Mechanical structure of JNLT     

N. Itoh  I. Mikami  Y. Yamashita  T. Noguchi 《Astrophysics and Space Science》1989,160(1-2):165-172

The Japanese National Large Telescope (JNLT) requires mechanical performance of high tracking accuracy to achieve good image quality and a mechanical configuration to provide several kinds of focus modes. Under these requirements, a conceptual design for the JNLT mechanical structure has been performed. This paper presents the results of the conceptual design currently under consideration.Paper presented at the symposium on the JNLT and Related Engineering Developments, Tokyo, November 29–December 2, 1988.  相似文献   

Land suitability analysis for maize production in Indonesia using satellite remote sensing and GIS-based multicriteria decision support system     

Habibie  Muhammad Iqbal  Noguchi  Ryozo  Shusuke  Matsushita  Ahamed  Tofael 《GeoJournal》2021,86(2):777-807

GeoJournal - Maize is one of the potential crops can help in regional food production with self-sufficiency of foods in the drought prone areas of East Java in Indonesia. The purpose of this...  相似文献   

Transition metals in the transition zone: partitioning of Ni,Co, and Zn between olivine,wadsleyite, ringwoodite,and clinoenstatite     

Li?ZhangEmail author  Joseph?R.?Smyth  Takaaki?Kawazoe  Steven?D.?Jacobsen  Shan?Qin 《Contributions to Mineralogy and Petrology》2018,173(7):52

Ni, Co, and Zn are widely distributed in the Earth’s mantle as significant minor elements that may offer insights into the chemistry of melting in the mantle. To better understand the distribution of Ni²⁺, Co²⁺, and Zn²⁺ in the most abundant silicate phases in the transition zone and the upper mantle, we have analyzed the crystal chemistry of wadsleyite (Mg₂SiO₄), ringwoodite (Mg₂SiO₄), forsterite (Mg₂SiO₄), and clinoenstatite (Mg₂Si₂O₆) synthesized at 12–20 GPa and 1200–1400 °C with 1.5–3 wt% of either NiO, CoO, or ZnO in starting materials. Single-crystal X-ray diffraction analyses demonstrate that significant amounts of Ni, Co, and Zn are incorporated in octahedral sites in wadsleyite (up to 7.1 at%), ringwoodite (up to 11.3 at%), olivine (up to 2.0 at%), and clinoenstatite (up to 3.2 at%). Crystal structure refinements indicate that crystal field stabilization energy (CFSE) controls both cation ordering and transition metal partitioning in coexisting minerals. According to electron microprobe analyses, Ni and Co partition preferentially into forsterite and wadsleyite relative to coexisting clinoenstatite. Ni strongly prefers ringwoodite over coexisting wadsleyite with \({D}_{\text{Ni}}^{\text{Rw}/\text{Wd}}\)?=?4.13. Due to decreasing metal–oxygen distances with rising pressure, crystal field effect on distribution of divalent metal ions in magnesium silicates is more critical in the transition zone relative to the upper mantle. Analyses of Ni partitioning between the major upper-mantle phases implies that Ni-rich olivine in ultramafic rocks can be indicative of near-primary magmas.  相似文献   

Correction to: Transition metals in the transition zone: partitioning of Ni,Co, and Zn between olivine,wadsleyite, ringwoodite,and clinoenstatite     

Li?ZhangEmail author  Joseph?R.?Smyth  Takaaki?Kawazoe  Steven?D.?Jacobsen  Shan?Qin 《Contributions to Mineralogy and Petrology》2018,173(7):60

  相似文献   

Mass dispersal and angular momentum transfer during collisions between rubble-pile asteroids     

Takaaki Takeda  Keiji Ohtsuki 《Icarus》2007,189(1):256-273

We perform N-body simulations of impacts between initially non-rotating rubble-pile asteroids, and investigate mass dispersal and angular momentum transfer during such collisions. We find that the fraction of the dispersed mass (Mdisp) is approximately proportional to , where Qimp is the impact kinetic energy; the power index α is about unity when the impactor is much smaller than the target, and 0.5?α<1 for impacts with a larger impactor. Mdisp is found to be smaller for more dissipative impacts with small values of the restitution coefficient of the constituent particles. We also find that the efficiency of transfer of orbital angular momentum to the rotation of the largest remnant depends on the degree of disruption. In the case of disruptive oblique impacts where the mass of the largest remnant is about half of the target mass, most of the orbital angular momentum is carried away by the escaping fragments and the efficiency becomes very low (<0.05), while the largest remnant acquires a significant amount of spin angular momentum in moderately disruptive impacts. These results suggest that collisions likely played an important role in rotational evolution of small asteroids, in addition to the recoil force of thermal re-radiation.  相似文献