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Kudo, H.,Cheng, K.J.,Rode, L.M.,Abdullah, N.,Ho, Y.W.,Hussain, H.Y.,Jalaludin, S. Asian Australasian Association of Animal Productio 1994 Animal Bioscience Vol.7 No.3
Effects of chemical treatments on in sacco and in vitro digestibility of barley straw by rumen fluid and pure cultures of cellulolytic bacteria were studied to evaluate the pretreatment and to improve the poor quality feed. Chemicals were applied by dissolving them in water equivalent to 40% of the weight of the straw (dry matter basis). Pretreatment with 5% NaOH yielded the largest increase in sacco digestion followed by pretreatment with 2% $(NH_4)_2SO_3$, 2.6% $NH_4OH$, 1.6% $NaHSO_3$ and untreated straw (control). In sacco dry matter digestibility of straw treated with NaOH and $(NH_4)_2SO_3$ continued to increase as the concentration of chemical increased (1 to 7.5%), as it was the in vitro dry matter loss by leaching. Treatment of barley straw with 5% NaOH enhanced significantly (p < 0.01) in vitro digestibility by rumen fluid, Fibrobacter suceinogenes and Ruminococcus albus though the fermentation products by cellulolytic bacteria were low, whereas the treatment with 5% $(NH_4)_2SO_3$ inhibited in vitro digestibility by F. succinogenes and R. albus together with lower fermentation products. Dry matter loss by leaching and bacterial digestion from barley straw treated with NaOH and $(NH_4)_2SO_3$ suggested the effect of pretreatment with these chemicals were based on leaching, and the cellulolytic bacteria had little to do with digestion.
Dark-chilling Pretreatment Protects PSI from Light-chilling Damage
Kudoh, Hideki,Sonoike, Kintake Korean Society of Photoscience 2002 Journal of Photosciences Vol.9 No.2
In chilling-sensitive plants, the donor side of Photosystem II is inhibited by the chilling treatment in the dark, while the acceptor side of Photosystem I is inhibited by the chilling under the moderate light. Since the addition of inhibitors of electron transfer from Photosystem II protects Photosystem I from chilling induced photoinhibition of Photosystem I, inhibition or down-regulation of Photosystem II activity in vivo may also protect Photosystem I from photoinhibition. It was revealed that dark-chilling pretreatment actually protected Photosystem I from photoinhibition. The results imply that down-regulation of Photosystem II under stress conditions may have a role to protect Photosystem I from photoinhibition.
Sato, Yasuhiro,Kudoh, Hiroshi The Ecological Society of Korea 2013 Journal of Ecology and Environment Vol.36 No.3
We estimated phenotypic selection on the height and number of flowering-stalks in a rosette annual Cardamine hirsuta by applying path analysis to the data collected at three natural populations located in central Japan. The path from rosette size was positively connected with the fruit production through the both height and number of flowering-stalks. In the all three populations, the paths from the number of stalks were more strongly connected with the fruit production than from the height of stalks. The paths from the rosette size showed similar magnitude with the number of stalks and the height of stalks. The direct path from rosette size to the fruit production was detected only at one site. These results suggest stronger phenotypic selection on the rosette size through the number of stalks than the height of stalks. The lateral branching rather than increment of individual inflorescence size is the major response to control the fruit production for C. hirsuta growing in a natural habitat.
Nakagawa, Takayuki,Kudoh, Keiko,Fukuda, Naoyuki,Kasugai, Shohei,Tachikawa, Noriko,Koyano, Kiyoshi,Matsushita, Yasuyuki,Sasaki, Masanori,Ishikawa, Kunio,Miyamoto, Youji Korean Academy of Periodontology 2019 Journal of Periodontal & Implant Science Vol.49 No.6
Purpose: The purpose of this study was to elucidate the efficacy and safety of carbonate apatite (CO<sub>3</sub>Ap) granules in 2-stage sinus floor augmentation through the radiographic and histomorphometric assessment of bone biopsy specimens. Methods: Two-stage sinus floor augmentation was performed on 13 patients with a total of 17 implants. Radiographic assessment using panoramic radiographs was performed immediately after augmentation and was also performed 2 additional times, at 7±2 months and 18±2 months post-augmentation, respectively. Bone biopsy specimens taken from planned implant placement sites underwent micro-computed tomography, after which histological sections were prepared. Results: Postoperative healing of the sinus floor augmentation was uneventful in all cases. The mean preoperative residual bone height was 3.5±1.3 mm, and this was increased to 13.3±1.7 mm by augmentation with the CO<sub>3</sub>Ap granules. The mean height of the augmented site had decreased to 10.7±1.9 mm by 7±2 months after augmentation; however, implants with lengths in the range of 6.5 to 11.5 mm could still be placed. The mean height of the augmented site had decreased to 9.6±1.4 mm by 18±2 months post-augmentation. No implant failure or complications were observed. Few inflammatory cells or foreign body giant cells were observed in the bone biopsy specimens. Although there were individual differences in the amount of new bone detected, new bone was observed to be in direct contact with the CO<sub>3</sub>Ap granules in all cases, without an intermediate layer of fibrous tissue. The amounts of bone and residual CO<sub>3</sub>Ap were 33.8%±15.1% and 15.3%±11.9%, respectively. Conclusions: In this first demonstration, low-crystalline CO<sub>3</sub>Ap granules showed excellent biocompatibility, and bone biopsy showed them to be replaced with bone in humans. CO<sub>3</sub>Ap granules are a useful and safe bone substitute for two-stage sinus floor augmentation.
Peritectic Transformation during Cooling of Iron-Carbon Alloy
Matsuura, Kiyotaka,Kudoh, Masayuki 대한금속재료학회(대한금속학회) 1998 METALS AND MATERIALS International Vol.4 No.3
Peritectic transformation behavior during cooling of iron-carbon alloys is simulated by a numerical analysis. The peritectic transformation, δ+L=γ, is divided into δ-γ transformation at δ/γ interface and L-γ solidification at γ/L interface, and proceeds by the following two mechanisms: (1) carbon diffusion from liquid (referred to as L) through austenite (γ) into b-ferrite (δ) and (2) precipitation of austenite from b-ferrite and crystallization of it from liquid due to cooling. Approximately 80% of the austenite formed during the peritectic transformation is the products of δ-γ transformation, which may cause the generation of tensile stress in the solidification shell of cast steels due to the difference in density between δ-ferrite and austenite The amount of the δ-γ transformation is largest, when the initial carbon content is 0.17 mass%. However, when the transformation in a well-developed dendrite network structure is focused on, the carbon content for the maximum amount of the δ-γ transformation decreases to 0.14-0.16 mass%, which corresponds to the carbon content at which surface cracking of continuously cast slabs is reported to be most frequent
Yasuhiro Sato,Hiroshi Kudoh 한국생태학회 2013 Journal of Ecology and Environment Vol.36 No.3
We estimated phenotypic selection on the height and number of flowering-stalks in a rosette annual Cardamine hirsuta by applying path analysis to the data collected at three natural populations located in central Japan. The path from rosette size was positively connected with the fruit production through the both height and number of flowering-stalks. In the all three populations, the paths from the number of stalks were more strongly connected with the fruit production than from the height of stalks. The paths from the rosette size showed similar magnitude with the number of stalks and the height of stalks. The direct path from rosette size to the fruit production was detected only at one site. These results suggest stronger phenotypic selection on the rosette size through the number of stalks than the height of stalks. The lateral branching rather than increment of individual inflorescence size is the major response to control the fruit production for C. hirsuta growing in a natural habitat.
TANUMA SYUNITI,YOKOYAMA TAKAAKI,KUDOH TAKAHIRO,SHIBATA KAZUNARI The Korean Astronomical Society 2001 Journal of The Korean Astronomical Society Vol.34 No.4
Strong thermal X-ray emission, called Galactic Ridge X-ray Emission, is observed along the Galactic plane (Koyama et al. 1986). The origin of hot ($\~$7 keV) component of GRXE is not known, while cool ($\~$0.8 keV) one is associated with supernovae (Kaneda et al. 1997, Sugizaki et al. 2001). We propose a possible mechanism to explain the origin; locally strong magnetic fields of $B_{local}\;\~30{\mu}G$ heat interstellar gas to $\~$7 keV via magnetic reconnection (Tanuma et al. 1999). There will be the small-scale (< 10 pc) strong magnetic fields, which can be observed as $(B)_{obs} \;\~3{\mu}G$ by integration of Faraday Rotation Measure, if it is localized by a volume filling factor of f $\~$ 0.1. In order to examine this model, we solved three-dimensional (3D) resistive magnetohydrodynamic (MHD) equations numerically to examine the magnetic reconnect ion triggered by a supernova shock (fig.l). We assume that the magnetic field is Bx = 30tanh(y/20pc) $\mu$G, By = Bz = 0, and the temperature is uniform, at the initial condition. We put a supernova explosion outside the current sheet. The supernova-shock, as a result, triggers the magnetic reconnect ion, and the gas is heatd to > 7 keV. The magnetic reconnect ion heats the interstellar gas to $\~$7 keV in the Galactic plane, if it occurs in the locally strong magnetic fields of $B_{local}\;\~30{\mu}G$. The heated plasma is confined by the magnetic field for $\~10^{5.5} yr$. The required interval of the magnetic reconnect ions (triggered by anything) is $\~$1 - 10 yr. The magnetic reconnect ion will explain the origin of X-rays from the Galactic ridge, furthermore the Galactic halo, and clusters of galaxies.