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28 May 2019 | Story Xolisa Mnukwa
Siphila Dlamini
Siphila Dlamini represented the UFS at the 15th Southern Africa Scout Youth Forum.

During the short April holidays, first-year BA student, Siphila Dlamini, led and participated in the 15th Southern Africa Scout Youth Forum and the 41st Southern Africa Scout Conference. Siphila previously also represented South Africa in the 8th and 13th World Scout Youth Forums in Baku, Azerbaijan and Harare, Zimbabwe respectively. He also participated in the 2018 International Leadership Training in Lilongwe, Malawi.

Siphila was elected as a member of the Southern Africa Youth Committee for the term 2017-2020, with the mandate of representing young leaders in decision making and youth engagement at Zonal level of the Southern Africa Scout Youth Forum.

He formed part of the forum committee and chaired several sessions of the proceedings since the tender age of 14. Youth leaders from Southern African Development Community (SADC) countries such as Botswana, the Kingdom of Eswatini, Malawi, South Africa, Mozambique, Namibia, Zambia, and Zimbabwe attended the conference. 

This 15th forum was themed ‘The Role of young people during emergencies’. Throughout the forum, young people deliberated on strategies to improve decision making in national scout organisations within their respective countries. The Southern Zone Youth Forum empowers young people by equipping them with good decision-making skills and increasing youth engagement on the African continent. 

According to Siphila, the Southern Zone Youth Forum is an effective tool for youth engagement and the continuation of skills development among young people in Southern Africa. It allows the youth to reflect on their growth and achievement, while broadening the unique impact of scouting in the world. 

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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