The South and Alternative Models of Trade and Investment Regulation

Author(s):  
Vivienne Bath
2003 ◽  
Vol 60 (5) ◽  
pp. 1159-1164 ◽  
Author(s):  
M Castro ◽  
P Encarnação ◽  
P Henriques

Abstract The increment at molt for Nephrops norvegicus was studied with the objective of obtaining a model for prediction of post-molt size based on pre-molt size for the population from the south coast of Portugal. Wild animals were maintained in a specially prepared laboratory facility until they molted. Individual values of increment at molt were obtained and used to evaluate alternative models and estimate their parameters. Six alternative models, used previously by several authors to relate pre- and post-molt size, were modified so that increment at molt was the dependent variable and pre-molt size the independent variable. These included the linear relationship of the growth factor (GF) on pre-molt size, the Hiatt equation, post-molt size a power function of pre-molt size, the hyperbolic function, GF exponential function of pre-molt size and the Misra equation. The analysis of the data showed that none of the models could be used to predict increment at molt for either sex. The distribution of the increment at molt was a random normal variable, with mean values not significantly different between sexes, 2.78 mm for males and 2.26 mm for females, variances 0.47 and 0.59, respectively. An analysis of the models suggests that using post-molt size or the GF as dependent variables may lead to a misinterpretation of the dependency of these variables on pre-molt size. It is suggested that the increment at molt should be the variable of interest for predicting post-molt size. The choice of a mathematical formulation should, besides having biological meaning, have the capacity of expressing a true relationship between increment at molt and pre-molt carapace length, namely, be able to model several options for the increment at molt after maturity, including a steady increase of the increment through life, the stabilization of the increment after maturity or the decrease of the increment for larger sizes.


Space Policy ◽  
2019 ◽  
Vol 47 ◽  
pp. 212-216
Author(s):  
Syeun Kim ◽  
Eun-Jung Choi ◽  
Sungki Cho ◽  
Jeong Yoo Hong

1979 ◽  
Vol 13 (1) ◽  
pp. 19-40 ◽  
Author(s):  
S. Arasaratnam

The English East India Company's Coromandel trade provided a spectacle of steady, if unspectacular, growth from its first inauguration early in the seventeenth century. It was not subject to the violent ups and downs, or the extremes of great success and utter failure that characterized the Company's trade in some other regions of India and Southeast Asia. An expanding trade on this coast was matched by an expanding presence. By the end of the century it was well-founded in two substantial Forts (St George and St David) and a number of residencies in important ports of outlet from Vizagapatnam in the north to Cuddalore in the south. By investment and enterprise, by diplomacy and force, English interests and influence on the coast grew and their settlements became nodal points of Indo-British exchange and interaction. The timely demonstration of controlled power, both when faced with threats from the ‘country’ powers of the hinterland and from European rivals on the seafront, helped in the growth of these settlements beyond mere centres of trade. Providing, as they did, not merely trade and investment, but also security of person and property, they were naturally an attraction to many groups in Indian society in the hinterland.


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.


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