Determination of the Cross-Reactivities of Immunoassays:  Effect of Common Cross-Reactants for Chlorpyrifos-ethyl in Water Matrices Using Magnetic Particle-Based ELISA

1996 ◽  
Vol 30 (2) ◽  
pp. 513-516 ◽  
Author(s):  
Anna Oubiña ◽  
Jordi Gascón ◽  
Damià Barceló
2021 ◽  
Vol 73 (1) ◽  
Author(s):  
Hirotomo Noda ◽  
Hiroki Senshu ◽  
Koji Matsumoto ◽  
Noriyuki Namiki ◽  
Takahide Mizuno ◽  
...  

AbstractIn this study, we determined the alignment of the laser altimeter aboard Hayabusa2 with respect to the spacecraft using in-flight data. Since the laser altimeter data were used to estimate the trajectory of the Hayabusa2 spacecraft, the pointing direction of the altimeter needed to be accurately determined. The boresight direction of the receiving telescope was estimated by comparing elevations of the laser altimeter data and camera images, and was confirmed by identifying prominent terrains of other datasets. The estimated boresight direction obtained by the laser link experiment in the winter of 2015, during the Earth’s gravity assist operation period, differed from the direction estimated in this study, which fell on another part of the candidate direction; this was not selected in a previous study. Assuming that the uncertainty of alignment determination of the laser altimeter boresight was 4.6 pixels in the camera image, the trajectory error of the spacecraft in the cross- and/or along-track directions was determined to be 0.4, 2.1, or 8.6 m for altitudes of 1, 5, or 20 km, respectively.


2009 ◽  
Vol 10 (8) ◽  
pp. n/a-n/a ◽  
Author(s):  
Christine Franke ◽  
Catherine Kissel ◽  
Eric Robin ◽  
Philippe Bonté ◽  
France Lagroix

1984 ◽  
Vol 30 (3) ◽  
pp. 823-825 ◽  
Author(s):  
R. J. Prestwood ◽  
D. B. Curtis ◽  
D. J. Rokop ◽  
D. R. Nethaway ◽  
N. L. Smith
Keyword(s):  

1995 ◽  
Vol 29 (11) ◽  
pp. 2754-2758 ◽  
Author(s):  
Charles S. Hottenstein ◽  
Scott W. Jourdan ◽  
Mary C. Hayes ◽  
Fernando M. Rubio ◽  
David P. Herzog ◽  
...  

1985 ◽  
Vol 85 ◽  
pp. 137-140
Author(s):  
P.L. Lamy

AbstractThe relevance of the bulk density as a physical parameter characterizing interplanetary dust grains is discussed. The various measurements which lead to a determination of this parameter are reviewed. The specific case of the collected interplanetary dust grains is considered.The bulk density of interplanetary dust grains has been and is still a matter of controversy. This quantity cannot, in general, be directly measured; it is used to relate the mass and the size of a grain. This duality stems from physics itself as there are interactions sensitive to the mass (e.g., gravitational forces) while others are sensitive to the size or the cross-section (e.g., light scattering, radiation pressure, gas and plasma interactions). The measuring technics of the grains reflect this duality as, for instance, impact sensors are generally sensitive to the kinetic energy and thus to the mass, while optical sensors are sensitive to the cross-section. One sees that the density is not strictly speaking the relevant parameter, but what is needed is a relationship between mass and average cross-section.


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