Determination of optimal rate of nitrogen for chewing sugarcane production in the southern Guinea Savanna of Nigeria

Sugar Tech ◽  
2008 ◽  
Vol 10 (3) ◽  
pp. 278-279
Author(s):  
A. K. Gana
2020 ◽  
Vol 34 (6) ◽  
pp. 801-806
Author(s):  
Kshitij Khatri ◽  
Nathan S. Boyd

AbstractMetam potassium (metam-K) is a soil fumigant used commonly in Florida at the end of the tomato and pepper production season. The fumigant essentially cleans a field by killing the established weeds and crops after harvest. The goal of this project was to determine the optimal rate of metam-K for the effective termination of tomato, pepper, and established weeds such as purple nutsedge, goosegrass, and dogfennel. Tomato, pepper, and purple nutsedge at bed center were effectively terminated with the metam-K rate of 65 kg ha−1. Optimal rates required for the termination of goosegrass and dogfennel were 91 and 156 kg ha−1, respectively. In contrast, metam-K at 500 to 680 kg ha−1 was required to terminate purple nutsedge on bed edges. The reduced efficacy of metam-K at bed edge might be related to the limited movement of metam-K in soil.


Sugar Tech ◽  
2000 ◽  
Vol 2 (3) ◽  
pp. 9-19 ◽  
Author(s):  
A. P. Keerthipala ◽  
N. Dharmawardene

1953 ◽  
Vol 31 (4) ◽  
pp. 326-337
Author(s):  
J. S. Barlow ◽  
J. F. Manery

A procedure has been described whereby the Perkin-Elmer flame photometer, Model 52A, can be used to analyze 10 ml. of a solution of ashed biological materials, the solution containing 0.5 m.e. of sodium or potassium per liter. The lithium concentration used for the internal standard, the optimal rate of flow through the atomizer, the air and gas pressures, and cation interferences are discussed. Applying the modifications and precautions adopted in this laboratory the results of photometer analyses of tissues and serum were shown to compare favorably with those obtained from well-established chemical methods. The merits and demerits of both procedures are outlined.


1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


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