Cespe UnB

Editorial Office:
Management:
R. S. Oyarzabal

Technical Support:
D. H. Diaz
M. A. Gomez
W. Abrahão
G. Oliveira

Publisher by
Knobook Pub






216/168=1.29


1.17

Volume 3, Issue 3 (Nov/Dec 2012)

Editorial Note


Page 1
Lucimara Martins and Paula Coelho
doi: 10.6062/jcis.2012.03.03.EN008(Free PDF)
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57.Current paradigms in parallelization: a comparison of vectorization, OpenMP and MPI
Penteado, P. F.
doi: 10.6062/jcis.2012.03.03.0057(Free PDF)
____________________________________________________________________

58.Two semi-automated computational approaches for spectroscopic analysis of stellar photospheres: detailed characterization at high resolution and abundance determination at medium resolution
Milone A., Da Silva, R., Sanson, A.
doi: 10.6062/jcis.2012.03.03.0058(Free PDF)
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59. A New Approach for Using the Hough Transform to Extract Features from Solar Coronal Images
Walker da Silva, C., Rosa, Reinaldo R., Costa, J. E. R.
doi: 10.6062/jcis.2012.03.03.0059 (Free PDF)
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60. Programing Using High Level Design With Python and FORTRAN: A Study Case in Astrophysics
Pereira, E. S. and Miranda O. D.
doi: 10.6062/jcis.2012.03.03.0060
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61. Initial conditions for N-body/SPH simulations of galaxy cluster mergers
R. E. G. Machado
doi: 10.6062/jcis.2012.03.03.0061(Status: Discussion Paper)
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62. The magnetic field in the Small Magellanic Cloud and in the Magellanic Bridge
A. Lobo Gomes et. al.
doi: 10.6062/jcis.2012.03.03.0062(Status: Discussion Paper)
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63. Use of Python programming language in astronomy and science
D. M. Faes.
doi: 10.6062/jcis.2012.03.03.0063 (Free PDF)
____________________________________________________________________

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doi: 10.6062/jcis.2008.01.01.0005
Freitas and Shimabukuro(Free PDF)

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doi: 10.6062/jcis.2009.01.02.0009
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doi: 10.6062/jcis.2008.01.01.0006
Alcantara.(Free PDF)

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doi: 10.6062/jcis.2008.01.01.0001
Luz et al.((Free PDF)

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