The South African National Space Agency is South Africa's government agency responsible for the promotion and development of aeronautics and aerospace space research. It fosters cooperation in space-related activities and research in space science, seeks to advance scientific engineering through human capital, as well as the peaceful use of outer space, and supports the creation of an environment conducive to the industrial development of space technologies within the framework of national government.SANSA was established on 9 December 2010 by the National Space Agency Act.Currently, SANSA's main focusses include using data obtained from remote sensing through satellites and other projects to provide assessment on flooding, fires, resource management and environmental phenomena in South Africa and the African continent. Wikipedia.
News Article | May 11, 2017
From Creamer Media in Johannesburg, this is the Real Economy Report. Sashnee Moodley: The South African National Space Agency has signed a Memorandum of Understanding with the NEPAD Agency. Keith Campbell reports. Keith Campbell: In April, the South African National Space Agency, or Sansa, signed a Memorandum of Understanding with the NEPAD Planning and Coordination Agency. Raoul Hodges, Managing Director of Sansa’s Space Operations Directorate, explains the significance of this MoU. Keith Campbell: For Sansa Space Operations, the past year has been an active one. Hodges tells us more. Sashnee Moodley: Other news making headlines: Davies promises support for downstream firms as he confirms steel safeguard duty Speaking in Johannesburg at the release of the ninth Industrial Policy Action Plan Trade and Industry Minister Dr Rob Davies reiterated the importance of sustaining a primary steel industry, which had come under intense pressure as a result of the current global oversupply of steel. Sashnee Moodley: That’s Creamer Media’s Real Economy Report. Join us again next week for more news and insight into South Africa’s real economy.
Kotze P.B.,The South African National Space Agency
Earth, Planets and Space | Year: 2017
Rapid secular variation pulses in the Earth's geomagnetic field have been identified during the last decade. In particular, the 2014 jerk is the latest in a series of localised rapid secular variation events observed at the Earth's surface which are thought to be the result of rapid oscillations at the core surface approximately at a depth of 3000 km. In Southern Africa, the 2014 jerk has been analysed using data from four observatories located at Hermanus, Hartebeesthoek, Keetmanshoop and Tsumeb and found that this event occurred with varying strengths in the different components at a particular observatory, while different observatories in the region showed strong individual characteristics. The changes in the secular variation patterns at individual magnetic observatories in this study took place in an area characterised by rapid changes in the geomagnetic field with time. Of particular interest is that global field models like CHAOS-6 and POMME 10 derived from various combinations of ground and satellite data do not always indicate similar short-period patterns in X, Y and Z as revealed by observatory measurements. This has been confirmed by comparing the secular variation pattern at the Kourou magnetic observatory located in French Guiana, a station close to the current centre of the South Atlantic Anomaly. © 2017 The Author(s).
Kotze P.B.,The South African National Space Agency
Earth, Planets and Space | Year: 2017
Global geomagnetic field models using spherical harmonic basis functions are important in space physics research, space weather and applications like navigation and mineral resources exploration. These models are based on various geomagnetic field data sets ranging from Earth surface magnetic observatory measurements to low-Earth orbit satellites equipped with highly sensitive and accurate magnetometers. Although these field models are derived by fitting harmonic functions to data distributed across the Earth, they are applied on regional scales within fixed boundaries in many instances and one can therefore question how well do these models perform on restricted areas. Three recently published global geomagnetic field models, IGRF-12, CHAOS-6 and POMME-10, have been statistically evaluated over Southern Africa using repeat station data as well as measurements from 4 INTERMAGNET observatories located at Hermanus and Hartebeesthoek in South Africa as well as Tsumeb and Keetmanshoop in Namibia for 2015. Apart from the observatory data, the field survey repeat station data do not form part of the data set on which these global field models are based and therefore can be regarded as an independent test of these field models over an area like Southern Africa which is well known for its rapid change of the geomagnetic field. Results obtained in this investigation for both main field and secular variation models clearly showed the importance of timely ground-based geomagnetic field observations in the derivation of accurate field models, particularly in regions characterised by rapid and unpredictable secular variation changes. © 2017 The Author(s).
Agency: European Commission | Branch: FP7 | Program: CSA-SA | Phase: ENV.2009.4.1.4.1 | Award Amount: 1.21M | Year: 2009
The purpose of the GEO Network for Capacity Building (GEO-Net-CaB) project is to create the conditions for the improvement and increase of the GEO capacity building activities and framework, with special emphasis on developing countries, new EU member states (and EU neighbouring states) and climate monitoring and will serve the bigger goal of improved effectiveness and efficiency of GEO capacity building for application in the GEO societal benefit areas. Coinciding with this purpose, successful brokerage with (potential) clients for earth observation products and services will be facilitated. The project will deliver the following output: 1. Capacity building needs in earth observation are identified (at a generic and global level, but with emphasis on the target regions). 2. Specifications for earth observation capacity buildings are described. 3. Resource providers are identified. 4. Sustainable brokerage between stakeholders (including resource providers) is established. 5. A mechanism to facilitate cooperation between stakeholders and providers is established. 6. A global base of technical expertise for education and training in earth observation is established (with emphasis on developing countries, new EU member states and climate monitoring). 7. Monitoring and evaluation mechanisms for determining the efficacy of GEO capacity building efforts are established. To achieve maximum impact demonstration projects will be carried out in Southern Africa, the French-speaking African region, Czechia and Poland, with spin-offs to EU neighbouring countries and Latin America and Asia. The project (with a duration of three years) will be carried out by a strong consortium of partners from the Netherlands, France, South Africa, Morocco, Czechia and Poland, supervised by an advisory board with worldwide representation and strong connections to GEO.
Agency: European Commission | Branch: FP7 | Program: CP | Phase: SPA.2010.2.3-1 | Award Amount: 2.63M | Year: 2011
The security of space assets are affected by the high-energy charged particle environment in the radiation belts. The controlling principal source and loss mechanisms in the radiation belts are not yet completely understood. During a geomagnetic storm the length of time during which space assets are in danger is determined by the loss mechanisms, particularly by relativistic electron precipitation. The primary mechanism for this precipitation is the interaction of several wave modes with resonant electrons which leads to scattering into the atmospheric loss cone. The nature of the wave activity and the interactions between the waves and radiation belt particles are strongly governed by the properties of the plasmasphere. At this point there are few existing and regular measurements of plasmaspheric properties, with existing plasmaspheric models lacking the structures known to exist in the real plasmasphere. There is evidence that enhanced wave activity and enhanced radiation belt losses occur due to such structures. In addition, there are large uncertainties concerning the fundamental nature of relativistic electron precipitation (REP), due to the difficulties of undertaking quality in-situ measurements. To address these uncertainties in this proposed project we will provide regular longitudinally-resolved measurements plasmaspheric electron and mass densities and hence monitor the changing composition of the plasmasphere, one of the properties which determines wave growth. This will allow us to develop a data assimilative model of the plasmasphere. At the same time, we will monitor the occurrence and properties of REP, tying the time-resolved loss of relativistic electrons to the dynamic plasmasphere observations. Our approach will primarily use ground-based networks of observing stations, operating in the ULF and VLF ranges, deployed on a worldwide level. Our proposal is made up of 6 work packages to meet these science goals.
Agency: European Commission | Branch: FP7 | Program: CSA-SA | Phase: SPA.2009.3.2.01 | Award Amount: 1.34M | Year: 2010
To enable and enhance the ability of African states to use satellite Earth Observation for the management of natural and man-made humanitarian emergencies. To develop a network of EU, African organisations and African users, in order to build economic, technical and commercial capacity within African states, along the priority lines being identified in consultation with the African Union under the GMES and Africa initiative.
Agency: European Commission | Branch: FP7 | Program: CSA-CA | Phase: ENV.2013.6.5-2 | Award Amount: 1.17M | Year: 2013
The purpose of the EOPOWER project is to create conditions for sustainable economic development through the increased use of Earth observation products and services for environmental applications. This purpose serves the higher goal of effective use of Earth observation for decision making and management of economic and sustainable development processes. This will be achieved through the following activities: 1. Roadshow activities to promote the increased use of EO products and services for environmental applications, including capacity building; 2. Portfolio of potential EO applications for economic development and environmental management; 3. Enhancement of the resource facility on capacity building in the GEO web portal; 4. Establishment of local focal points (nodes) that actively promote and provide capacity building on the use of EO for environmental applications effectively and at low-cost; 5. Explore the establishment of a high-level forum of stakeholders (resource providers, international organizations) that have an interest in EO for economic development and environmental applications; 6. Establishment of a central feedback node that digests and shares information on incubators, innovation, successes, experiences, visibility and provides brokerage and advice on resource mobilization. This will result in the output presented below: 1. Opportunities created for economic development, in particular in developing countries; 2. Key international economic development processes identified that require environmental information and mechanisms to develop them in a sustainable fashion; 3. Local communities and authorities have received capacity building and are able to collaborate with international development programs, use environmental EO information and products, and engage resource providers; 4. Mechanism established to market and exploit EO applications for the creation of new innovative products and support services.
Malahlela O.E.,The South African National Space Agency
International Journal of Remote Sensing | Year: 2016
Surface waterbodies in arid and semi-arid environments are threatened by both natural and anthropogenic pressures. Mapping the distribution of surface waterbodies is crucial for managing their dwindling quantities and quality. In this study, a fast and reliable method of water extraction has been introduced. A remote-sensing index called the simple water index (SWI) was formulated to differentiate waterbodies from vegetation class automatically, and to differentiate waterbodies from shadows or built-up areas (water-like features). Its performance was compared with the automated water extraction index (AWEI) and the modified normalized difference water index (MNDWI) on Landsat 8 Operational Land Imager (OLI) image of South Africa. The robustness of the algorithm was tested on images in Madagascar and the Democratic Republic of Congo (DRC) with different biomes. The overall accuracies and kappa coefficient (κ) were used to compare the performance of each index. The McNemar test was performed to assess the significance of the output map and the validation data set. The SWI showed the highest overall accuracy of 91.9% (κ = 0.83), whereas the AWEI and MNDWI yielded overall accuracies of 83.8% (κ = 0.65) and 78.4% (κ = 0.53), respectively. The McNemar test showed that there was no significant difference between the SWI map (p = 0.248), whereas both AWEI and MNDWI maps were significantly different from the validation data set at p = 0.041 and p = 0.013, respectively. The SWI approach reduces the thresholding problem by 50% over the conventional MNDWI and AWEI. It is expected that the SWI will also be useful for the accurate quantification of waterbodies for large areas. © 2016 Informa UK Limited, trading as Taylor & Francis Group.
Kotze P.B.,The South African National Space Agency
South African Journal of Geology | Year: 2011
Quiet-time mean monthly values from the INTERMAGNET observatory at Hermanus (HER) in South Africa were used to study the changes in secular variation during the period between 2005 and 2009. After removing an annual variation resulting from magnetospheric and ionospheric currents by means of a 12-month running means applied to the respective observatory first differences of the X, Y, and Z components, clear evidence was revealed of a strong geomagnetic jerk that occurred during 2007 in this area. The GRIMM-2X model also provided evidence of the occurrence of this jerk in 2007. Of particular interest is that GRIMM-2X predicts the turning points in all the secular variation trends to occur much earlier than revealed by the observatory data. We also observed that the power of this jerk, determined as the difference in slope of the secular variation before and after the jerk, is several times stronger than the global jerk of 1982/3. © 2011 June Geological Society of South Africa.