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23 January 2020 | Story Lacea Loader

Update: 26 January 2020
Bloemfontein Campus registration process to continue on Monday 27 January 2020

The registration process for students on the Bloemfontein Campus of the University of the Free State (UFS) will continue on Monday 27 January 2020 as per the registration programme.

First-year students who have not registered must refer to their email, the university’s self-service portal, and the Call Centre (051 401 9666) for information. Senior students can visit registration venues on campus if they require academic advice.

Released by:
Lacea Loader (Director: Communication and Marketing)
Telephone: +27 51 401 2584 | +27 83 645 2454
Email: news@ufs.ac.za | loaderl@ufs.ac.za
Fax: +27 51 444 6393



Update: 24 January 2020
Bloemfontein Campus registration process not to continue the afternoon of Friday 24 January 2020  

The first-year registration process on the Bloemfontein Campus will not continue after 13:00 today (Friday 24 January 2020), but will resume on Monday 27 January 2020.

This decision taken by the executive management of the university comes after a number of students disrupted the registration process this morning and prevented first-year students to enter registration venues.

Constant engagements with the Institutional Student Representative Council (ISRC) and the Student Representative Council (SRC) of the Bloemfontein Campus have taken place since the beginning of the year regarding matters of concern to students, and the executive management will continue to do so. The university management is disappointed with this morning’s disruptive behaviour led by the Bloemfontein Campus SRC, despite these regular engagements.

The situation on the campus is being closely monitored by the university’s Protection Services and the South African Police Service.

 

Released by:
Lacea Loader (Director: Communication and Marketing)
Telephone: +27 51 401 2584 | +27 83 645 2454
Email: news@ufs.ac.za | loaderl@ufs.ac.za
Fax: +27 51 444 6393

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.

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