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多显微镜技术(LM 和 SEM)在巴基斯坦分布的 Asteraceae 成员比较孢粉学研究中的应用。

Application of multimicroscopic techniques (LM and SEM) in comparative palynological study of Asteroideae members, inhabited in Pakistan.

机构信息

Department of Botany, Lahore College for Women University, Lahore, Pakistan.

Department of Botany, Faculty of Life Sciences, University of Okara, Pakistan.

出版信息

Microsc Res Tech. 2021 May;84(5):1063-1077. doi: 10.1002/jemt.23667. Epub 2020 Dec 17.

DOI:10.1002/jemt.23667
PMID:33332675
Abstract

In the present study light and scanning electron microscopic approaches were used to study the palynological variations among 30 Asteroideae members. Variety of qualitative and quantitative palynological characters like pollen shape and type, pollen sculpturing, pollen size, P/E ratio, exine and intine thickness, interspecific difference, colpi size, pore size, spines length, spine width, and pollen fertility were observed. Results reported remarkable variations among pollen characters of studied taxa. The shape of pollen grains in polar and equatorial views varied from specie to specie such as spheroidal, prolate, oblate, subspheroidal, oblate spheroidal, prolate spheroidal, suboblate, and sub prolate. Bidens pilosa L. showed maximum pollen size in both polar and equatorial views, whereas minimum pollen size in polar view was found in Tetraneuris scaposa (DC.) Greene. (i.e., 30.5 μm) and in equatorial view was found in Cosmos sulphureus Cav. (25.5 μm).The highest P/E ratio (1.39 μm) was measured in Glebionis coronaria L. The values of exine and intine thickness also varied. Tricolporate, tetracolporate, trizonocolporate, pentoporate, and polypentoporate pollen types were examined. Spinateand echinate pollen sculpturingobserved under SEM. Variations in spine length and width also recorded. The maximum pollen fertility (98%) was measured in Chrysanthemum morifolium Ramat. and the lowest (56%) was recorded in Thymophylla tenuiloba (DC.) Small. It was concluded that the variations in qualitative and quantitative characters were seemed to be valuable for the taxonomic investigations of Asteroideae taxa.

摘要

在本研究中,使用光学和扫描电子显微镜方法研究了 30 种 Asteroidae 成员之间的花粉学变化。观察了各种定性和定量花粉学特征,如花粉形状和类型、花粉纹饰、花粉大小、P/E 比、外壁和内壁厚度、种间差异、沟的大小、孔大小、刺的长度、刺的宽度和花粉活力。研究报告表明,研究类群的花粉特征存在显著差异。花粉粒在极面和赤道面的形状从一个种到另一个种变化,如球形、长球形、扁球形、近球形、扁球形、长球形、近扁球形和近长球形。在极面和赤道面,Bidens pilosa L. 的花粉粒最大,而 Tetraneuris scaposa (DC.) Greene. 的花粉粒最小(即 30.5 μm),Cosmos sulphureus Cav. 的花粉粒最小(25.5 μm)。在 Glebionis coronaria L. 中测量到最高的 P/E 比(1.39 μm)。外壁和内壁厚度的值也有所不同。检查了三孔、四孔、三沟孔、五孔和多孔花粉类型。使用 SEM 观察了具刺和具刺花粉纹饰。还记录了刺的长度和宽度的变化。Chrysanthemum morifolium Ramat. 的花粉活力最高(98%),Thymophylla tenuiloba (DC.) Small. 的花粉活力最低(56%)。研究结论认为,定性和定量特征的变化似乎对 Asteroidae 类群的分类研究具有重要价值。

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