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| 1 | New host and locality records of snake intestinal nematode Kalicephalus spp in Indonesia显示文摘Objective:To observe three species of Kalicephalus found in three species of snake(Ophkphagus hannah,Ptyas mucosus,and Naja Sputatrix) during research on Capture Snake for Trading in Java and Snake Biodiversity in Kalimantan Islands.Methods:Specimens for light microscopy examination were fixed with warm 70%alcohol,cleared and mounted in lactophenol for wet mounting.Drawings were made with the aid of a drawing tube attached to a Nikon compound microscope.Measurements were given in micrometers(μ) as the average of findings,followed by the range in parentheses,unless otherwise stated.Results:Kalkephalus(Costatus) indicus was found from 7 Ptyas mucosus,Kalicephalus bungari from 2 Naja sputatrix and 1 Kalicephalus(Costatus) indicus and Kalicephalus assimilis found from 1 Ophiophagus hannah.The morphology and measurement of three species of Kalicephalus found in this study were close to those described before.Conclusions:New finding of host of Kalicephalus(Costalus) indicus and Kalicephalus bungari was a snake species of Naja sputatrix.New records of locality were Kalimantan island as the new locality of Kalicephalus assimilis,and Java island was new locality of Kalicephalus(Costatus) indicus. | Endang Purwaningsih Mumpuni | 2011 | Asian Pacific Journal of Tropical Biomedicine2011，1，2： | 3 |
| 2 | Effect of Metabolites Produced by Trichoderma harzianum Biotypesand Agaricus bisporus on Their RespectiveGrowth Radii in Culture 显示文摘 | MUMPUNI A SHARMA H S AVERIL E B | 1998 | Applied and Environmental Microbiology1998，，： | 1 |
| 3 | Multi-wavelength fibril dynamics and oscillations above sunspot– I. morphological signature显示文摘In this work we selected one particular fibril from a high resolution observation of the solar chromosphere with the Dutch Open Telescope, and tried to obtain a broad picture of the intricate mechanism that might be operating in the multiple layers of the solar atmosphere visible in high cadence multi-wavelength observations. We analyzed the changing fibril pattern using multi-wavelength tomography, which consists of both the Hα line center and the blue wing, Doppler signal, Ca II H, and the G-band. We have found that the intermittent ejected material through the fibril from Doppler images has clearly shown an oscillation mode, as seen in the Hα blue wing.The oscillations in the umbrae and penumbrae magnetic field lines that are above the sunspot cause a broadening and the area forms a ring shape from 3 to 15 minute oscillations as a function of height. These made a distinct boundary between the umbrae and penumbrae which suggests a comb structure, and indicates that the oscillations could propagate along the inclined magnetic flux tubes from below. The 3 minute oscillations strongly appeared in the broadly inclined penumbrae magnetic field lines and showed a clear light bridge. The well known 5 minute oscillations were dominant in the umbrae-penumbrae region boundary. The long 7 minute oscillations were transparent in the Hα blue wing, as well as the 10 and 15 minute oscillations. They were concentrated in the inner-penumbrae, as seen in the Hα line center. From these findings we propose that the fibril acts as a fabric for interaction between the layers,as well as related activities around the active region under investigation. | Emanuel Sungging Mumpuni Dhani Herdiwijaya Mitra Djamal Thomas Djamaluddin | 2015 | Research in Astronomy and Astrophysics2015，15，11： | 0 |
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