PopHorn: A deployable folding horn antenna for low frequency space-based applications
Lead Research Organisation:
University of Manchester
Department Name: Physics and Astronomy
Abstract
Different shapes and types of radio antennas are useful in different circumstances. Horn-shaped antennas are particularly good for when a very accurate calibration of some radio instrumentation (e.g. a radio telescope) is needed, for example. This makes horn antennas very popular for many different applications at microwave frequencies, where they only need to be a few centimetres (or tens of centimetres) across. At low frequencies, a horn antenna would have to be gigantic to work in the same way however. This large size limits their usefulness, particularly for space-based applications where there are restrictive requirements on size and weight of the payloads. We will develop a type of folding antenna that can be packaged up into a relatively small and lightweight form suitable for attaching to a spacecraft, but which folds out into a large horn antenna shape when deployed, suitable for low-frequency applications. This will make it practical to do very high precision radio measurements at low frequencies from space.
Organisations
| Title | RHINO antenna patterns |
| Description | Simulated antenna patterns for the RHINO horn antenna experiment. These antenna patterns were simulated using CST Studio. They may be used under a CC-BY-SA 4.0 license, credited to "A. El-Makadema, on behalf of the RHINO Collaboration". |
| Type Of Material | Database/Collection of data |
| Year Produced | 2024 |
| Provided To Others? | Yes |
| Impact | We have made our full EM simulations of antenna patterns available to the public, which we believe is unique for this type of experiment. |
| URL | https://github.com/RHINO-Experiment/rhino-beams |
| Title | Hydra |
| Description | Hydra is a code that implements a statistical model of complex visibility data from radio telescope arrays that target the 21cm line from neutral hydrogen. Once the 21cm signal, foreground emission, and instrumental effects like primary beams have been incorporated, hundreds of thousands of parameters are required to fully describe the model. Hydra uses a technique called Gibbs sampling to efficiently draw samples from the joint posterior distribution of all the parameters. It is implemented in Python and is compatible with the data formats used by the HERA pipeline, such as UVData and UVBeam. |
| Type Of Technology | Software |
| Year Produced | 2024 |
| Open Source License? | Yes |
| Impact | Hydra is still under development, but has been used in several publications. |
| URL | https://github.com/HydraRadio/Hydra |
| Description | Lovell Lecture at Jodrell Bank Observatory |
| Form Of Engagement Activity | A talk or presentation |
| Part Of Official Scheme? | No |
| Geographic Reach | Regional |
| Primary Audience | Public/other audiences |
| Results and Impact | This was a public lecture called "Chaos at Cosmic Dawn" on the topic of early Universe physics, at the Jodrell Bank Centre for Engagement. Around 200 people attended on the evening, with another approx. 100 watching online. |
| Year(s) Of Engagement Activity | 2025 |
| URL | https://www.jodrellbank.net/events/professor-phil-bull-chaos-at-cosmic-dawn/ |
