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10 February 2025 Photo Supplied
Prof Theo Neethling
Prof Theo Neethling is from the Department of Political Studies and Governance at the University of the Free State.

Opinion article by Prof Theo Neethling, Department of Political Studies and Governance, University of the Free State.


In recent days, 14 South African soldiers have died in clashes with the Rwandan-backed M23 rebels in the eastern Democratic Republic of Congo (DRC). Several analysts argue that this marks a low point for the South African National Defence Force (SANDF) and that it is almost too late to implement the reforms needed to restore the military to an institution South Africans can once again take pride in. The incident recalls the so-called Battle of Bangui in March 2013 during the Central African Republic civil war — a major defeat for the SANDF that led to the Séléka rebels seizing control of the country.

This article aims to shed light on the challenges facing the South African military.

Following the historic transition of 1994, South Africa’s foreign policy shifted from a stance of conflict with its neighbours to one centred on regional relations built on the principles of common destiny, friendship, cooperation, and conflict resolution. The South African government sought to take on a leadership role on the continent, creating new opportunities for the SANDF as a military instrument.

Towards the end of the Mandela presidency, South Africa’s involvement in peace and security operations became a defining feature of its post-1994 foreign policy. The government demonstrated its firm commitment to regional stability by deploying the SANDF in peacekeeping operations — first in Lesotho in 1998, followed by the DRC in 1999 and Burundi in 2001.

Dwindling defence budget

However, since 1998 it became evident that the SANDF found it increasingly difficult to conduct operations as a declining budget started to constrain the SANDF. This is linked to the fact that between 1995 and 1998, the defence budget was cut by 11.1%, which eventually resulted in a growing mismatch between policy intent and execution. As a percentage of gross domestic product (GDP) South African defence spending had been reduced to less than 3% in the mid-1990s, which boiled down to less than 10% of total government spending. The defence budget then further decreased to 1.54% of GDP in 2004/05 and levelled out in 2014/15 at around 1.2% to 1.1% of GDP.

Despite a dwindling defence budget, the government increasingly expected the SANDF to support the SAPS as murder and death rates rose to levels comparable to — or in some cases even exceeding — those in high-intensity war zones internationally. This has placed the SANDF in an almost impossible position, forced to balance its demanding regional deployments with ongoing appeals from politicians and the public to intervene in crime-ridden hotspots where the SAPS is unable to fulfil its constitutional duty to protect South Africans.

Given these constraints and the changing global and regional geopolitical landscape in which the SANDF operated, the government appointed a task team to draft a second defence review, following the South African Defence Review of 1998, which was finally published as the 2015 South African Defence Review. The task team made it clear that the decrease in funding levels was highly problematic, and that inadequate funding would eventually severely compromise the defence capabilities of the SANDF. They emphasised that the government had to decide on one of two options: approving a greater budget allocation to the SANDF or alternatively opting for a significantly scaled-down level of ambition and commitment which is aligned to the budget allocation. One thing was clear: South Africa’s spending was low in terms of comparative international military spending practice. Since 2015 defence spending in South Africa has declined even further to about 0.7% of GDP, which is way below the international norm of more or less 2% of GDP.

Despite its budgetary challenges, in 2023, the SANDF was the fifth largest troop-contributing nation in the UN’s operation in the eastern DRC and played a key role in the SADC operation against insurgents in northern Mozambique from 2021 to 2024. However, considering the history of SANDF operations, a major problem is that the SANDF’s deployments tend to be open-ended, resulting in protracted deployments with serious implications for the defence budget. Moreover, there is no plan to either opt for an adequate defence budget on the one hand, or to scale down the level of political ambition on the other.

It should also be noted that border protection and support for the South African Police Service (SAPS) in internal operations have become increasingly important and demanding in the SANDF’s activities and responsibilities and can even be regarded as among its primary functions. However, a major concern is that the SANDF is too often used as a stopgap in South Africa’s domestic security landscape — hindering its ability to function as a professional, well-equipped armed force with a clear mandate.

For instance, in 2023, politicians called on the SANDF to assist in combating violence linked to zama zamas after the government deployed soldiers in large numbers to curb illegal mining activities. Even local communities expect the government to utilise the SANDF internally, adding pressure on the state to consider such deployments. In this context, the SANDF has little choice but to respond to political calls to assist the SAPS in maintaining internal security. Another recent example of internal deployment was the government’s decision in 2023 to deploy the SANDF to safeguard the coal power plants of South Africa’s major power utility, Eskom.

In conclusion, it should be clear from the above that there is a significant mismatch between what is expected of the SANDF at the political level and its budget and capabilities. The challenge for the SANDF is that defence remains central to its raison d’être, yet it must also be ready to respond to political calls for assistance in peace and security operations across the continent. Additionally, the SANDF is expected to support the SAPS in providing security services in a crime-ridden and fragile South African society — all while operating on a budget of approximately 0.7% of the country’s GDP. It is therefore no surprise that the SANDF is often described as institutionally overstretched and has, in fact, been in a state of ongoing decline for some time.

Critics can rightly argue that the South African government has shown little to no political will to address the SANDF’s financial challenges over the past two decades, contributing to the difficulties its members face in defending themselves against the M23 rebels in the DRC. At the same time, growing fiscal pressures and severe socio-economic challenges leave the government in a weak position to significantly increase the defence budget. Be that as it may, the SANDF’s troubles in the DRC mark a low point for the institution. Perhaps now is the time to reassess both its mandate and funding, particularly in light of the persistent gap between political expectations and available resources.

News Archive

UFS physicists publish in prestigious Nature journal
2017-10-16

Description: Boyden Observatory gravitational wave event Tags: Boyden Observatory, gravitational wave event, Dr Brian van Soelen, Hélène Szegedi, multi-wavelength astronomy 
Hélène Szegedi and Dr Brian van Soelen are scientists in the
Department of Physics at the University of the Free State.

Photo: Charl Devenish

In August 2017, the Boyden Observatory in Bloemfontein played a major role in obtaining optical observations of one of the biggest discoveries ever made in astrophysics: the detection of an electromagnetic counterpart to a gravitational wave event.
 
An article reporting on this discovery will appear in the prestigious science journal, Nature, in October 2017. Co-authors of the article, Dr Brian van Soelen and Hélène Szegedi, are from the Department of Physics at the University of the Free State (UFS). Both Dr Van Soelen and Szegedi are researching multi-wavelength astronomy.
 
Discovery is the beginning of a new epoch in astronomy
 
Dr van Soelen said: “These observations and this discovery are the beginning of a new epoch in astronomy. We are now able to not only undertake multi-wavelength observations over the whole electromagnetic spectrum (radio up to gamma-rays) but have now been able to observe the same source in both electromagnetic and gravitational waves.”
 
Until recently it was only possible to observe the universe using light obtained from astronomical sources. This all changed in February 2016 when LIGO (Laser Interferometer Gravitational-Wave Observatory) stated that for the first time they had detected gravitational waves on 14 September 2015 from the merger of two black holes. Since then, LIGO has announced the detection of two more such mergers. A fourth was just reported (27 September 2017), which was the first detected by both LIGO and Virgo. However, despite the huge amount of energy released in these processes, none of this is detectable as radiation in any part of the electromagnetic spectrum. Since the first LIGO detection astronomers have been searching for possible electromagnetic counterparts to gravitational wave detections. 
 
Large international collaboration of astronomers rushed to observe source
 
On 17 August 2017 LIGO and Virgo detected the first ever gravitational waves resulting from the merger of two neutron stars. Neutron star mergers produce massive explosions called kilonovae which will produce a specific electromagnetic signature. After the detection of the gravitational wave, telescopes around the world started searching for the optical counterpart, and it was discovered to be located in an elliptical galaxy, NGC4993, 130 million light years away. A large international collaboration of astronomers, including Dr Van Soelen and Szegedi, rushed to observe this source.
 
At the Boyden Observatory, Dr Van Soelen and Szegedi used the Boyden 1.5-m optical telescope to observe the source in the early evening, from 18 to 21 August. The observations obtained at Boyden Observatory, combined with observations from telescopes in Chile and Hawaii, confirmed that this was the first-ever detection of an electromagnetic counterpart to a gravitational wave event. Combined with the detection of gamma-rays with the Fermi-LAT telescope, this also confirms that neutron star mergers are responsible for short gamma-ray bursts.  
 
The results from these optical observations are reported in A kilonova as the electromagnetic counterpart to a gravitational-wave source published in Nature in October 2017.
 
“Our paper is one of a few that will be submitted by different groups that will report on this discovery, including a large LIGO-Virgo paper summarising all observations. The main results from our paper were obtained through the New Technology Telescope, the GROND system, and the Pan-STARRS system. The Boyden observations helped to obtain extra observations during the first 72 hours which showed that the light of the source decreased much quicker than was expected for supernova, classifying this source as a kilonova,” Dr Van Soelen said.

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