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| 1 | Microstructure of Y203 Doped Al2OgZrO2 Eutectic Fibers Grown by the Micro-pulling-down Method 显示文摘 | Lee J H Yoshikawa A Kaiden H | 2001 | Journal of Crystal Growth2001，231，： | 1 |
| 2 | Microstructure of Y2O3Doped Al2O3/Zr O2Eutectic Fibers Grown by the Micro-Pulling-Down Method显示文摘 | Lee J H Yoshikawa A Kaiden H | 2001 | Journal of Crystal Growth2001，231，12： | 1 |
| 3 | Microstructure of Y2O3 doped Al2O3/ZrO2 euteetic fibers grown by the micro-pulling-down method 显示文摘 | LEE J H YOSHIKAWA A KAIDEN H | 2001 | Journal of Crystal Growth2001，231，： | 1 |
| 4 | Septum Polar- izer for Ka-band H-shaped Rotary Joint显示文摘 | KAIDEN M KiMURA K OGAWA H | 2009 | Journal of In- frared Millimeter and Terahertz Waves2009，30，7： | 1 |
| 5 | A study of the amide Ⅲ band by FT-IR spectrometry of the secondary structure of albu- min, myoglo-bin, and g-globulin显示文摘 | KAIDEN K MATSUI T TANAKA S | 1987 | Appl Spectrosc1987，41，： | 1 |
| 6 | Septum Polarizer for Ka-Band H-Shaped Rotary Joint显示文摘 | KAIDEN Masahiro KIMURA Kimihiro OGAWA Hideo | 2009 | Journal of Infrared Millimeter and Terahertz Waves2009，30，7： | 1 |
| 7 | Meteorite search by JARE-39in 1998-99 season显示文摘 | Kojima H Kaiden H Yada T | 2000 | Antarctic Meteorite Research2000，13，： | 1 |
| 8 | Microstrueture of Y2O3 doped Al2O3/ZrO2 eutectic fibers grown by the micro-pullingdown method显示文摘 | LEE J H YOSHIKAWA A KAIDEN H | 2001 | Journal of Crystal Growth2001，231，： | 1 |
| 9 | A study of the amide III band by FTIR spectrometry of albumin, myoglobin, and c-globulin 显示文摘 | Kaiden K Matsui T Tanaka S | 1987 | Applied spectroscopy1987，4，2： | 1 |
| 10 | Microstructure of Y2O3 doped ZrO2/Al2O3 eutectic fibers grown by the micropulling-down method 显示文摘 | Lee J H Yoshikawa A Kaiden H | 2001 | J Cryst Growth2001，231，： | 1 |
| 11 | A study of the amide II and by FTIR spectrometry of the secondary structure of albumin, myoglobin and globulin显示文摘 | Kaiden K | 1987 | Appl Spectroscopy1987，41，2： | 1 |
| 12 | Microstructure of Y 2 O 3 doped Al 2 O 3 /ZrO 2 eutectic fibers grown by the micro-pulling-down method显示文摘 | J.H. Lee A. Yoshikawa H. Kaiden K. Lebbou T. Fukuda D.H. Yoon Y. Waku | 2001 | Journal of Crystal Growth2001，，： | 1 |
| 13 | Microstructure of Y203 Doped A1203/ZrO2 Eutectic Fibers Grown by the Micro-pulling-down Method 显示文摘 | Lee J H Yoshikawa A Kaiden H | 2001 | Journal of Crystal Growth2001，231，： | 1 |
| 14 | Stenian A-type granitoids in the Namaqua-Natal Belt,southern Africa,Maud Belt,Antarctica and Nampula Terrane,Mozambique:Rodinia and Gondwana amalgamation implications显示文摘We carried out SHRIMP zircon U-Pb dating on A-type granitic intrusions from the Namaqua-Natal Province,South Africa,Sverdrupfjella,western Dronning Maud Land,Antarctica and the Nampula Province of northern Mozambique.Zircon grains in these granitic rocks are typically elongated and oscillatory zoned,suggesting magmatic origins.Zircons from the granitoid intrusions analyzed in this study suggest^1025-1100 Ma ages,which confirm widespread Mesoproterozoic A-type granitic magmatism in the Namaqua-Natal(South Africa),Maud(Antarctica)and Mozambique metamorphic terrains.No older inherited(e.g.,~2500 Ma Achean basement or^1200 Ma island are magmatism in northern Natal)zircon grains were seen.Four plutons from the Natal Belt(Mvoti Pluton,Glendale Pluton,Kwalembe Pluton,Ntimbankulu Pluton)display 1050-1040 Ma ages,whereas the Nthlimbitwa Pluton in northern Natal indicates older 1090-1080 Ma ages.A sample from Sverdrupfjella,Antarctica has^1091 Ma old zircons along with^530 Ma metamorphic rims.Similarly,four samples analysed from the Nampula Province of Mozambique suggest crystallization ages of^1060-1090 Ma but also show significant discordance with two samples showing younger^550 Ma overgrowths.None of the Natal samples show any younger overgrowths.A single sample from southwestern Namaqualand yielded an age of^1033 Ma.Currently available chronological data suggest magmatism took place in the Namaqua-Natal-MaudMozambique(NNMM)belt between^1025 Ma and^1100 Ma with two broad phases between^1060-1020 Ma and 1100-1070 Ma respectively,with peaks at between^1030-1040 Ma and^1070-1090 Ma.The age data from the granitic intrusions from Namaqualand.combined with those from Natal,Antarctica and Mozambique suggest a crude spatial-age relationship with the older>1070 Ma ages being largely restricted close to the eastern and western margins of the Kalahari Craton in northern Natal,Mozambique.Namaqualand and WDML Antarctica whereas the younger<1060 Ma ages dominate in southern Natal and western Namaqualand and are largely restricted to the southern and possibly the western margins of the Kalahari Craton.The older ages of magmatism partially overlap with or are marginally younger than the intracratonic Mkondo Large lgneous Provinee intruded into or extruded onto the Kalahari Craton,suggesting a tectonic relationship with the Maud Belt.Similar ages from granitic augen gneisses in Sri Lanka suggest a continuous belt stretching from Namaqualand to Sri Lanka in a reconstituted Gondwana,formed during the terminal stages of amalgamation of Rodinia and predating the East African Orogen.This contiguity contributes to defining the extent of Rodinia-age crustal blocks,subsequently fragmented by the dispersal of Rodinia and Gondwana. | Tomokazu Hokada Geoffrey H.Grantham Makoto Arima Satoshi Saito Kazuyuki Shiraishi Richard A.Armstrong Bruce Eglington Keiji Misawa Hiroshi Kaiden | 2019 | Geoscience Frontiers2019，10，6： | 1 |
| 15 | A study of the amide Ⅲ by FT-IR spectrometry of the secondary structure of albumin,myoglobin,and γ-globulin显示文摘 | KAIDEN K MATSUI T TANAKA S | 1987 | Appl Spectrosc1987，41，2： | 1 |
| 16 | Microstructure of Y2O3 doped Al2O3/ZrO2 eutectic fibers grown by the micro-pulling-down method显示文摘 | LEE H J YOSHIKAWA A KAIDEN H | 2001 | J Crystal Growth2001，231，12： | 1 |
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