Effect of White Light on Taxol and Baccatin III Accumulation in Cell Cultures of Taxus cuspidata Sieb and Zucc.

1995 ◽  
Vol 146 (5-6) ◽  
pp. 584-590 ◽  
Author(s):  
Arthur G. Fett-Neto ◽  
Jason J. Pennington ◽  
Frank DiCosmo
2007 ◽  
Vol 62 (1-2) ◽  
pp. 1-10 ◽  
Author(s):  
Chun F. Zhao ◽  
Long J. Yu ◽  
Li Q. Li ◽  
Fu Xiang

Liquid chromatography electrospray ionization tandem mass spectrometry (LC/ESI-MS/ MS) and high-performance liquid chromatography (HPLC) methods have been used to identify and quantify the major taxoids from extracts of Taxus chinensis cell cultures. Chromatography was carried out on a reverse phase C18 column with isocratic-mode elution. By analytically comparing LC/ESI-MS/MS of the extracts with that of the available reference substances and literature, six taxoids were identified as taxuyunnanine C (Tc, 1), yunnanxane (2), 2α,5α,10β-triacetoxy-14β-propionyloxytaxa-4(20),11-diene (3), 2α,5α,10β-triacetoxy-14β- (2-methyl)butyryloxytaxa-4(20),11-diene (4), taxol (5), and baccatin III (B III, 6), respectively. Among them, 2, 3 and 4 were assigned in the absence of the corresponding reference substances, and 3 and 4 were detected in this cell line for the first time. The identification was validated by NMR spectra. The precise quantification of 1 and 5 was made using HPLC. The limit of detection (LOD), 0.5 μg/ml for 5, 1.5 μg/ml for 1, and the linearity and accuracy of the quantitative method were evaluated, indicating a wide linear range and satisfactory accuracy. The amounts of other identified taxoids were calculated on the basis of comparison of the absolute response factors of similar structural substances. The proposed method provides a rapid, conventional and reliable tool to characterize and study cell lines for elucidating the taxane biosynthesis.


1999 ◽  
Vol 4 (2) ◽  
pp. 112-118 ◽  
Author(s):  
Sung Ho Son ◽  
Sung Mee Choi ◽  
Kum Boo Choi ◽  
Yun Hee Lee ◽  
Dea Sook Lee ◽  
...  

2007 ◽  
Vol 33 (2) ◽  
pp. 159-167 ◽  
Author(s):  
Rosa M. Cusidó ◽  
Javier Palazón ◽  
Mercedes Bonfill ◽  
Oscar Expósito ◽  
Elisabet Moyano ◽  
...  

1994 ◽  
Vol 8 (8) ◽  
pp. 547-550 ◽  
Author(s):  
Moon-Kyoon Chun ◽  
Hye-Won Shin ◽  
Huen Lee ◽  
Jang-Ryol Liu

2000 ◽  
Vol 19 (6) ◽  
pp. 628-633 ◽  
Author(s):  
S. H. Son ◽  
S. M. Choi ◽  
Y. H. Lee ◽  
K. B. Choi ◽  
S. R. Yun ◽  
...  

1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož

AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.


1994 ◽  
Vol 144 ◽  
pp. 82
Author(s):  
E. Hildner

AbstractOver the last twenty years, orbiting coronagraphs have vastly increased the amount of observational material for the whitelight corona. Spanning almost two solar cycles, and augmented by ground-based K-coronameter, emission-line, and eclipse observations, these data allow us to assess,inter alia: the typical and atypical behavior of the corona; how the corona evolves on time scales from minutes to a decade; and (in some respects) the relation between photospheric, coronal, and interplanetary features. This talk will review recent results on these three topics. A remark or two will attempt to relate the whitelight corona between 1.5 and 6 R⊙to the corona seen at lower altitudes in soft X-rays (e.g., with Yohkoh). The whitelight emission depends only on integrated electron density independent of temperature, whereas the soft X-ray emission depends upon the integral of electron density squared times a temperature function. The properties of coronal mass ejections (CMEs) will be reviewed briefly and their relationships to other solar and interplanetary phenomena will be noted.


2000 ◽  
Vol 179 ◽  
pp. 197-200
Author(s):  
Milan Minarovjech ◽  
Milan Rybanský ◽  
Vojtech Rušin

AbstractWe present an analysis of short time-scale intensity variations in the coronal green line as obtained with high time resolution observations. The observed data can be divided into two groups. The first one shows periodic intensity variations with a period of 5 min. the second one does not show any significant intensity variations. We studied the relation between regions of coronal intensity oscillations and the shape of white-light coronal structures. We found that the coronal green-line oscillations occur mainly in regions where open white-light coronal structures are located.


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