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Multilingualism at the UFS reaches remarkable milestones

15 June 2021 | Story Dr Cindé Greyling

Drummers entertained the Mokete crowds throughout the day.

During the past eight months, the University of the Free State Academy for Multilingualism has reached remarkable milestones. The Academy for Multilingualism was born from the UFS Language Policy (2016) and was approved by Senate in November 2020.

Letting languages grow

Multilingualism at the UFS entails the use of English as the primary medium of instruction, with Afrikaans, Sesotho, and isiZulu used selectively in tutorials to support the achievement of greater levels of academic literacy and understanding of the epistemology of the discipline, mostly among undergraduate students. “Accordingly, the academy’s drivers are to develop Sesotho and Isizulu as academic languages, encourage multilingualism in teaching and learning and as a social asset, and to develop English as a language of instruction,” says Dr Peet van Aardt, Custodian of the Academy for Multilingualism.

Developing Sesotho and Isizulu as academic languages

Academic word lists from seven departments are in the process of being translated, in conjunction with the Unit of Lexicography, to create glossaries. The team at South African Sign Languages will add videos to these glossaries to provide unique and inclusive content in the realm of multilingualism.

In April 2021, the academy – in collaboration with the TK Mopeli Library on the Qwaqwa Campus – hosted the launch of an English and Sesotho book on the campus. This work, Meriana ya Dimela tsa Basotho Medicinal Plants, was authored by Prof Rodney Moffett, honorary Research Fellow on the Qwaqwa Campus.

Multilingualism in teaching and learning

To assist students in overcoming the language barrier caused by English as medium of instruction, the academy is working with the Centre for Teaching and Learning’s A_STEP programme to pilot the use of translanguaging in tutor sessions. It is currently done in Law and Geography on the Bloemfontein Campus, and in Academic Literacy on the Qwaqwa Campus.

Voice-over translations of English lessons in the Faculties of Theology and Religion into Afrikaans and Sesotho paved the way for the academy to proceed with this practice in other subjects. They have been able to start with the Departments of Political Studies and Governance (Afrikaans, Sesotho, isiZulu) and Criminology (Sesotho).

English as a language of instruction

The university’s Academic Literacy and Language Development (ALLD) unit has also launched their English Academic Literacy courses for the Faculties of Law, Natural and Agricultural Sciences, Education, the Humanities, Health Sciences, and Economic and Management Sciences.

UFS staff will also be trained in teaching and translanguaging practices. Thus far, one lecturer has been nominated to track her use of translanguaging in the Academic Literacy classroom on the Qwaqwa Campus.

Multilingualism as a social asset

The fourth annual iCAN (Initiative for Creative African Narratives) was launched in April 2021. This project motivates students from all three campuses to write short stories in their mother tongue, and at the end of the year an anthology of stories will be published. In addition, some of the English stories will be injected into the English Academic Literacy courses for first-year students in order to localise the curriculum.

The Kovsies Multilingual Mokete will be hosted online this year and will include activities from the Bloemfontein, Qwaqwa, and South Campuses. The theme of this year’s festival is ‘Hearing you, hearing me’, ‘Ukungizwe, ukukuzwa’ (isiZulu), ‘Ons luister na mekaar’ (Afrikaans), and ‘Mmamele ke o mamele’ (Sesotho).

Academy for Multilingualism extending its footprint

A building that will house the academy on the Qwaqwa Campus is currently being built next to the new media lab. The building will comprise, among others, a 100-seater multipurpose lecture hall that can be converted into four smaller lecture halls. Similarly, a building for the academy is being constructed on the Bloemfontein Campus.

“The Academy for Multilingualism wants to ensure that the UFS becomes the South African leader in multilingualism, and at the impressive rate that they are delivering outputs, this goal will be reached soon,” says Dr Van Aardt.

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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