Calcium localization in oat aleurone cells using chlorotetracycline and X-ray microanalysis

Planta ◽  
1988 ◽  
Vol 175 (2) ◽  
pp. 237-240 ◽  
Author(s):  
Andrzej Tretyn ◽  
Jan Kopcewicz
1975 ◽  
Vol 23 (2) ◽  
pp. 103-106 ◽  
Author(s):  
T Sato ◽  
L Herman ◽  
J A Chandler ◽  
A Stracher ◽  
T C Detwiler

Electron microscopic x-ray microprobe analysis of pyroantimonate precipitates in platelets fixed in osmium tetroxide-pyroantimonate revealed calcium localization in the nucleoids of alpha-granules. This pool of calcium had largely disappeared within 10 sec after stimulation of platelets by thrombin. Such a rapid change suggests that this calcium pool may have a regulatory role in stimulus-response coupling.


1993 ◽  
Vol 25 (4) ◽  
pp. 276-285 ◽  
Author(s):  
A. Bonhomme ◽  
L. Pingret ◽  
P. Bonhomme ◽  
J. Michel ◽  
G. Balossier ◽  
...  

1977 ◽  
Vol 57 (1) ◽  
pp. 21-30 ◽  
Author(s):  
J. T. MILLS ◽  
J. CHONG

Gross morphology, ultrastructure and distribution of minerals in sound and severely heat-damaged, elevator-stored rapeseeds (Brassica napus L.) were studied by electron microscopy and X-ray microanalysis. Sound seeds had surface reticulations and a thick seed coat of five layers: epidermis, palisade, crushed parenchyma, aleurone and inner crushed parenchyma. The aleurone cells in the seed coat and the embryonic cells contained many lipid droplets and protein bodies among the cytoplasmic organelles. Severely heat-damaged seeds had a more compressed, electron-dense seed coat with much surface debris which obscured the reticulations; embryonic tissues appeared distorted and shrunken. Aleurone cells in the seed coat and most embryonic cells were necrotic and had large structureless areas and abnormal protein bodies. In the coat of sound seeds, calcium, potassium, sulphur, silicon, magnesium and phosphorus were found in decreasing order of proportional amounts. In cotyledonous tissue the sequence was phosphorus, potassium, sulphur, magnesium and silicon with phosphorus in highest relative proportion. In severely heat-damaged seeds, cotyledonous protein bodies had lower proportions of phosphorus and sulphur, while the seed coat had a higher proportion of phosphorus and lower calcium when compared to sound seeds.


2013 ◽  
Vol 76 (4) ◽  
pp. 627-633 ◽  
Author(s):  
Tracy Punshon ◽  
Ryan Tappero ◽  
Felipe K. Ricachenevsky ◽  
Kendal Hirschi ◽  
Paul A. Nakata
Keyword(s):  
X Ray ◽  

1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.


1994 ◽  
Vol 144 ◽  
pp. 1-9
Author(s):  
A. H. Gabriel

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.


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.


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