EPSRC-Royal Society fellowship engagement (2013): Heating of the solar atmosphere by small flares
Lead Research Organisation:
University of Glasgow
Department Name: School of Physics and Astronomy
Abstract
Please refer to attached Royal Society application
Planned Impact
Please refer to attached Royal Society application
People |
ORCID iD |
| Iain Hannah (Principal Investigator / Fellow) |
Publications
Kuhar M
(2017)
EVIDENCE OF SIGNIFICANT ENERGY INPUT IN THE LATE PHASE OF A SOLAR FLARE FROM NuSTAR X-RAY OBSERVATIONS
in The Astrophysical Journal
Marsh A
(2017)
First NuSTAR Limits on Quiet Sun Hard X-Ray Transient Events
in The Astrophysical Journal
Marsh A
(2017)
First NuSTAR Limits on Quiet Sun Hard X-Ray Transient Events
Wang J
(2017)
Observations of Reconnection Flows in a Flare on the Solar Disk
in The Astrophysical Journal Letters
Wright P
(2017)
Microflare Heating of a Solar Active Region Observed with NuSTAR, Hinode/XRT, and SDO/AIA
in The Astrophysical Journal
| Description | The work was able to successfully use EUV and X-ray observations of the Sun to investigate the amount of emission at different temperatures (known as the Differential Emission Measure, or DEM), with the X-ray data helping to constraint the amount of material at higher (> 5-10 MK) temperatures, which some models of the energy release in the Sun's atmosphere predict to be present. The code used for this project, which can be adapted to other temperature senesitive observations, has been made publicly available via https://pypi.org/project/demregpy/ and https://github.com/ianan/demreg - where the latter has examples of usage with solar X-ray and EUV data in either IDL or Python. The Python version of the software (partially developed during this project, and with subsequent additional funding of a PDRA) has now been used by in several solar journal publications. |
| Exploitation Route | The software is publicly available on either via https://pypi.org/project/demregpy/ and https://github.com/ianan/demreg - where the latter has examples of usage with solar X-ray and EUV data in either IDL or Python. |
| Sectors | Digital/Communication/Information Technologies (including Software) Other |
| Description | ISSI Bern team meeting |
| Amount | SFr. 6,000 (CHF) |
| Organisation | International Space Science Institute (ISSI) |
| Sector | Academic/University |
| Country | Switzerland |
| Start | 01/2016 |
| End | 06/2017 |
| Description | Collaboration with Ireland & Viall |
| Organisation | National Aeronautics and Space Administration (NASA) |
| Department | Goddard Space Flight Center |
| Country | United States |
| Sector | Public |
| PI Contribution | Visit and placement at Nasa Goddard Space Flight Centre, USA for a month to develop the analysis tools for producing lightcurves as a function of temperature instead of wavelength channel for quiescent regions observed in EUV with SDO/AIA. This can then be used as an input to other analysis techniques to determine the heating properties of regions of the solar atmosphere. |
| Collaborator Contribution | Expertise of different analysis techniques to be applied to the SDO/AIA lightcurves which can determine physical properties of the underlying heating mechanisms within different model scenarios. Dr Nicholeen Viall has expertise on a time-lag approach in comparison to EBTEL nanoflare models and Dr. Jack Ireland has expertise in fourier time series analysis to determine heating properties. |
| Impact | Work is still on going and publications should be finished and submitted in 2017. There have been presentations on this work at some meeting, including at the LWS/SDO workshop in Burlington, US in Oct 2016. |
| Start Year | 2016 |
| Description | Live TV/Web coverage of partial solar eclipse |
| Form Of Engagement Activity | A press release, press conference or response to a media enquiry/interview |
| Part Of Official Scheme? | No |
| Geographic Reach | Regional |
| Primary Audience | Schools |
| Results and Impact | The RA employed on the grant spent a morning at the STV studios in Glasgow where a live TV/Web programme was broadcast leading up to and during the partial solar eclipse. The main audience here was school children learning about the eclipse but also the work at Glasgow on solar physics. |
| Year(s) Of Engagement Activity | 2015 |
| Description | Solar Eclipse event |
| Form Of Engagement Activity | Participation in an activity, workshop or similar |
| Part Of Official Scheme? | No |
| Geographic Reach | Local |
| Primary Audience | Undergraduate students |
| Results and Impact | We hosted a viewing event at two locations on campus for the partial solar eclipse in March 2015. We were able to chat to those attending about the solar physics we do at Glasgow whilst the eclipse was happening. Well over thousand people attended at our two locations on campus. We also conducted several TV, radio, newspaper and online interviews before and during the event. |
| Year(s) Of Engagement Activity | 2015 |
| URL | http://www.astro.gla.ac.uk/?p=3626 |