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14 August 2020 | Story Amanda Tongha | Photo NSFAS

Applications for the National Student Financial Aid Scheme (NSFAS) 2021 are now open.  

The NSFAS application cycle will run for a period of four months starting from 3 August to 30 November 2020. 

NSFAS applications are open to students from poor and working-class backgrounds who wish to further their studies at any public Technical and Vocational Education and Training (TVET) college or university. To qualify for NSFAS funding, the applicant must be a South African citizen; come from a family with a combined annual household income of not more than R350 000; for students with a disability, a combined annual household income of not more than R600 000. 

Applications for 2021 funding will be completed online via the myNSFAS portal as per previous years. 

New applicants need a copy of their ID or birth certificate to register and create a myNSFAS account or profile on the myNSFAS portal. Applicants with existing accounts must log on to their accounts to complete an application. Applicants are not allowed to create more than one profile on the portal. The applicant will be required to give consent to NSFAS to verify their personal information with third parties and will not be able to create a profile without giving this consent. This feature allows NSFAS to conduct a three-step verification process with the Department of Home Affairs (DHA), where an ID number will be linked to the name and surname of the applicant and the parents' details. 

In response to the status quo due to the COVID-19 pandemic, applicants will not be required to submit or upload the consent form; however, they will have to grant consent electronically during the application process, along with accepting the terms and conditions for funding. 

Applicants will, however, still be required to submit their supporting documents, comprising a copy of own ID; parents’/guardian's proof of income; copies of parents’/guardian's ID; and/or Annexure A for applicants with disabilities. 

Qualifying students are urged to make use of this opportunity and apply for funding in time. 

 
 

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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