Determination of pendimethalin (PROWL®480 EC) spray drift from ground applications

1996 ◽  
Vol 31 (5) ◽  
pp. 969-985
Author(s):  
B. J. Harris ◽  
B. Reliford ◽  
G. Annette ◽  
K. Jennings
Keyword(s):  
2016 ◽  
Vol 20 (1) ◽  
pp. 79-89
Author(s):  
I.S. Kruk ◽  
O.V. Gordeenko ◽  
T.P Kot ◽  
Andrzej Marczuk ◽  
Jan Kamiński ◽  
...  

AbstractThe objective of the paper is to determine the optimal geometric parameters of the windshield device limiting the spray drift by wind in herbicides spraying. Tests were carried out with the use of the planning methods of experiments and statistical methods of processing of the obtained results. The result of the research consisted in obtaining structural parameters of the windshield made in the shape of gratings with rectangular boards. It was found out that this device may be used at the wind speed exceeding agrotechnological sizes. The research results will be used in the work on devices protecting against wind at a precise herbicides spraying.


2008 ◽  
Vol 61 ◽  
pp. 159-163
Author(s):  
J.A. Zabkiewicz ◽  
K.D. Steele ◽  
J.P. Praat

An alternative method to the use of dyes in spray drift estimation has been developed using different metal cations with each spray solution This removes the need to collect the targets until all the spray events have been completed Spray drift trials were conducted with a tractor plus boom over a grass sward with plastic tape as the collector to capture ground spray deposits The extracted deposits from the collectors were quantified by ICPMS The advantages of using cations are that they are stable very low levels of detection are possible analytical and operational costs are reduced and they are nonphytotoxic at operational amounts


Author(s):  
W. Clint Hoffmann ◽  
Bradley K. Fritz ◽  
William E. Bagley ◽  
Joe Gednalske ◽  
Curt E. Elsik ◽  
...  

Author(s):  
W. Clint Hoffmann ◽  
Bradley K. Fritz ◽  
William E. Bagley ◽  
Joe Gednalske ◽  
Curt E. Elsik ◽  
...  

2020 ◽  
Vol 714 ◽  
pp. 136666 ◽  
Author(s):  
Xavier Torrent ◽  
Eduard Gregorio ◽  
Joan R. Rosell-Polo ◽  
Jaume Arnó ◽  
Miquel Peris ◽  
...  

1993 ◽  
Vol 45 (3-4) ◽  
pp. 283-293 ◽  
Author(s):  
R.H. Marrs ◽  
A.J. Frost ◽  
R.A. Plant ◽  
P. Lunnis
Keyword(s):  

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.


1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.


1961 ◽  
Vol 13 ◽  
pp. 29-41
Author(s):  
Wm. Markowitz
Keyword(s):  

A symposium on the future of the International Latitude Service (I. L. S.) is to be held in Helsinki in July 1960. My report for the symposium consists of two parts. Part I, denoded (Mk I) was published [1] earlier in 1960 under the title “Latitude and Longitude, and the Secular Motion of the Pole”. Part II is the present paper, denoded (Mk II).


1972 ◽  
Vol 1 ◽  
pp. 27-38
Author(s):  
J. Hers

In South Africa the modern outlook towards time may be said to have started in 1948. Both the two major observatories, The Royal Observatory in Cape Town and the Union Observatory (now known as the Republic Observatory) in Johannesburg had, of course, been involved in the astronomical determination of time almost from their inception, and the Johannesburg Observatory has been responsible for the official time of South Africa since 1908. However the pendulum clocks then in use could not be relied on to provide an accuracy better than about 1/10 second, which was of the same order as that of the astronomical observations. It is doubtful if much use was made of even this limited accuracy outside the two observatories, and although there may – occasionally have been a demand for more accurate time, it was certainly not voiced.


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