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13 September 2021 | Story Bulelwa Moikwatlhai | Photo Supplied
Ms. Mosa Moerane; UFS officer: Kovsie support services.


The COVID-19 pandemic has forced the world into a new normal, with no tips on how to navigate it, nor an end date in sight. We have all found ourselves learning, piloting, evaluating, and repeating the process. Fortunately, one can now say that we have somehow found a balance; however, in this balance, a lot of variables are emerging. One of these is how our diversity impacts the way we interact when we use virtual spaces. As a university, we serve people of diverse cultures daily – hence, as an office, we wanted to explore this variable further. Furthermore, as an institution of higher education, we have a responsibility to contribute knowledge about teaching and learning in virtual spaces.  

The purpose of the International Cultural Diversity Festival is to have intellectual engagements; to learn from experts as well as peers (educate); to teach one another (information sharing); to have social cohesion and to celebrate the diverse cultures through artistic expressions. All of this will be done under the theme ‘embracing diversity in virtual spaces.’ Some of the topics include practising cultural sensitivity; how to incorporate diversity, honour, respect, and your cultural background; social media communication with people of diverse cultures; the psychology of human behaviour and cross-cultural networking in virtual spaces; as well as how the UFS strives to embrace diversity in virtual spaces.

Date: 17 September 2021
Topic: Embracing diversity in virtual spaces
Time: 10:00
Venue: 2021 ICDF 

Facilitator: Ms Mosa Moerane

Panellists:

Prof Katherine Wimpenny
Professor of Research in Global Learning at Coventry University

Dr. Grey Magaiza
Head of Community Development at the UFS and Program Director in the Faculty of Humanities at the QwaQwa campus 

Ms. Reabetswe Mabine
Marketing and Communication strategist: UFS Postgraduate School

Mrs Bulelwa Moikwatlhai
Coordinator: Internationalisation at Home and Inbound Student Mobility

Biographies of panellist


Prof Katherine Wimpenny, PhD, leads the research theme ‘Global Education: Learning without Boundaries’ in the Research Institute for Global Learning, Coventry University, UK. Prof Wimpenny’s research focuses on contextualised and comprehensive internationalisation at the interface of decolonisation of education practices, embedded in the broader context of curriculum transformation. She is researching a diversity of learning spaces (digital – especially Collaborative Online International learning, face to face, blended, formal, and non-formal) that interweave to impact educational opportunities, which can serve to connect international learning communities, as well as to connect the university to its locale.  Prof Wimpenny has a substantial track record as principal and co-investigator on large-scale international education research projects and disseminates her work widely through a range of publications/media.

Dr Magaiza is a social scientist with an interest in community development, particularly participatory, bottom-up approaches to social change. He uses his interest in inclusive development approaches to not only theorise sustainable change, but also to critically reflect on the role of science and knowledge in community change. As a scholar of community development, he has used this knowledge with student structures such as Enactus to look for ways of using business principles to improve communities. Dr Magaiza is also coordinating the UK-USDP project that currently has 10 staff members enrolled as PhD students at the UFS, Univen, and the University of the Highlands and Islands in Scotland. 
 
He is currently the Head of Community Development at the UFS and Programme Director in the Faculty of the Humanities on the Qwaqwa Campus.

Being multi-faceted often makes it difficult to discover your voice and place in this fast-paced society; this is, however, not the case with Reabetswe Mabine – also known as Rea Mabine – who embodies authenticity and self-determinism. From pageantry to leadership and business, she positions herself as someone who is grounded and wants to achieve success on her terms. 
Rea Mabine is a marketing and communications strategist who runs a branding and marketing consultancy that helps start-ups and small businesses to launch and position their businesses competitively within their industries, using effective marketing and communication strategies as well as strategic brand development. 

- She is a friend of ‘The Network’ – a show on City Radio, which is an online radio station where she gives her expert opinion on topics about digital marketing, social media, and legal aspects in the marketing field. 
- She is the former Youth President of Phenomenal Women Youth Chamber of Commerce and Industry, an organisation aimed at encouraging entrepreneurship among young females in South Africa. 
- In 2018, she was recognised as Young Woman of Achievement by the Free State Heroines Awards Ceremony. This award recognises a young female who portrays outstanding involvement with youth-related initiatives and shows excellence in her pursuits. 
- She is a Play Your Part, Brand SA ambassador.
- Rea Mabine co-produced, co-directed, and co-presented a television show that aired on national TV and received an award for the best traditional TV programme at the nationally renowned South African Traditional Music Awards (SATMA). 
- Rea Mabine was a top-10 finalist for Miss Heritage South Africa in 2016, and the first-ever to be crowned Miss Heritage Free State.

Despite her achievements, she stays grounded and is always looking for the next challenge. Rea Mabine is also passionate about professional and career development for women; initiatives that empower women are very close to her heart.

Mrs Moikwatlhai is passionate about student life and integration; internationalisation; the development of students’ international and intercultural competencies, as well as ensuring that all UFS students have an international experience during their studies at the UFS. She achieves this by developing co-curricular activities that help to improve students’ experiences at the UFS. As the university’s expert on internationalisation at home, she uses her knowledge to improve first-year experiences in her capacity as a member of the UFS First-Year Experience (FYE) Committee. Mrs Moikwatlhai is also the university’s expert on student mobilities, coordinating and managing the UFS’ first virtual mobility programme. Additionally, she coordinates and manages the UFS’ flagship integration programme for local and international students in the Umoja Buddy Programme. 

She currently leads the University of the Free State Internationalisation at Home and Inbound Student Mobility portfolio in the Office for International Affairs.

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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