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DOI | 10.1126/science.275.5296.49 |
Generation of x-rays from comet C/Hyakutake 1996 B2 | |
Bingham R.; Dawson J.M.; Shapiro V.D.; Mendis D.A.; Kellett B.J. | |
发表日期 | 1997 |
ISSN | 0036-8075 |
起始页码 | 49 |
结束页码 | 50 |
卷号 | 275期号:5296 |
英文摘要 | The instability resulting from the relative motion of newly picked-up cometary photoions and the solar wind generates lower hybrid waves that are capable of accelerating electrons to the keV range of energies. These electrons may be responsible for the x-rays from comet C/Hyakutake 1996 B2 seen by the Rontgen X-ray Satellite. The inferred x-ray photon power depends on the electron energy, with keV electrons providing values of photon power two orders of magnitude greater than 100 eV electrons. These observations and in particular, spectral resolution of the x-rays, should provide more insight into the composition of the comet. |
英文关键词 | article; astronomy; electron; energy; photon; priority journal; X ray |
语种 | 英语 |
来源期刊 | Science |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/243048 |
作者单位 | Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX11 0QX, United Kingdom; Department of Physics, University of California, Los Angeles, CA 90024, United States; Department of Physics, Univ. of California at San Diego, San Diego, CA 92092, United States; Dept. of Elec. and Computing Science, Univ. of California at San Diego, San Diego, CA 92092, United States |
推荐引用方式 GB/T 7714 | Bingham R.,Dawson J.M.,Shapiro V.D.,et al. Generation of x-rays from comet C/Hyakutake 1996 B2[J],1997,275(5296). |
APA | Bingham R.,Dawson J.M.,Shapiro V.D.,Mendis D.A.,&Kellett B.J..(1997).Generation of x-rays from comet C/Hyakutake 1996 B2.Science,275(5296). |
MLA | Bingham R.,et al."Generation of x-rays from comet C/Hyakutake 1996 B2".Science 275.5296(1997). |
条目包含的文件 | 条目无相关文件。 |
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