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紫金山天文台 [4]
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期刊论文 [4]
发表日期
2010 [2]
2008 [2]
学科主题
Physics [4]
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学科主题:Physics
专题:紫金山天文台
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An alternative evolution scenario for OAO 1657-415 and IGR J18483-0311
期刊论文
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 卷号: 53, 期号: 1, 页码: 130-134
作者:
Liu QingZhong
;
Li Hui
;
Yan JingZhi
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浏览/下载:21/0
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提交时间:2011/11/23
high-mass X-ray binary
pulsar
Corbet's diagram
stellar evolution
Optical results of the black hole microquasar SS 433
期刊论文
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 卷号: 53, 期号: 1, 页码: 153-156
作者:
Li Hui
;
Yan JingZhi
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浏览/下载:12/0
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提交时间:2011/11/23
high-mass X-ray binary
black hole
spectroscopy
outflow wind
relativistic jet
Solitary kinetic Alfven waves in dusty plasmas
期刊论文
PHYSICS OF PLASMAS, 2008, 卷号: 15, 期号: 8, 页码: 083703
作者:
Li, Yang-fang
;
Wu, D. J.
;
Morfill, G. E.
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浏览/下载:22/0
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提交时间:2011/12/29
Solitary kinetic Alfven waves in dusty plasmas are studied by Considering the dust charge variation. The effect of the dust charge-to-mass ratio on the soliton solution is discussed. The Sagdeev potential is derived analytically with constant dust charge and then calculated numerically by taking the dust charge variation into account. We show that the dust charge-to-mass ratio plays an important role in the soliton properties. The soliton solutions are comprised of two branches. One branch is sub-Alfvenic and the soliton velocity is obviously smaller than the Alfven speed. The other branch is super-Alfvenic and the soliton velocity is very close to or greater than the Alfven speed. Both compressive and rarefactive solitons can exist. For the sub-Alfvenic branch
the rarefactive soliton is bell-shaped and it is much narrower than the compressive one. However
for the super-Alfvenic branch
the compressive soliton is bell-shaped and narrower
and the rarefactive one is broadened. When the charge-to-mass ratio of the dust grains is sufficiently high
the width of the rarefactive soliton
in the super-Alfvenic branch
will broaden extremely and a electron depletion will be observed. It is also shown that the bell-shaped soliton can transition to a cusped structure when the velocity is sufficiently high. (C) 2008 American Institute of Physics.
From equivalence principles to cosmology: Cosmic polarization rotation, CMB observation, neutrino number asymmetry, Lorentz invariance and CPT
期刊论文
PROGRESS OF THEORETICAL PHYSICS SUPPLEMENT, 2008, 卷号: 172, 期号: 172, 页码: 49-60
作者:
Ni, Wei-Tou
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浏览/下载:84/0
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提交时间:2011/12/29
PROBE WMAP OBSERVATIONS
ANGULAR POWER SPECTRUM
DISTANT RADIO-SOURCES
2003 FLIGHT
INERTIAL MASS
LAMB SHIFT
ANISOTROPY
LIMITS
BIREFRINGENCE
BOOMERANG
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