Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
22 May 2020 | Story Leonie Bolleurs | Photo Supplied
Prof Das Steÿn was announced as the recipient of the prestigious Stals Prize this week (19 May 2020), awarded by the Suid-Afrikaanse Akademie vir Wetenskap en Kuns.

Prof Das Steÿn, former Head and currently a research fellow in the Department of Urban and Regional Planning at the University of the Free State (UFS), has been named the recipient of the prestigious Stals Prize this week (19 May 2020), awarded by the Suid-Afrikaanse Akademie vir Wetenskap en Kuns (South African Academy for Science and Arts).

The current Head of the Department, Prof Maléne Campbell, together with two academics from the North-West University, Profs Juanée Cilliers (Head of the Urban and Regional Planning group) and Ewert Kleynhans (School of Economic Sciences), nominated Prof Steyn for the award.

A lifetime’s work

The Stals Prize for Urban and Regional Planning was awarded to Prof Steÿn, based on his numerous publications in Afrikaans, the important role he played in the planning profession in South Africa, his major contribution to the planning of literature, as well as the academic development of urban and regional planning. The award recognises Prof Steÿn for a lifetime's work in the field of urban and regional planning – including his appointment as a lecturer (1980-2009) and also for his time as editor of the journal Stads-en Streekbeplanning / Town and Regional Planning / Meralo ya Ditoropo le Mabatowa (2000-2019).

“As editor of the journal for Urban and Regional Planning, Prof Steÿn set a very high standard. So much so that this UFS journal was listed earlier this year on the international SciELO (Scientific Electronic Library Online), a Norwegian database. As an academic, his research and theoretical knowledge of normative planning are also highly regarded,” says Prof Campbell.

Motivating Prof Steÿn’s nomination for the Stals Prize, Prof Campbell states that as editor, he has sought to highlight issues in the South African planning industry through well-founded headlines. “The journal also grew from a small local journal to a journal that is being read every month in more than 60 countries on the free access platform,” she adds.

In addition to this journal, Prof Steÿn has also published in other journals and written books that have appeared bilingually in South Africa. Then there is also a work that has appeared in Dutch in the Netherlands with his contribution in Afrikaans.

He applied a combination of the urbanistic concept with Christian philosophy in his work and published some articles on the topic.

Distinction between thought and action

Prof Steÿn says that in urbanistics, a distinction is made between the framework of thought and action. It is a matter of answering the ‘what?’, ‘how?’, and ‘why?’ questions.

He believes urbanistics is particularly useful in public participation to bring the various role players in planning together. It makes it possible to distinguish between the considerable number of factors that complicate matters. South Africa, with its unique situation regarding planning, may be able to make good use of this concept.

As example, he uses the matter of providing basic services such as electricity to a community. “At the first level of infrastructure, the problem of providing electricity is easy to solve: x people use y units, implying that z units must be provided. This solves the ‘what?’ part of the problem. The ‘how?’ question in the superstructure is also relatively easy to answer. Different engineers may have different solutions about the appropriate design of the distribution network and how it should link to the greater whole. Still, in the end, the most effective design will be sufficient.”
 
“The major crisis is in the ‘why?’ question. At the ideological level, basic services mean different things to different people. Basic services to the Marxist are a right that every person must receive free of charge, while the capitalist considers it a commodity that every human being should pay for to receive.”

“This simple example shows that there is a definite difference in viewpoints about the mere provision of electricity and that these attitudes of people will, as a matter of course, influence the planning process itself,” he explains. 

Recognising outstanding work

The Suid-Afrikaanse Akademie vir Wetenskap en Kuns awards the Stals Prize for, among others, high-quality publications or a series of high-quality publications (preferably in Afrikaans) whereby extraordinary contributions are made to the practice of science.

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.

We use cookies to make interactions with our websites and services easy and meaningful. To better understand how they are used, read more about the UFS cookie policy. By continuing to use this site you are giving us your consent to do this.

Accept