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The Alpha Magnetic Spectrometer (AMS) on the International Space Station: Part I - results from the test flight on the space shuttle [Review]

机译:国际空间站上的Alpha电磁光谱仪(AMS):第一部分-航天飞机上的试飞结果[查看]

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The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7degrees orbit at altitudes between 320 and 390 km. A search for antihelium nuclei in the rigidity range 1-140 GV was performed. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1 x 10(-6) was obtained. The high energy proton, electron, positron, helium, antiproton and deuterium spectra were accurately measured. For each particle and nuclei two distinct spectra were observed: a higher energy spectrum and a substantial second spectrum. Positrons in the second spectrum were found to be much more abundant than electrons. Tracing particles from the second spectra shows that most of them travel for an extended period of time in the geomagnetic field, and that the positive particles (p and e(+)) and negative ones (e(-)) originate from two complementary geographic regions. The second helium spectrum flux over the energy range 0.1-1.2 GeVucleon was measured to be (6.3 +/- 0.9) x 10(-3)(m(2) s sr)(-1). Over 90 percent of the helium flux was determined to be He-3 at the 90% confidence level. (C) 2002 Elsevier Science B.V. All rights reserved. [References: 179]
机译:Alpha电磁光谱仪(AMS)在STS-91航班(1998年6月)中以51.7度的轨道在320至390 km的高度飞行时,被搭载在发现号航天飞机上。在刚度范围1-140 GV中搜索抗氦核。在任何刚性下均未检测到抗氦核。获得的抗氦气与氦气通量比的上限为<1.1 x 10(-6)。准确测量了高能质子,电子,正电子,氦气,反质子和氘光谱。对于每个粒子和原子核,观察到两个不同的光谱:较高的能量光谱和大量的第二光谱。发现第二光谱中的正电子比电子丰富得多。从第二个光谱中追踪到的粒子表明,它们中的大多数在地磁场中传播了一段较长的时间,而正粒子(p和e(+))和负粒子(e(-))源自两个互补的地理区域。地区。在能量范围0.1-1.2 GeV /核子中的第二氦光谱通量测得为(6.3 +/- 0.9)x 10(-3)(m(2)s sr)(-1)。在90%的置信水平下,超过90%的氦通量被确定为He-3。 (C)2002 Elsevier Science B.V.保留所有权利。 [参考:179]

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