Comment: Influence of stationary magnetic fields on water relations in lettuce seeds

2002 ◽  
Vol 23 (7) ◽  
pp. 550-550 ◽  
Author(s):  
Robert K. Adair
Planta ◽  
1971 ◽  
Vol 101 (1) ◽  
pp. 1-25 ◽  
Author(s):  
Murray W. Nabors ◽  
Anton Lang

Planta ◽  
1981 ◽  
Vol 152 (2) ◽  
pp. 131-136 ◽  
Author(s):  
Nicholas C. Carpita ◽  
Murray W. Nabors

2020 ◽  
Vol 96 (7) ◽  
pp. 951-957
Author(s):  
Angel De Souza-Torres ◽  
Lilita Sueiro-Pelegrín ◽  
Miguel Zambrano-Reyes ◽  
Idalberto Macías-Socarras ◽  
Mario González-Posada ◽  
...  

Planta ◽  
1979 ◽  
Vol 144 (3) ◽  
pp. 225-233 ◽  
Author(s):  
Nicholas C. Carpita ◽  
Murray W. Nabors ◽  
Cleon W. Ross ◽  
Nancy L. Petretic

Planta ◽  
1971 ◽  
Vol 101 (1) ◽  
pp. 26-42 ◽  
Author(s):  
Murray W. Nabors ◽  
Anton Lang

Planta ◽  
1979 ◽  
Vol 144 (3) ◽  
pp. 217-224 ◽  
Author(s):  
Nicholas C. Carpita ◽  
Murray W. Nabors ◽  
Cleon W. Ross ◽  
Nancy L. Petretic

2001 ◽  
Vol 22 (8) ◽  
pp. 596-602 ◽  
Author(s):  
Francisco Garc�a Reina ◽  
Luis Arza Pascual ◽  
Ilvelisse Almanza Fundora

1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora

AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.


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