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首页> 外文期刊>Geophysical Research Letters >Far-ultraviolet observations of the neutral comae of Comet Hale-Bopp (C/1995 01) near perihelion
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Far-ultraviolet observations of the neutral comae of Comet Hale-Bopp (C/1995 01) near perihelion

机译:对近日点附近的黑尔-波普彗星(C / 1995 01)的中性彗星的远紫外线观测

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The Ultraviolet Imager on the Polar spacecraft observed the neutral oxygen and carbon comae of Comet Hale-Bopp (C/1995 01) at far-ultraviolet wavelengths near perihelion on March 31 and April 2, 1997. The OI (1304) coma was circularly symmetric with a diameter of about 5 million km. The coma was smaller in the longer wavelength (1400-1600 Angstrom and 1600-1800 Angstrom) bands, which is probably due to fluorescence of neutral carbon at 1561 Angstrom and 1657 Angstrom. The production rate for O calculated from the observed OI (1304) flux was (9.8 +/- 2.5) x 10(30). Using this value the estimated production rate for OH was (8.9 +/-2.5) x 10(30) and for H2O was (1.0 +/- 0.3) x 10(31). [References: 19]
机译:极地飞船上的紫外线成像仪于1997年3月31日至4月2日在近日点附近的远紫外线波长观察到了黑尔-波普彗星(C / 1995 01)的中性氧和碳彗星。OI(1304)彗星是圆对称的直径约500万公里在更长的波长(1400-1600埃和1600-1800埃)波段中,昏迷较小,这可能是由于中性碳在1561埃和1657埃处发出的荧光所致。由观察到的OI(1304)焊剂计算出的O生产率为(9.8 +/- 2.5)x 10(30)。使用该值,OH的估计生产率为(8.9 +/- 2.5)x 10(30),H2O的估计生产率为(1.0 +/- 0.3)x 10(31)。 [参考:19]

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