scholarly journals A Post-Keynesian Stock-Flow Consistent Macroeconomic Growth Model: Preliminary Results

2004 ◽  
Author(s):  
Claudio H. Dos Santos ◽  
Gennaro Zezza
Keyword(s):  
Growth Model ◽  
Preliminary Results ◽  
Stock Flow ◽  
Macroeconomic Growth

scholarly journals Harrod–Domar Growth Model with Memory and Distributed Lag

Axioms ◽  
2019 ◽  
Vol 8 (1) ◽  
pp. 9 ◽  
Author(s):  
Vasily E. Tarasov ◽  
Valentina V. Tarasova
Keyword(s):  
Asymptotic Behavior ◽  
Time Delay ◽  
Growth Model ◽  
National Income ◽  
Fading Memory ◽  
Distributed Lag ◽  
Distributed Time Delay ◽  
Fractional Differential ◽  
With Memory ◽  
Macroeconomic Growth

In this paper, we propose a macroeconomic growth model, in which we take into account memory with power-law fading and gamma distributed lag. This model is a generalization of the standard Harrod–Domar growth model. Fractional differential equations of this generalized model with memory and lag are suggested. For these equations, we obtain solutions, which describe the macroeconomic growth of national income with fading memory and distributed time-delay. The asymptotic behavior of these solutions is described.

Remote sensing input to GIS-integrated cotton growth model: preliminary results

2004 ◽  
Author(s):  
Swapna Gogineni ◽  
J. Alex Thomasson ◽  
Javed Iqbal ◽  
James R. Wooten ◽  
Bulli M. Kolla ◽  
...  
Keyword(s):  
Remote Sensing ◽  
Growth Model ◽  
Preliminary Results

A SIMPLIFIED, ‘BENCHMARK’, STOCK-FLOW CONSISTENT POST-KEYNESIAN GROWTH MODEL

2008 ◽  
Vol 59 (3) ◽  
pp. 441-478 ◽  
Author(s):  
Claudio H. Dos Santos ◽  
Gennaro Zezza
Keyword(s):  
Growth Model ◽  
Stock Flow

The O–C diagrams of minor planets − a new approach to modelling the rotation

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss
Keyword(s):  
Error Analysis ◽  
Time Dependence ◽  
Theoretical Work ◽  
Minor Planet ◽  
Minor Planets ◽  
New Approach ◽  
Preliminary Results ◽  
Ccd Observations

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.

Cyclic Evolution of Sunspots: Gleaning New Results from Old Data

2000 ◽  
Vol 179 ◽  
pp. 163-165
Author(s):  
S. K. Solanki ◽  
M. Fligge ◽  
P. Pulkkinen ◽  
P. Hoyng
Keyword(s):  
Sunspot Number ◽  
Sunspot Cycle ◽  
Preliminary Results ◽  
Butterfly Diagram

AbstractThe records of sunspot number, sunspot areas and sunspot locations gathered over the centuries by various observatories are reanalysed with the aim of finding as yet undiscovered connections between the different parameters of the sunspot cycle and the butterfly diagram. Preliminary results of such interrelationships are presented.

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