Estimation of skin pigment concentration from spectral reflectance using the Wiener estimation and color CCD camera

2016 ◽  
Vol 2016.54 (0) ◽  
pp. 5-6
Author(s):  
Shota MIYAZAWA ◽  
Kiyomi SATO ◽  
Hideki FUNAMIZU ◽  
Tomonori YUASA ◽  
Yoshihisa AIZU
Sensors ◽  
2013 ◽  
Vol 13 (6) ◽  
pp. 7902-7915 ◽  
Author(s):  
Izumi Nishidate ◽  
Takaaki Maeda ◽  
Kyuichi Niizeki ◽  
Yoshihisa Aizu

2012 ◽  
Vol 2012.51 (0) ◽  
pp. 167-168
Author(s):  
Kazuma SHIBATA ◽  
Ysuyoshi FURUMIDA ◽  
Hideki FUNEMIZU ◽  
Yoshihisa AIZU

2017 ◽  
Author(s):  
Kiyomi Sato ◽  
Shota Miyazawa ◽  
Hideki Funamizu ◽  
Tomonori Yuasa ◽  
Izumi Nishidate ◽  
...  

1974 ◽  
Vol 14 (66) ◽  
pp. 122
Author(s):  
JR Peterson

CCC ((2-chloroethyl) trimethylammonium chloride) was applied to whole vines at the rates of 0, 300, 600, 1200, or 2400 p.p.m. three and two weeks before flowering and its effects on bunch and berry characteristics of both proximal and distal bunches observed. CCC increased berry number per bunch and bunch weight despite reduced berry weights. Rachis weights were generally decreased, although they increased with the 300 p.p.m. treatment. Fruit maturation, expressed as skin pigment concentration, juice soluble solids, and acidity were delayed. No differences occurred due to time of spray application. Unsprayed proximal bunches carried larger berries, which matured earlier than those on distal bunches. Despite the larger berries on untreated proximal bunches, the skins weighed no more than those on distal bunches and contained similar pigment concentration. Following CCC application, the proximal bunches set more berries, which were no larger than those on distal bunches, so that proximal were heavier than distal bunches (expressed in absolute terms or as a percentage increase). Treatment reduced the soluble solids of proximal but not distal bunches. It also tended to increase proximal rachis weight at concentrations of 300-1 200 p.p.m., but decreased it at 2400 p.p.m. It had no effect on distal bunch rachises when applied at 300 or 600 p.p.m., but decreased the weight at 1200 and 2400 p.p.m.


1999 ◽  
Vol 173 ◽  
pp. 189-192
Author(s):  
J. Tichá ◽  
M. Tichý ◽  
Z. Moravec

AbstractA long-term photographic search programme for minor planets was begun at the Kleť Observatory at the end of seventies using a 0.63-m Maksutov telescope, but with insufficient respect for long-arc follow-up astrometry. More than two thousand provisional designations were given to new Kleť discoveries. Since 1993 targeted follow-up astrometry of Kleť candidates has been performed with a 0.57-m reflector equipped with a CCD camera, and reliable orbits for many previous Kleť discoveries have been determined. The photographic programme results in more than 350 numbered minor planets credited to Kleť, one of the world's most prolific discovery sites. Nearly 50 per cent of them were numbered as a consequence of CCD follow-up observations since 1994.This brief summary describes the results of this Kleť photographic minor planet survey between 1977 and 1996. The majority of the Kleť photographic discoveries are main belt asteroids, but two Amor type asteroids and one Trojan have been found.


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