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01 July 2020

The composition of the UFS Council is stipulated in the UFS Statute, which was published in the Government Gazette on 26 January 2018 and amended by publication in the Government Gazette on 29 March 2019.

The Convocation has to elect one (1) external (neither employee nor student of the UFS) representative to the Council to represent the Convocation and Alumni on Council, following the expiry of the term of office of the current representative on 23 November 2020. The elected representative will serve for a period of four years on Council.

The Convocation comprises all persons who obtained a formal qualification from the UFS, as  well as all permanent academic staff members.

Members of the Convocation are invited to submit written nominations by using the Nomination Form attached hereto.
 
Every nomination form must be signed by 4 (four) members of the Convocation and must contain the written acceptance of the nomination by the nominee under his/her signature, as
well as an abridged CV and a motivation of ± 200 words.

All nominations must reach the office of the Registrar no later than 16:30 on 4 September 2020.
 
If more than one person is nominated an election will be held as stipulated in the Institutional Rules.  More information regarding this process will follow at that stage. 


Nominations are to be submitted to:
 
• or by post (strongly advised not to use this method due to delays):
Mr NN Ntsababa  
Registrar
University of the Free State
PO Box 339
Bloemfontein
9300

• or hand-delivered to:   (depending on the lockdown level and the regulations that are in place).
Mr NN Ntsababa
Room 51, 1st Floor
Main Building
UFS Bloemfontein Campus
 

For enquiries, please contact Mr NN Ntsababa at registrar@ufs.ac.za or +27 51 401 3796.

Kindly take note that late or incomplete nominations will not be accepted or considered.
Every nomination must be submitted separately.

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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