Zobrazeno 1 - 9
of 9
pro vyhledávání: '"赤外線スペクトル"'
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :100-103
The ASTER (Advanced Spaceborne Thermal Emission and Reflection Radiometer) VNIR (Visible and Near Infrared) and SWIR (Short Wave Infrared) lunar imageries were used to derive the bidirectional reflectance of the lunar surface and used for mineralogic
In-situ heating decrease kinetics of aliphatic hydrocarbons in carbonaceous chondrites by micro-FTIR
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :116-119
資料番号: AA0063350030
Publikováno v:
第36回月・惑星シンポジウム = Proceedings of the 36th ISAS Lunar and Planetary Symposium. :262-265
Experimental studies of coalescence between MgO grains and SiO2 grains in smoke reveal the direct production of crystalline forsterite grains and amorphous Mg-bearing silicate owing to the difference of cooling velocity after the formation of Mg2SiO4
Publikováno v:
第36回月・惑星シンポジウム = Proceedings of the 36th ISAS Lunar and Planetary Symposium. :242-245
The spectra of carbonates were measured in mid- and far-infrared region. These spectra show very strong and broad peaks in the far infrared region. The calcite and dolomite have peaks at about 92, and about 63 micrometer, respectively. The unidentifi
Publikováno v:
スペース・プラズマ研究会 平成16年度 = Space Plasma Conference FY2004. :43-45
資料番号: AA0063347012
Publikováno v:
第28回月・惑星シンポジウム = Proceedings of the 28th ISAS Lunar and Planetary Symposium. :182-185
Infrared spectra of various alumina particles produced by the oxidation of aluminum particles were measured. Infrared spectrum of alumina particles produced by the treatment below 600 C showed an absorption peak at 10.8 micrometer, and identified as
Publikováno v:
第28回月・惑星シンポジウム = Proceedings of the 28th ISAS Lunar and Planetary Symposium. :186-189
The infrared absorption spectra of CO and CO2 in amorphous water ice have been measured at 10 K over a wide concentration range of CO and CO2. It is found that that the calibration curves (concentration dependence of ratio of integrated absorbance, I
Autor:
Keller, L. P., Zolensky, M. E., Suzuki, Akiko, Kebukawa, Yoko, Nakashima, Satoru, Nakamura, Tomoki
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :120-121
資料番号: AA0063350031
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :123-123
We model cometary dust by taking into account its formation and evolution. Light scattering, absorption, and emission properties of the dust expected from our model are compared with observations. We assume unprocessed cometary dust as primordial int