The National Research Foundation was established as an independant government agency, through the National Research Foundation Act [Act No.23 of 1998].
The NRF receives its mandate from the National Research Foundation Act (Act No 23 of 1998, as amended). According to Section 3 of the Act, the object of the NRF is to contribute to national development by:
Chief Executive Officer (CEO)
Deputy Chief Executive Officer: National Research Infrastructure Platforms.
Group Executive: Finance and Business Systems and (CFO)
Deputy CEO: Research and Innovation Support and Advancement (RISA)
Group Executive: Science Engagement and Corporate Relations
Group Executive: Strategy Planning and Partnerships
Group Executive: Human Resources and Legal Services
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Africa’s leading research facility for accelerator based science. Probing fundamental structure and the origins of matter; Advancing the understanding of condensed matter; Impacting the Societal need through provision for the health and environmental sector
The iThemba Laboratory for Accelerator Based Sciences is the continents' biggest facility for particle and nuclear research.
The SAAO is a national facility of the NRF and the national centre for optical and infrared astronomy in South Africa.
SAEON is a national platform for detecting, translating and predicting environmental change.
SAIAB provides unique skills and infrastructure support in marine, estuarine and freshwater ecosystems research, molecular research, collections and bioinformatics.
SARAO is a national facility of the NRF and incorporates radio astronomy instruments and programmes such as MeerKAT and KAT-7 telescopes in the Karoo, (HartRAO) in Gauteng...
South Africa’s innovation revolution must assist in solving our society’s deep and pressing socio-economic challenges. Global competitiveness, shrinking resource availability, and the requirements of a skilled labour force mean that, increasingly, an awareness and understanding of why science and research are critical to our lives is essential for developing an innovation culture.
Within the next five years, the aim is to begin to more fully embed engagement in and with science in the core NRF missions of supporting and promoting new knowledge and growing new knowledge workers. This is led by the formulation of an acceptable NRF position on engaged research which will guide the NRF approach…
NRF | SAASTA is the NRF business division tasked with leading and coordinating the science engagement programme across the NRF and beyond. The NRF is equally committed to ensuring that the science engagement leadership and national coordination role…
The NRF provides leading-edge research infrastructure platforms that ensure that the national research enterprise has the requisite infrastructure to undertake globally competitive discovery science, train the next generation of researchers, support engagement with science by and with the public and promote innovation that positively impacts society, the environment, the economy.
The annual NRF Awards recognize and celebrate South African research excellence. The awards presented to researchers are in two categories, the ratings linked awards and special recognition awards.
The National Research Foundation (NRF) conducts its procurement of goods, services, and works in accordance with its Supply Chain Management Policy in a manner that is fair, equitable, transparent, competitive, and cost-effective
The National Research Foundation (NRF) is guided by its Supply Chain Management Policy in its procurement of goods and services. The Policy sets out the prescripts issued by National Treasury with the exact note referenced in the footnotes. The Supply Chain Management policy adheres to the National Treasury’s prescribed supply chain system framework.
The NRF’s Supply Chain Management Policy and the conduct of supply chain management at the NRF seeks to give effect to section 217 of the South African Constitution which requires that all procurement of goods and services must be done in a manner that is fair, equitable, transparent, competitive and cost-effective.
The National Research Foundation bid awards and contracts. Below is the latest award.
New observations and simulations show that jets of high-speed particles emitted by the central massive black hole in brightest galaxy in galaxy clusters can be used to map the structure of invisible inter-cluster magnetic fields. These findings provide astronomers with a new tool for investigating previously unexplored aspects of clusters of galaxies.
As clusters of galaxies grow through collisions with surrounding matter, they create bow shocks and wakes in their dilute plasma. The plasma motion induced by these activities can drape intra-cluster magnetic layers, forming virtual walls of magnetic force. These magnetic layers, however, can only be observed indirectly when something interacts with them. Because it is simply difficult to identify such interactions, the nature of intra-cluster magnetic fields remains poorly understood. A new approach to map/characterize magnetic layers is highly desired.
An international team of astronomers including Haruka Sakemi, a graduate student at Kyushu University (now a research fellow at the National Astronomical Observatory of Japan – NAOJ), used the MeerKAT radio telescope located in the Northern Karoo desert of South Africa to observe a bright galaxy in the merging galaxy cluster Abell 3376 known as MRC 0600-399.
Located more than 600 million light-years away in the direction of the constellation Columba, MRC 0600-399 is known to have unusual jet structures bent to 90-degree angles. Previous X-ray observations revealed that MRC 0600-399 is the core of a sub-cluster penetrating the main cluster of galaxies, indicating the presence of strong magnetic layers at the boundary between the main and sub-clusters. These features make MRC 0600-399 an ideal laboratory to investigate interactions between jets and strong magnetic layers.
The MeerKAT observations revealed unprecedented details of the jets, most strikingly, faint “double-scythe” structure extending in the opposite direction from the bend points and creating a “T” shape. These new details show that, like a stream of water hitting a pane of glass, this is a very chaotic collision. Dedicated computer simulations are required to explain the observed jet morphology and possible magnetic field configurations.
Takumi Ohmura, a graduate student at Kyushu University (now a research fellow at the University of Tokyo’s Institute for Cosmic-Ray Research – ICRR), from the team performed simulations on NAOJ’s supercomputer ATERUI II, the most powerful computer in the world dedicated to astronomical calculations. The simulations assumed an arch-like strong magnetic field, neglecting messy details like turbulence and the motion of the galaxy.
This simple model provides a good match to the observations, indicating that the magnetic pattern used in the simulation reflects the actual magnetic field intensity and structure around MRC 0600-399. More importantly, it demonstrates that the simulations can successfully represent the underlying physics so that they can be used on other objects to characterize more complex magnetic field structures in clusters of galaxies. This provides astronomers with a new way to understand the magnetized Universe and a tool to analyze the higher-quality data from future radio observatories like the SKA (the Square Kilometre Array).
These results appeared as Chibueze, Sakemi, Ohmura, et. al. “Jets from MRC 0600-399 bent by magnetic fields in the cluster Abell 3376” in Nature on May 6, 2021.
African languages key to the transformation of Africa
The Global Research Council launches first of its kind Report on Gender-Disaggregated Data
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