Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
19 June 2023 | Story Sfundo Mazibuko | Photo Supplied
Sfundo Mazibuko
Sfundo Mazibuko is a Presidential Youth Employment Initiative (PYEI) Intern in the Qwaqwa Campus Health and Wellness Centre

The University of the Free State (UFS) is celebrating Youth Month by showcasing the positive influence of the institution on career development. As part of this initiative, we are sharing the stories of UFS alumni who are now working at the university.

Sfundo Mazibuko, Presidential Youth Employment Initiative (PYEI) Intern in the Qwaqwa Campus Health and Wellness Centre, shares his UFS journey:

Q: Year of graduation from the UFS:

A: My graduation year is 2023.

Q: Qualification obtained from the UFS:

A: Bachelor of Education in Intermediate Phase Teaching, majoring in social sciences and life skills.

Q: Date of joining the UFS as a staff member:

A: March 2023.

Q: Initial job title and current job title:

A: Data Capture Intern in the Health and Wellness Centre.

Q: How did the UFS prepare you for the professional world? 

A: Since I started working as a UFS staff member, I have gained skills in collaborating with colleagues, administration skills, data capturing skills, client welcoming skills, confidentiality skills, and time management skills.

Q: What are your thoughts on transitioning from a UFS alumnus to a staff member?

A: Working at the UFS is an incredibly rewarding experience, with ample career advancement opportunities, a focus on work-life balance, comprehensive benefits, a collaborative work culture, and a commitment to making a positive impact. The UFS nurtures its employees' growth through professional development programmes, offers flexible work arrangements, provides competitive perks, fosters inclusivity and teamwork, and actively engages in philanthropic initiatives. Joining the UFS means embarking on a fulfilling journey of personal and professional growth.

News Archive

Two scientists part of team that discovers the source of the highest energy cosmic rays at the centre of the Milky Way
2016-03-22

Description: Giant molecular clouds  Tags: Giant molecular clouds

Artist's impression of the giant molecular clouds surrounding the Galactic Centre, bombarded by very high energy protons accelerated in the vicinity of the central black hole and subsequently shining in gamma rays.
Artist's impression: © Dr Mark A. Garlick/ H.E.S.S. Collaboration

Spotlight photo:
Dr Brian van Soelen and Prof Pieter Meintjes of the UFS Department of Physics.
Photo: Charl Devenish

H.E.S.S. (High Energy Stereoscopic System) scientists publically revealed their latest galactic discovery in the international science journal, Nature, on 16 March 2016. These scientists were able to pinpoint the most powerful source of cosmic radiation – which, up to now, remained a mystery.

Part of this team of scientists are Prof Pieter Meintjes and Dr Brian van Soelen, both in the University of the Free State (UFS) Department of Physics. Dr Van Soelen explains that they have discovered a proton PeVatron – a source that can accelerate protons up to energies of ~1 PeV (10^15 eV) – at the centre of the Milky Way. The supermassive black hole called Sagittarius A has been identified as the most plausible source of this unprecedented acceleration of protons.

The protons are accelerated to Very High Energy (VHE) gamma rays. The energy of these protons are 100 times larger than those achieved by the Large Hadron Collider at CERN (the European Organization for Nuclear Research).

According to Dr Van Soelen, the fact that this research has been published in Nature demonstrates the importance and pioneering nature of the research conducted by H.E.S.S. The H.E.S.S. observatory – operational in Namibia – is a collaboration between 42 scientific institutions in 12 countries.

In 2006, H.E.S.S. was awarded the Descartes Prize of the European Commission – the highest recognition for collaborative research – and in 2010 the prestigious Rossi Prize of the American Astronomical Society. The extent of the observatory’s significance places it among the ranks of the Hubble Space Telescope and the telescopes of the European Southern Observatory in Chile.

“The next generation VHE gamma-ray telescope,” Dr Van Soelen says, “will be the Cherenkov Telescope Array (CTA), which is currently in the design and development stage.” Both Dr Van Soelen and Prof Meintjes are part of this project as well.

H.E.S.S. has issued a complete statement about the paper published in Nature.

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