Business Leadership in the South

1956 ◽  
Vol 29 (2) ◽  
pp. 130
Author(s):  
Clarence Danhof
Author(s):  
Mogaramedi Frans Mashabela ◽  
Professor. Ray M Kekwaletswe

The adoption and usage of e-filing applications is a phenomenon most governments, including South Africa are still grappling with, and therefore, an ongoing information systems business leadership research is a key issue. The research problem is that despite the e-Government application being implemented and maintained at a high cost, there is little uptake and optimal use. The revenue application has greater benefits such as tax calculation accuracy, tax submission done timeously during any time of the day, improving tax efficiency by reducing administration cost. Since the value and the investment is huge, the burning question is then why the accepting and usage ofe-filing by taxpayers not as it should? Information from previous studies arequite on this phenomenon, in the South Africancontext and this then left a knowledge gaps, which this paper bridges.This paperfocuses on explaining and explore adopting and using e-filing as reasons why some of taxpayers accept and use the revenue application while others are not using it are still unknown. Argument is that despite South Africa implemented a cutting-edgesystemsince 2006, taxpayers still queueat its branches for manualsubmissions.


1962 ◽  
Vol 24 (2) ◽  
pp. 303-322 ◽  
Author(s):  
Bernard Cosman
Keyword(s):  

2000 ◽  
Vol 179 ◽  
pp. 201-204
Author(s):  
Vojtech Rušin ◽  
Milan Minarovjech ◽  
Milan Rybanský

AbstractLong-term cyclic variations in the distribution of prominences and intensities of green (530.3 nm) and red (637.4 nm) coronal emission lines over solar cycles 18–23 are presented. Polar prominence branches will reach the poles at different epochs in cycle 23: the north branch at the beginning in 2002 and the south branch a year later (2003), respectively. The local maxima of intensities in the green line show both poleward- and equatorward-migrating branches. The poleward branches will reach the poles around cycle maxima like prominences, while the equatorward branches show a duration of 18 years and will end in cycle minima (2007). The red corona shows mostly equatorward branches. The possibility that these branches begin to develop at high latitudes in the preceding cycles cannot be excluded.


2014 ◽  
Author(s):  
John Narborough ◽  
Abel Tasman ◽  
John Wood ◽  
Friderich Martens
Keyword(s):  

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