Consolidated Solar System Physics Research at UCLan
Lead Research Organisation:
University of Central Lancashire
Department Name: Jeremiah Horrocks Institute
Abstract
This consolidated grant proposal brings together research within the Jeremiah Horrocks Institute (JHI) of the University of Central Lancashire (UCLan), along with consortium collaboration with researchers at the Open University, in the research areas of solar and heliospheric physics. In these areas we will be addressing key science questions at the cutting edge of solar system research about the dynamics of the Sun and how it effects it local environment.
Specific projects include:
- investigating the effect of the rotation of sunspots on solar activity such as solar flares and coronal mass ejections to determine whether sunspot rotation leads to increased solar activity;
- exploring the nature of coronal loop heating using data from the MaGIXS sounding rocket flight and the EIS instrument on the Hinode satellite to constrain theoretical and numerical heating models;
- determining how conditions in the different layers of the Sun's atmosphere influence the onset of coronal mass ejections (CMEs), and whether atmospheric dimmings can be used as a diagnostic to predict CMEs;
- modelling the propagation of Solar Energetic Particles (SEPs) in the inner heliosphere with numerical codes and comparing with observations to determine the underlying physics throughout the solar system;
- mapping the zodiacal cloud near Mercury to better understand dust impacts on that planet, and, surveying the zodiacal cloud as a whole to investigate the effects of planets on the cloud and the sources of interplanetary dust.
Specific projects include:
- investigating the effect of the rotation of sunspots on solar activity such as solar flares and coronal mass ejections to determine whether sunspot rotation leads to increased solar activity;
- exploring the nature of coronal loop heating using data from the MaGIXS sounding rocket flight and the EIS instrument on the Hinode satellite to constrain theoretical and numerical heating models;
- determining how conditions in the different layers of the Sun's atmosphere influence the onset of coronal mass ejections (CMEs), and whether atmospheric dimmings can be used as a diagnostic to predict CMEs;
- modelling the propagation of Solar Energetic Particles (SEPs) in the inner heliosphere with numerical codes and comparing with observations to determine the underlying physics throughout the solar system;
- mapping the zodiacal cloud near Mercury to better understand dust impacts on that planet, and, surveying the zodiacal cloud as a whole to investigate the effects of planets on the cloud and the sources of interplanetary dust.
Planned Impact
A principal impact is Community Engagement, of which our primary beneficiaries are students at schools and colleges, as well as members of the broader community, in Lancashire. In addition via social media and partnerships with organisations beyond the county, our reach is global.
While there is an element of dissemination in much of this work, the real impact derives from demonstrating to the people of Lancashire that work of national and international importance is taking place on their doorstep, and they can both benefit and become involved. Lancashire has some significant areas of very low engagement in Higher Education, including one of the lowest regions, Burnley. Our engagement work allows us to influence aspirations amongst children from a young age, and maintain interest in physics-focused study through the critical teenage years. In addition some of the initiatives described in Pathways to Impact have regional (North West) and wider reach, demonstrating that such work is not restricted to the largest and most prestigious institutes that may not be perceived as accessible to those from under-represented communities. For more details see:
http://www.star.uclan.ac.uk/events/
and
http://www.star.uclan.ac.uk/outreach/
Alston Observatory
We run the Alston Observatory, about 8 miles from Preston, which is a purpose-built teaching facility. Also on the site are telescopes with a long history, as well as a new 0.7-metre teaching telescope. We run monthly star-gazing events for the public. We also have a Discovery Dome planetarium system, exhibits on Telescopes as Time Machines funded by the Royal Astronomical Society, and an outside experiment on Measuring the Cosmos. Discovery Dome is an exciting system that allows a laptop computer and digital projector to display movies onto a planetarium dome, as well as enhanced planetarium shows. This will enable both informative material to be presented for evening events, and educational material for curriculum enhancement. We run many outreach events at Alston, including Stargazing Live and other public observing evenings. We have links with many local astronomical societies. We also run many events for local schools at Alston. See:
http://www.star.uclan.ac.uk/alston/workshops.php
Lancashire Science Festival
The University runs a 3-day science festival every year attracting up to 17,000 visitors from local schools and the general public. The JHI, and members of the solar physics group, actively participate in this event, developing and delivering activities ranging from stands on the show floor (there are separate mathematics, physics, and astrophysics stands), to scheduled seminars and shows. This event allows us to enthuse school students and the general public about solar and astrophysics, and disseminate results from our research.
Space Weather
Research on Solar Energetic Particles (SEPs) has application to Space Weather forecasting. A number of approaches and systems that aim to predict the radiation risk associated with SEPs are currently being developed worldwide. UCLan's earlier research on SEP propagation was used to produce a forecasting model, SPARX. This tool has been incorporated into the COMESEP Alert System and ESA Space Situational Awareness Services. A collaboration with the UK Met Office on implementing SPARX as one of its forecasting tools is ongoing. Therefore a clear pathway to impact for the work on SEP modelling exists.
While there is an element of dissemination in much of this work, the real impact derives from demonstrating to the people of Lancashire that work of national and international importance is taking place on their doorstep, and they can both benefit and become involved. Lancashire has some significant areas of very low engagement in Higher Education, including one of the lowest regions, Burnley. Our engagement work allows us to influence aspirations amongst children from a young age, and maintain interest in physics-focused study through the critical teenage years. In addition some of the initiatives described in Pathways to Impact have regional (North West) and wider reach, demonstrating that such work is not restricted to the largest and most prestigious institutes that may not be perceived as accessible to those from under-represented communities. For more details see:
http://www.star.uclan.ac.uk/events/
and
http://www.star.uclan.ac.uk/outreach/
Alston Observatory
We run the Alston Observatory, about 8 miles from Preston, which is a purpose-built teaching facility. Also on the site are telescopes with a long history, as well as a new 0.7-metre teaching telescope. We run monthly star-gazing events for the public. We also have a Discovery Dome planetarium system, exhibits on Telescopes as Time Machines funded by the Royal Astronomical Society, and an outside experiment on Measuring the Cosmos. Discovery Dome is an exciting system that allows a laptop computer and digital projector to display movies onto a planetarium dome, as well as enhanced planetarium shows. This will enable both informative material to be presented for evening events, and educational material for curriculum enhancement. We run many outreach events at Alston, including Stargazing Live and other public observing evenings. We have links with many local astronomical societies. We also run many events for local schools at Alston. See:
http://www.star.uclan.ac.uk/alston/workshops.php
Lancashire Science Festival
The University runs a 3-day science festival every year attracting up to 17,000 visitors from local schools and the general public. The JHI, and members of the solar physics group, actively participate in this event, developing and delivering activities ranging from stands on the show floor (there are separate mathematics, physics, and astrophysics stands), to scheduled seminars and shows. This event allows us to enthuse school students and the general public about solar and astrophysics, and disseminate results from our research.
Space Weather
Research on Solar Energetic Particles (SEPs) has application to Space Weather forecasting. A number of approaches and systems that aim to predict the radiation risk associated with SEPs are currently being developed worldwide. UCLan's earlier research on SEP propagation was used to produce a forecasting model, SPARX. This tool has been incorporated into the COMESEP Alert System and ESA Space Situational Awareness Services. A collaboration with the UK Met Office on implementing SPARX as one of its forecasting tools is ongoing. Therefore a clear pathway to impact for the work on SEP modelling exists.
Organisations
- University of Central Lancashire (Lead Research Organisation)
- North-West University (Collaboration)
- UNIVERSITY OF READING (Collaboration)
- University of Minnesota (Collaboration)
- Helmholtz Association of German Research Centres (Collaboration)
- Kiel University (Collaboration)
- Research Institute in Astrophysics and Planetology (Collaboration)
- University of New Hampshire (Collaboration)
- China University of Geosciences (Collaboration)
- Johns Hopkins University (Collaboration)
- Stanford University (Collaboration)
- University of Helsinki (Collaboration)
- University of Graz (Collaboration)
- Harbin Institute of Technology (Collaboration)
- Western Kentucky University (Collaboration)
- Observatory of Paris (Collaboration)
- National Aeronautics and Space Administration (NASA) (Collaboration)
- University College London (Collaboration)
- University of Alabama in Huntsville (Collaboration)
- University of St Andrews (Collaboration)
- Peking University (Collaboration)
- Russian Academy of Sciences (Collaboration)
- Meteorological Office UK (Collaboration)
- Rutherford Appleton Laboratory (Collaboration)
- Florida Institute of Technology (Collaboration)
- UNIVERSITY OF GLASGOW (Collaboration)
- University of Göttingen (Collaboration)
- University of Leuven (Collaboration)
- University of Würzburg (Collaboration)
People |
ORCID iD |
Silvia Dalla (Principal Investigator) | |
Timo Laitinen (Researcher) |
Publications
Battarbee M
(2018)
Multi-spacecraft observations and transport simulations of solar energetic particles for the May 17th 2012 event
in Astronomy & Astrophysics
Dalla S
(2018)
Application of Test Particle Simulations to Solar Energetic Particle Forecasting
in Proceedings of the International Astronomical Union
Dalla S
(2020)
3D propagation of relativistic solar protons through interplanetary space
in Astronomy & Astrophysics
Dalla S
(2019)
Solar and Heliospheric Physics
Doran D
(2019)
Temporal Evolution of Heavy-Ion Spectra in Solar Energetic Particle Events
in Solar Physics
Description | The research has produced new understanding of how turbulence influences the propagation of Solar Energetic Particles (SEPs) from the Sun to the Earth. Specifically it has shown that it is important to include turbulence effects when modelling the length of meandering field lines that the particles propagate on. Turbulence has a big impact on the timing of arrival near Earth of the first particles. The work has also studied how energetic particles propagate from acceleration regions high in the solar corona towards the photosphere. It has shown that only a small fraction of particles (of the order of a few percent) can back-precipitate and produce the long duration gamma ray emission that can be observed in connection with solar flares. Analysis of spacecraft observations of SEPs, taken by a fleet of spacecraft including Solar Orbiter and Parker Solar Probe, has demonstrated that particle propagation across the average magnetic field is more efficient than previously thought and likely to be caused by turbulence-associated propagation effects. |
Exploitation Route | Other researchers working on similar topics have adopted some of our approaches to modelling turbulence effects. |
Sectors | Aerospace Defence and Marine Transport |
Description | Models of SEP propagation that this project contributed to are being used at the Met Office Space Weather Centre. |
First Year Of Impact | 2019 |
Sector | Aerospace, Defence and Marine |
Impact Types | Policy & public services |
Description | Consolidated Solar and Heliospheric Physics Research at UCLan |
Amount | £339,027 (GBP) |
Funding ID | ST/V000934/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2021 |
End | 03/2024 |
Description | NASA HSR NNH16ZDA001N-HSR for Research Opportunities in Space and Earth Science - 2016 (ROSES-2016) |
Amount | $250,000 (USD) |
Organisation | National Aeronautics and Space Administration (NASA) |
Sector | Public |
Country | United States |
Start | 03/2017 |
End | 02/2019 |
Description | SSA P3-SWE-IV.2:USE OF L5 DATA IN CME PROPAGATION MODELS |
Amount | € 449,912 (EUR) |
Organisation | European Space Agency |
Sector | Public |
Country | France |
Start | 09/2021 |
End | 09/2022 |
Description | SWIMMR Aviation Risk Modelling (SWARM) |
Amount | £279,817 (GBP) |
Funding ID | NE/V002864/1 |
Organisation | Natural Environment Research Council |
Sector | Public |
Country | United Kingdom |
Start | 05/2020 |
End | 05/2024 |
Description | Dr Georgia De Nolfo, NASA Goodard Space Flight Center |
Organisation | National Aeronautics and Space Administration (NASA) |
Country | United States |
Sector | Public |
PI Contribution | Dr Georgia De Nolfo visited us for a week in January 2018 to work on comparing PAMELA spacecraft data with our simulations of SEP propagation. This collaboration is ongoing. |
Collaborator Contribution | 3D test particle simulations of relativistic protons during flare/CME events. |
Impact | Conference presentation at SHINE Meeting 2018 and at ICRC 2019. Two refereed journal papers currently in preparation. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | Helmholtz Association of German Research Centres |
Department | German Research Centre for Geosciences |
Country | Germany |
Sector | Private |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | North-West University |
Country | South Africa |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | Observatory of Paris |
Country | France |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | Stanford University |
Country | United States |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | University of Alabama in Huntsville |
Country | United States |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | University of Glasgow |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | University of Kiel |
Country | Germany |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | University of Minnesota |
Country | United States |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI Team on Flares and SEPs, 6-6-2018 |
Organisation | Western Kentucky University |
Country | United States |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching "Solar flare acceleration signatures and their connection to solar energetic particles". |
Collaborator Contribution | Participation to meetings and associated research. Scientific presentation at meeting |
Impact | It is expected that scientific publications will be outcome of this activity in future. |
Start Year | 2018 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | China University of Geosciences |
Country | China |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | Florida Institute of Technology |
Country | United States |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | Harbin Institute of Technology |
Country | China |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | Helmholtz Association of German Research Centres |
Department | German Research Centre for Geosciences |
Country | Germany |
Sector | Private |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | Johns Hopkins University |
Department | Applied Physics Laboratory (APL) |
Country | United States |
Sector | Charity/Non Profit |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | Peking University |
Country | China |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | Research Institute in Astrophysics and Planetology |
Country | France |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | Russian Academy of Sciences |
Department | Ioffe Physical-Technical Institute |
Country | Russian Federation |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | University of Alabama in Huntsville |
Country | United States |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | University of Leuven |
Country | Belgium |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | University of New Hampshire |
Country | United States |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | ISSI team 469, on using energetic particles to investigate solar wind structures |
Organisation | University of Wurzburg |
Country | Germany |
Sector | Academic/University |
PI Contribution | Timo Laitinen was invited to be part of this Team funded by the International Space Science Institute (ISSI, Bern, Switzerland) to hold a series of research meetings. The team is researching how to use solar energetic particles to investigate solar wind structures and infer solar wind magnetic field configurations. The first meeting was to take place in April 2020 in Bern, Switzerland, but this was cancelled due to coronavirus situation. An online meeting was organised during the online American Geophysical Union meeting in December 2021. The first in-person meeting in Bern took place in July 2022, and the second meeting, in Beijing, will take place in June 2023. In the Bern meeting, Laitinen gave a talk about the recent work, now published, receiving valuable feedback. Laitinen also participated actively in discussion of the works of other participants. Further collaborative work was planned, and is in progress. |
Collaborator Contribution | The partners provided valuable comments to ongoing work during the meeting. Wider range of topics were discussed, and collaborative work was discussed. |
Impact | 10.3847/1538-4357/aca892 (contribution from other team members through discussions during the meeting) |
Start Year | 2020 |
Description | Use of L5 Data in CME Propagation Models. P3-SWE-IV. |
Organisation | Meteorological Office UK |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Proposal for an ESA-funded project for investigating use of a spacecraft at L5 to forecast space weather efffects due to coronal mass ejections. The project was approved, with RAL as lead applicant and the others as subcontractors. The subcontracts were projected to start April 2021, but due to partly Covid-related delays , the project started only in October 2022, and is currently projected to end 1 June 2023. Dr. Laitinen is the PI of the UCLan subcontract, and supervises the project subproject, which is being delivered by Dr. Bill Swalwell. |
Collaborator Contribution | The partners provided modelling and observational data on coronal mass ejections observed by STEREO spacecraft. The UCLan group then utilised this data in analysing how inclusion of observations of the CME at Earth and L5 affect the forecasting of solar energetic particle fluxes at Earth. |
Impact | Outputs are anticipated in terms of reports from first-second quarter of 2023. Publications are anticipated. |
Start Year | 2019 |
Description | Use of L5 Data in CME Propagation Models. P3-SWE-IV. |
Organisation | Rutherford Appleton Laboratory |
Department | RAL Space |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Proposal for an ESA-funded project for investigating use of a spacecraft at L5 to forecast space weather efffects due to coronal mass ejections. The project was approved, with RAL as lead applicant and the others as subcontractors. The subcontracts were projected to start April 2021, but due to partly Covid-related delays , the project started only in October 2022, and is currently projected to end 1 June 2023. Dr. Laitinen is the PI of the UCLan subcontract, and supervises the project subproject, which is being delivered by Dr. Bill Swalwell. |
Collaborator Contribution | The partners provided modelling and observational data on coronal mass ejections observed by STEREO spacecraft. The UCLan group then utilised this data in analysing how inclusion of observations of the CME at Earth and L5 affect the forecasting of solar energetic particle fluxes at Earth. |
Impact | Outputs are anticipated in terms of reports from first-second quarter of 2023. Publications are anticipated. |
Start Year | 2019 |
Description | Use of L5 Data in CME Propagation Models. P3-SWE-IV. |
Organisation | University College London |
Department | Department of Space and Climate Physics (MSSL) |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Proposal for an ESA-funded project for investigating use of a spacecraft at L5 to forecast space weather efffects due to coronal mass ejections. The project was approved, with RAL as lead applicant and the others as subcontractors. The subcontracts were projected to start April 2021, but due to partly Covid-related delays , the project started only in October 2022, and is currently projected to end 1 June 2023. Dr. Laitinen is the PI of the UCLan subcontract, and supervises the project subproject, which is being delivered by Dr. Bill Swalwell. |
Collaborator Contribution | The partners provided modelling and observational data on coronal mass ejections observed by STEREO spacecraft. The UCLan group then utilised this data in analysing how inclusion of observations of the CME at Earth and L5 affect the forecasting of solar energetic particle fluxes at Earth. |
Impact | Outputs are anticipated in terms of reports from first-second quarter of 2023. Publications are anticipated. |
Start Year | 2019 |
Description | Use of L5 Data in CME Propagation Models. P3-SWE-IV. |
Organisation | University of Graz |
Country | Austria |
Sector | Academic/University |
PI Contribution | Proposal for an ESA-funded project for investigating use of a spacecraft at L5 to forecast space weather efffects due to coronal mass ejections. The project was approved, with RAL as lead applicant and the others as subcontractors. The subcontracts were projected to start April 2021, but due to partly Covid-related delays , the project started only in October 2022, and is currently projected to end 1 June 2023. Dr. Laitinen is the PI of the UCLan subcontract, and supervises the project subproject, which is being delivered by Dr. Bill Swalwell. |
Collaborator Contribution | The partners provided modelling and observational data on coronal mass ejections observed by STEREO spacecraft. The UCLan group then utilised this data in analysing how inclusion of observations of the CME at Earth and L5 affect the forecasting of solar energetic particle fluxes at Earth. |
Impact | Outputs are anticipated in terms of reports from first-second quarter of 2023. Publications are anticipated. |
Start Year | 2019 |
Description | Use of L5 Data in CME Propagation Models. P3-SWE-IV. |
Organisation | University of Göttingen |
Country | Germany |
Sector | Academic/University |
PI Contribution | Proposal for an ESA-funded project for investigating use of a spacecraft at L5 to forecast space weather efffects due to coronal mass ejections. The project was approved, with RAL as lead applicant and the others as subcontractors. The subcontracts were projected to start April 2021, but due to partly Covid-related delays , the project started only in October 2022, and is currently projected to end 1 June 2023. Dr. Laitinen is the PI of the UCLan subcontract, and supervises the project subproject, which is being delivered by Dr. Bill Swalwell. |
Collaborator Contribution | The partners provided modelling and observational data on coronal mass ejections observed by STEREO spacecraft. The UCLan group then utilised this data in analysing how inclusion of observations of the CME at Earth and L5 affect the forecasting of solar energetic particle fluxes at Earth. |
Impact | Outputs are anticipated in terms of reports from first-second quarter of 2023. Publications are anticipated. |
Start Year | 2019 |
Description | Use of L5 Data in CME Propagation Models. P3-SWE-IV. |
Organisation | University of Helsinki |
Country | Finland |
Sector | Academic/University |
PI Contribution | Proposal for an ESA-funded project for investigating use of a spacecraft at L5 to forecast space weather efffects due to coronal mass ejections. The project was approved, with RAL as lead applicant and the others as subcontractors. The subcontracts were projected to start April 2021, but due to partly Covid-related delays , the project started only in October 2022, and is currently projected to end 1 June 2023. Dr. Laitinen is the PI of the UCLan subcontract, and supervises the project subproject, which is being delivered by Dr. Bill Swalwell. |
Collaborator Contribution | The partners provided modelling and observational data on coronal mass ejections observed by STEREO spacecraft. The UCLan group then utilised this data in analysing how inclusion of observations of the CME at Earth and L5 affect the forecasting of solar energetic particle fluxes at Earth. |
Impact | Outputs are anticipated in terms of reports from first-second quarter of 2023. Publications are anticipated. |
Start Year | 2019 |
Description | Use of L5 Data in CME Propagation Models. P3-SWE-IV. |
Organisation | University of Reading |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Proposal for an ESA-funded project for investigating use of a spacecraft at L5 to forecast space weather efffects due to coronal mass ejections. The project was approved, with RAL as lead applicant and the others as subcontractors. The subcontracts were projected to start April 2021, but due to partly Covid-related delays , the project started only in October 2022, and is currently projected to end 1 June 2023. Dr. Laitinen is the PI of the UCLan subcontract, and supervises the project subproject, which is being delivered by Dr. Bill Swalwell. |
Collaborator Contribution | The partners provided modelling and observational data on coronal mass ejections observed by STEREO spacecraft. The UCLan group then utilised this data in analysing how inclusion of observations of the CME at Earth and L5 affect the forecasting of solar energetic particle fluxes at Earth. |
Impact | Outputs are anticipated in terms of reports from first-second quarter of 2023. Publications are anticipated. |
Start Year | 2019 |
Description | Use of L5 Data in CME Propagation Models. P3-SWE-IV. |
Organisation | University of St Andrews |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Proposal for an ESA-funded project for investigating use of a spacecraft at L5 to forecast space weather efffects due to coronal mass ejections. The project was approved, with RAL as lead applicant and the others as subcontractors. The subcontracts were projected to start April 2021, but due to partly Covid-related delays , the project started only in October 2022, and is currently projected to end 1 June 2023. Dr. Laitinen is the PI of the UCLan subcontract, and supervises the project subproject, which is being delivered by Dr. Bill Swalwell. |
Collaborator Contribution | The partners provided modelling and observational data on coronal mass ejections observed by STEREO spacecraft. The UCLan group then utilised this data in analysing how inclusion of observations of the CME at Earth and L5 affect the forecasting of solar energetic particle fluxes at Earth. |
Impact | Outputs are anticipated in terms of reports from first-second quarter of 2023. Publications are anticipated. |
Start Year | 2019 |
Description | Public talk at West Didsbury Astronomical Society |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Public/other audiences |
Results and Impact | Public talk on space weather, connected to performed research, to abou 25 amateur astronomers. Widening knowledge on part of space research that is usually not well known by general public, including amateur astronomers. |
Year(s) Of Engagement Activity | 2019 |
Description | SUN Art Installation - Lightpool Festival, Blackpool Winter Gardens, 14-26 October 2019 |
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 | A world premiere, SUN is a partnership between public artist Alex Rinsler and Prof. Robert Walsh, one of the UK's leading solar physicists. SUN is a seven-metre diameter suspended sphere, presenting astrophysical data from NASA's Solar Dynamic Observatory in stunning 360°. SUN displays several months in the life of our closest star but in tens of minutes of real time. Dalla and Laitinen supported the art display by talking with the public about how the SUN movies were obtained, what they showed and the physics of the Sun, over several evenings. |
Year(s) Of Engagement Activity | 2019 |
URL | https://www.visitblackpool.com/things-to-do/festival/sun-(2)/ |