FTS-SPM: A Software Process Model for Follow the Sun Development: Preliminary Results

Author(s):  
Josiane Kroll ◽  
Ita Richardson ◽  
Jorge Luis Nicolas Audy
2015 ◽  
Author(s):  
Josiane Kroll ◽  
Jorge L. N. Audy

O desenvolvimento Follow the Sun é visto como uma potencial estratégia para o desenvolvimento de projetos de software globais. Esse tipo de desenvolvimento de software ajuda a reduzir o ciclo de vida de desenvolvimento de software. Entretanto, enquanto esse conceito é descrito como promissor na teoria, ele é difícil de ser aplicado em prática. Muitas empresas de software tentaram aplicar o desenvolvimento Follow the Sun, mas depois abandonaram pela dificuldade de colocá-lo em prática. Neste, artigo, é apresentado um modelo de processo de software para a adoção do desenvolvimento Follow the Sun em projetos de software globais. O modelo foi chamado FTS-SPM (Follow the Sun Software Process Model). Ele é composto por seis subprocessos e vinte e uma boas práticas de software. A sua adoção contribui para aumentar a probabilidade de sucesso com a implementação do desenvolvimento Follow the Sun em empresas de software e também contribui para enfrentar os diferentes desafios do desenvolvimento global de software.


1909 ◽  
Vol 6 (4) ◽  
pp. 145-148 ◽  
Author(s):  
E. H. L. Schwarz

Dr. J. R. Sutton has recently read a most important paper to the Royal Society of South Africa on the diurnal variation of level at Kimberley. The paper gave the preliminary results of observations made during the course of three years upon the variation of the level of the ground as recorded by a large horizontal pendulum of a special design made for the author by the Cambridge Instrument Company. It appeared from the results that the movements in the surface of the ground, which set up corresponding movements in the pendulum, were very great. The maximum westerly elongation of the extremity of the pendulum occurred about 5.30 a.m., the maximum easterly about 4.15 p.m., the medium positions a little before 11 a.m. and 9.30 p.m. Geometrically these movements may be represented on the hypothesis that the hemisphere facing the sun bulges out, forming a sort of meniscus to the geosphere. The rise and fall of the surface of the ground which such a supposition would postulate is enormous, and the very magnitude has led Dr. Sutton to hesitate in giving the figures. There can, however, be very little doubt that some rise and fall in the earth's surface is occasioned by the sun's gravitational pull, although the present figures may have to be lessened by taking into consideration other causes which contribute to the disturbance of the pendulum.


2014 ◽  
Vol 90 (5) ◽  
pp. 1-7 ◽  
Author(s):  
Lata Nautiyal ◽  
Neena Gupta

2021 ◽  
Vol 922 (2) ◽  
pp. 104
Author(s):  
Raymond G. Carlberg ◽  
Carl J. Grillmair

Abstract The proper motions of stars in the outskirts of globular clusters are used to estimate cluster velocity dispersion profiles as far as possible within their tidal radii. We use individual color–magnitude diagrams to select high-probability cluster stars for 25 metal-poor globular clusters within 20 kpc of the Sun, 19 of which have substantial numbers of stars at large radii. Of the 19, 11 clusters have a falling velocity dispersion in the 3–6 half-mass radii range, 6 are flat, and 2 plausibly have a rising velocity dispersion. The profiles are all in the range expected from simulated clusters that started at high redshift in a zoom-in cosmological simulation. The 11 clusters with falling velocity dispersion profiles are consistent with no dark matter above the Galactic background. The six clusters with approximately flat velocity dispersion profiles could have local dark matter, but are ambiguous. The two clusters with rising velocity dispersion profiles are consistent with a remnant local dark matter halo, but need membership confirmation and detailed orbital modeling to further test these preliminary results.


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