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19 October 2021 | Story Leonie Bolleurs | Photo Supplied
Prof Arno Hugo was recently elected as Vice-Chair of the Professional Advisory Committee (PAC) for Food Science in the SACNASP.

Prof Arno Hugo from the Department of Animal Science at the University of the Free State (UFS) was recently elected as Vice-Chair of the Professional Advisory Committee (PAC) for Food Science in the South African Council for Natural Scientific Professions (SACNASP).

SACNASP, similar to other professional bodies, is the registration, regulatory and enabling body for natural science professionals. The Natural Scientific Professions Act, 2003 (Act 27 of 2003) mandates SACNASP to register practising natural scientists in one of various fields of practice. Food science is one of 26 fields of practice gazetted for natural science.

Acknowledged as experienced professional

As Vice-Chair of the PAC, Prof Hugo – who is familiar with the processes – is acknowledged as an experienced professional to evaluate applications in this field of practice, where candidates apply for professional registration in Food Science.

He explains that the Advisory Committee ensures that candidates have adequate and relevant training in the natural sciences and in the field of food science. “For registration as professional natural scientist in this specific field, the appropriately qualified candidates must also have one to three years of working experience in the food industry, depending on the level of their food science qualification,” he says. 

Prof Hugo is also involved in interviewing candidates who want to register as professional food scientists via the route of recognition of prior learning (RPL). “Candidates with relevant qualifications can also register as professional food scientists via RPL if they have 10 years of working experience in this field,” he states.

Furthermore, he also evaluates the qualifications and work experience of foreign nationals applying for critical skills visas to work as food scientists in South Africa, due to a shortage of food scientists in South Africa. 

Food safety – a basic human right

According to Prof Hugo, consumers should not have to hope and trust that their food is safe to consume.

Food safety is internationally regarded as a basic human right. Prof Hugo says people must have access to clean (meaning safe) food and water at all times. “When food processing and preservation activities are performed at commercial level, or food – including processed food – is traded to consumers who have no control over the process, the consumers should not only ‘trust’ that their food is safe to be consumed after processing. 

“There need to be processes in place to ensure that consumers are served safe food and water.”

He believes that in order to achieve this, only sufficiently trained and registered scientists should be responsible for ensuring that food safety and quality principles are always applied and adhered to during the manufacture of food products.

“Individuals who want to work in this space must therefore show training and competency to take responsibility for risks such as food spoilage or food poisoning. We all remember the 2018 outbreak of Listeria in the meat processing industry, which caused the death of 200 consumers,” he adds. 

Importance of quality education and lifelong learning skills

Prof Hugo is of the opinion that it is very important that education and lifelong learning skills, through continuing professional development (CPD), are of a high standard and are available to scientists who are contributing to the country's growth, as well as social and economic development.

“The Minister of Higher Education, Science and Technology consults a statutory body such as the SACNASP for input on the science professions. SACNASP is also mentioned in the White Paper on Science and Technology as the custodian of CPD, through which additional skills/re-skilling of scientists are conducted,” he explains.

He says some of the advantages of being registered as a professional natural scientist with SACNASP include that you are recognised as a professional; there is public confidence in you as a scientist, you are more marketable; and you adhere to a code of conduct (you are trusted for ethical values).

Regarding the work he is doing as the Vice-Chair of the Professional Advisory Committee (PAC), Prof Hugo says: “I consider this voluntary work as a privilege and part of my community service to the industry that employs our students.”

News Archive

UFS physicists publish in prestigious Nature journal
2017-10-16

Description: Boyden Observatory gravitational wave event Tags: Boyden Observatory, gravitational wave event, Dr Brian van Soelen, Hélène Szegedi, multi-wavelength astronomy 
Hélène Szegedi and Dr Brian van Soelen are scientists in the
Department of Physics at the University of the Free State.

Photo: Charl Devenish

In August 2017, the Boyden Observatory in Bloemfontein played a major role in obtaining optical observations of one of the biggest discoveries ever made in astrophysics: the detection of an electromagnetic counterpart to a gravitational wave event.
 
An article reporting on this discovery will appear in the prestigious science journal, Nature, in October 2017. Co-authors of the article, Dr Brian van Soelen and Hélène Szegedi, are from the Department of Physics at the University of the Free State (UFS). Both Dr Van Soelen and Szegedi are researching multi-wavelength astronomy.
 
Discovery is the beginning of a new epoch in astronomy
 
Dr van Soelen said: “These observations and this discovery are the beginning of a new epoch in astronomy. We are now able to not only undertake multi-wavelength observations over the whole electromagnetic spectrum (radio up to gamma-rays) but have now been able to observe the same source in both electromagnetic and gravitational waves.”
 
Until recently it was only possible to observe the universe using light obtained from astronomical sources. This all changed in February 2016 when LIGO (Laser Interferometer Gravitational-Wave Observatory) stated that for the first time they had detected gravitational waves on 14 September 2015 from the merger of two black holes. Since then, LIGO has announced the detection of two more such mergers. A fourth was just reported (27 September 2017), which was the first detected by both LIGO and Virgo. However, despite the huge amount of energy released in these processes, none of this is detectable as radiation in any part of the electromagnetic spectrum. Since the first LIGO detection astronomers have been searching for possible electromagnetic counterparts to gravitational wave detections. 
 
Large international collaboration of astronomers rushed to observe source
 
On 17 August 2017 LIGO and Virgo detected the first ever gravitational waves resulting from the merger of two neutron stars. Neutron star mergers produce massive explosions called kilonovae which will produce a specific electromagnetic signature. After the detection of the gravitational wave, telescopes around the world started searching for the optical counterpart, and it was discovered to be located in an elliptical galaxy, NGC4993, 130 million light years away. A large international collaboration of astronomers, including Dr Van Soelen and Szegedi, rushed to observe this source.
 
At the Boyden Observatory, Dr Van Soelen and Szegedi used the Boyden 1.5-m optical telescope to observe the source in the early evening, from 18 to 21 August. The observations obtained at Boyden Observatory, combined with observations from telescopes in Chile and Hawaii, confirmed that this was the first-ever detection of an electromagnetic counterpart to a gravitational wave event. Combined with the detection of gamma-rays with the Fermi-LAT telescope, this also confirms that neutron star mergers are responsible for short gamma-ray bursts.  
 
The results from these optical observations are reported in A kilonova as the electromagnetic counterpart to a gravitational-wave source published in Nature in October 2017.
 
“Our paper is one of a few that will be submitted by different groups that will report on this discovery, including a large LIGO-Virgo paper summarising all observations. The main results from our paper were obtained through the New Technology Telescope, the GROND system, and the Pan-STARRS system. The Boyden observations helped to obtain extra observations during the first 72 hours which showed that the light of the source decreased much quicker than was expected for supernova, classifying this source as a kilonova,” Dr Van Soelen said.

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