bbc.co.uk/programmes/p05rrm08
 
Description Interview with Polygon, an American video gaming website, on the use of VLF recordings from Halley in the space simulation game Elite Dangerous 
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 Interview with Polygon, an American online video gaming website, about the use of VLF recordings from Halley, Antarctica in the space simulation game Elite dangerous. This resulted in a news story entitled "Elite's new exploration system brings even more real-life science into the game - Billions of new audio channels courtesy of a British research team in Antarctica"
Year(s) Of Engagement Activity 2018
URL https://www.polygon.com/2018/12/4/18125779/elite-dangerous-chapter-4-beyond-exploration-audio
 
Description News Article on the Sounds of Space 
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 I was interviewed by Maddie Stone of the Earther, an online environmental news website, about our sounds of space project at BAS. This resulted in an article in the Earther entitled "Listen to the creepy noises picked up by a space weather station in Antarctica". This article has had over 64,900 views. The article included links to vlf recordings from Halley Antarctica, the most popular of which has received over 50,000 hits.
Year(s) Of Engagement Activity 2018
URL https://gizmodo.com/listen-to-the-creepy-noises-picked-up-at-a-space-weathe-1831234519
 
Description Sounds of Space at Cambridge Science Festival 
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 This activity took place at Anglia Ruskin University as part of the Cambridge Science Festival. It included included a scientific presentation on the sounds of space, followed by a performance with animation, contemporary dance and soundscapes, and finished with a question and answer session.
Year(s) Of Engagement Activity 2018
URL https://www.bas.ac.uk/event/cambridge-science-festival-sounds-of-space/
 
Description Sounds of Space at the Bluedot Festival 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach National
Primary Audience Public/other audiences
Results and Impact I gave a talk on the "Sounds of Space" at the Bluedot Festival, Jodrell Bank Observatory. 250 members of the general public were in attendance.
Year(s) Of Engagement Activity 2019
URL https://www.discoverthebluedot.com/profile/panel:-sounds-of-space
 
Description Sounds of Space at the British Antarctic Survey 
Form Of Engagement Activity Participation in an activity, workshop or similar
Part Of Official Scheme? No
Geographic Reach Local
Primary Audience Other audiences
Results and Impact This activity took place at the British Antarctic Survey. It included included a scientific presentation on the sounds of space, followed by a performance with live music, animation, contemporary dance and soundscapes, and finished with a question and answer session. The event was live-streamed and has since had over 11,500 views on the BAS Youtube channel.
Year(s) Of Engagement Activity 2018
URL https://www.bas.ac.uk/event/sounds-of-space-performance/
 
Description Sounds of Space at the Cambridge Festival of Ideas 
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 In October 2019 a new immersive performance of the 'sounds of space' was showcased at the Cambridge Festival of Ideas. This show included a science talk followed by a performance with vibrant, experimental, contemporary dance, in which the dancers moved through the audience and space as they responded to the sound-led, data-driven journey from Antarctica to beyond the galaxy. The dynamic performance was followed by a serene meditative experience, led by Diana Scarborough, featuring 'sounds' from the VLF receiver at Halley, images of Antarctica and the beautiful piano music of Kim Cunio.
Year(s) Of Engagement Activity 2019