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01 October 2019 | Story Nikile Ntsababa (Registrar)

The nomination process for the election of two representatives to serve on the UFS Council was finalised on Tuesday, 17 September 2019 – the closing date for nominations.
 
Here are the names of the nominees (listed alphabetically):
 
Representative from the Qwaqwa Campus:
None
 
Other representative:
Mr Christo Dippenaar
Dr Pieter du Toit
Mr Lefa Mabaso
Dr Walter Matli
Mr Zama Sigwebela
 
Please note that no nominations were received for representatives from the Qwaqwa Campus.  Since this scenario is not legislated in the Statute, Institutional Rules, and Convocation Constitution, the Registrar will, after consultation with the President of the Convocation, open another round of nominations for Qwaqwa representatives to Council (with the closing date 8 October 2019) to ensure that the campus is also represented on Council.
 
Convocation and Alumni members from the Qwaqwa Campus are therefore given a second opportunity to nominate one representative from among their members for the Qwaqwa Campus.  All nominations must reach the office of the Registrar no later than 16:30 on Wednesday, 9 October 2019.
 
Every nomination form  shall be signed by four (4) members of the Convocation and shall contain the written acceptance of the nomination by the nominee under his/her signature as well as an abridged CV and a motivation of more or less 200 words.
 
Nominations are to be submitted to:  email: registrar@ufs.ac.za or delivered by hand to Nikile Ntsababa, Main Building, Room 51, Bloemfontein Campus.
 
Kindly take note that late or incomplete nominations will not be accepted or considered.
 
Further information regarding the election process will follow in due course.

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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