An agglomerative technique for Pearson Type II mixture decomposition with applications

2002 ◽  
Author(s):  
S. Medasani ◽  
R. Krishnapuram ◽  
S. Auphenwiryakul
Keyword(s):  
Type Ii ◽  
Mixture Decomposition ◽  
Pearson Type

scholarly journals Estimation of the precision matrix of multivariate Pearson type II model

Metrika ◽  
2008 ◽  
Vol 69 (1) ◽  
pp. 31-44
Author(s):  
Amadou Sarr ◽  
Arjun K. Gupta ◽  
Anwar H. Joarder
Keyword(s):  
Type Ii ◽  
Precision Matrix ◽  
Pearson Type

Inference under representable priors for Pearson type II models in finite populations

2003 ◽  
Vol 111 (1-2) ◽  
pp. 23-36 ◽  
Author(s):  
Heleno Bolfarine ◽  
Loretta B. Gasco ◽  
Pilar L. Iglesias
Keyword(s):  
Type Ii ◽  
Finite Populations ◽  
Pearson Type

scholarly journals Matric variate Pearson type II-Riesz distribution

2016 ◽  
Vol 28 (4) ◽  
pp. 359-367
Author(s):  
José A. Díaz-García ◽  
Francisco J. Caro-Lopera
Keyword(s):  
Type Ii ◽  
Riesz Distribution ◽  
Pearson Type

Type II Solar Radio Bursts over Solar Cycle 21

1994 ◽  
Vol 144 ◽  
pp. 283-284
Author(s):  
G. Maris ◽  
E. Tifrea
Keyword(s):  
Solar Radio ◽  
Interplanetary Space ◽  
Impulsive Phase ◽  
Radio Bursts ◽  
Type Ii ◽  
Solar Radio Bursts ◽  
Strong Energy ◽  
Mass Ejection ◽  
Geophysical Effect ◽  
Radio Event

The type II solar radio bursts produced by a shock wave passing through the solar corona are one of the most frequently studied solar activity phenomena. The scientific interest in this type of phenomenon is due to the fact that the presence of this radio event in a solar flare is an almost certain indicator of a future geophysical effect. The origin of the shock waves which produce these bursts is not at all simple; besides the shocks which are generated as a result of a strong energy release during the impulsive phase of a flare, there are also the shocks generated by a coronal mass ejection or the shocks which appear in the interplanetary space due to the supplementary acceleration of the solar particles.

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