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1.
电视行同步频率综合器的研制 总被引：1，自引：0，他引：1
叙述了最新研制的一种标准频率综合器。它通过直接接收中央电视台１、２或４套节目的全电视信号,利用行同步脉冲,便可输出人们常用的１０ＭＨｚ、５ＭＨｚ、１ＭＨｚ、１００ＫＨｚ标准频率信号．经测试,秒级短稳１×１０－９;频率准确度估计可达１０－１２。该设备既能对无线电频率直接进行计量和校准,也可作为标准频率信号源使用。 相似文献
2.
位于日冕微波区的微波Ⅲ型爆发界面频率的发现 总被引：3，自引：0，他引：3
在北京天台１．０－２．０ＧＨｚ射电频谱仪记录到的１９９４年１月５日爆发图上，首次发现一界面频率位于１２４０ＭＨｚ与１３４０ＭＨｚ之间的微波Ⅲ型爆发对，其频率漂率为－０．２２ＧＨｚ／ｓ和＋０．２３ＧＨｚ／ｓ由此推出电子加速区位于光球之上，３．７×１０＾４ｋｍ的高度，电子加速区及Ⅲ型爆发形成区的高度范围约为１０００公里，而电子束的速度相应为０．１０２ｃ及０．１０６ｃ。 相似文献
3.
我们用新的时间分辨率短至８ｍｓ 的２ ．６ ～３ ．８ＧＨｚ 微波动态频谱仪在１９９８ 年４ 月１５ 日爆发和１９９７ 年１１ 月３ 日爆发中发现了微Ｕ 型爆发。其顶部频率为３ ．２ ～３ ．４ＧＨｚ（ 相应的等离子体密度：基波：１ ．２ ×１０１１ － １ ．４ ×１０１１／ｃｍ ３ ,二次谐波：３ ．２ ×１０１０ － ３ ．５ ×１０１０／ｃｍ ３） ;根部频率为３ ．４ ～３ ．６ＧＨｚ;单个Ｕ 型爆发的频率范围为６０ ～２２０ ＭＨｚ ;上升段频漂率为７ ～２８ＧＨｚ／ｓ;上升段持续时间为８ ～２４ｍｓ;寿命为１６ ～４８ｍｓ;偏振度大于８０ ％ 。在活动区为偶极子磁场的假设下,估计源区高度约为１ ．３ ×１０４ 公里,单一环的高度为２５０ ～８００ 公里。由此得出结论：１ ．由于高频漂率和高偏振度,似乎发现的微Ｕ 型爆发不是Ⅲ型爆发形成,而是尖峰辐射（Ｓｐｉｋｅ） 形成。２ ．我们发现的是小尺度的微磁环,其尺度与Ｓｐｉｋｅ 辐射的寿命相当。我们在１９９７ 年１１ 月２ 日的爆发中发现平均周期为数十ｍｓ 的准周期振荡群。在高密度流管的磁声波ＭＨＤ 振荡条件下,可取得磁环半径约９０ 公里的结果。由此可以得到微磁环物理尺度的图象 相似文献
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利用北京天文台 ２．６—３．８ ＧＨｚ频谱仪的观测资料,找到 １１个微波尖峰辐射事件．尖峰一般具有数十毫秒的寿命,数百个ｓｆｕ的流量密度和数十至数百ＭＨｚ的带宽,这与以前的报道类似．尖峰的偏振度各式各样,有的尖峰还有数千ＭＨｚ／ｓ的频率漂移．某些尖峰在二个偏振态之间有８毫秒的时间延迟（最大延迟可达１６毫秒）．另外,还发现了尖峰的偏振度随频率剧烈变化的偏振反转现象． 相似文献
6.
介绍ＢＰＭ短波授时台新的载频产生器的设计与实现，该ＢＰＭ载频产生器以原子频标的５ＭＨｚ标频信号为参考，利用频率合成技术，产生出供发射机使用的２．５ＭＨｚ、５ＭＨｚ，１０ＭＨｚ、１５ＭＨｚ和２０ＭＨｚ五种高准确度的载频信号。这些信号既能单独输出，也可利用面板控制或遥控选择输出。为了保证系统的可靠性，采用了两冗余结构，并设置了必要的报警与指示。 相似文献
7.
给出了来自新发现的孤立中子星１ＥＳ１８５３－３７９方向的γ射线上限为５×１０－８ｐｈｃｍ－２ｓ－１．假设γ射线辐射的立体角的成束和１ＧｅＶ的平均光子能量,对应的１光度上限为７．６×１０~２３（Ｄ／１００ｐｃ）２Ｊ／ｓ．导出的γ射线辐射效率上限比极冠模型或外间隙模型所预期的辐射效率低两个量级．由此给出了这一中子星自转参数的限制． 相似文献
8.
用于分子谱线观测的512路数字式自相关频谱仪 总被引：1，自引：0，他引：1
本文简要介绍了采用一比特自相关技术实现的５１２路数字式自相关频谱仪的工作原理及系统的硬件和软件构成。该频谱仪主要用于分米及ｃｍ波段分子谱线观测。频谱仪系统时钟可在６２５ＫＨｚ和２０ＭＨｚ之间按２的倍率选择，最大分析带宽为１０ＭＨｚ。最高频率分辨率为０．６１ＫＨｚ，相应于１８ｃｍ波段的速度分辨率为０．１ｋｍ／ｓ。文章最后给出了利用上海天文台２５ｍ射电望远镜观测ＯＨ脉泽源的结果。 相似文献
9.
俞志尧 《中国天文和天体物理学报》1994,(1)
我们从对Ｏｒｉｏｎ－ＫＬ星云中ＯＨ１６６５ＭＨｚ脉泽的单基线干涉观测的分析中,提出一种新的外流模型,即多重分离的旋转膨胀环．这种模型与观测结果是一致的．通过对２４ｋｍ单基线观测得到的１９个ＯＨ１６６５ＭＨｚ脉泽斑点的相对位置图进行分析、统计、拟合和计算,得到这１９个ＯＨ１６６５ＭＨｚ脉泽斑点分别分布在三个旋转膨胀环上．这三个旋转膨胀环的视距分别为３＂．８１,５＂．８７,６＂．０;对应的环半径分别为１７４２,２７２０,２７６６ＡＵ;径向膨胀速度分别为７．０７,１６．４,２６．４ｋｍｓ－１;旋转运动的切向线速度分别为１．５５,１．２３,１．２１ｋｍｓ－１． 相似文献
10.
用云南天文台高时间分辨率（１０ｍｓ）高频率分辨率（０．５ＭＨｚ）的射电频谱仪观测分析证认了米波窄带短持续时间快频漂爆发的存在．这种爆发既不同于经典的ＩＩＩ型爆发，也不同于ｓｐｉｋｅ和Ｉ型爆发，是一种新的米波爆发型别．它的特性与分米波的“ｂｌｉｐｓ”相近． 相似文献
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《中国天文和天体物理学报》2014,(10)
正Research in Astronomy and Astrophysics publishes original research papers and reviews on all branches of astronomy and astrophysics.Reviews are by invitation only.Important new results that require rapid publication can be submitted as a Letter(Letters must be restricted in length to 6 printed pages).Authors who submit a paper are expected to be able to certify that the paper is original work, 相似文献
13.
Laura Schaefer 《Icarus》2005,173(2):454-468
We use chemical equilibrium calculations to model the speciation of alkalis and halogens in volcanic gases emitted on Io. The calculations cover wide temperature (500-2000 K) and pressure (10−6 to 10+1 bars) ranges, which overlap the nominal conditions at Pele (T=1760 K, P=0.01 bars). About 230 compounds of 11 elements (O, S, Li, Na, K, Rb, Cs, F, Cl, Br, I) are considered. The elemental abundances for O, S, Na, K, and Cl are based upon observations. CI chondritic elemental abundances relative to sulfur are used for the other alkalis and halogens (as yet unobserved on Io). We predict the major alkali species in Pele-like volcanic gases and the percentage distribution of each alkali are LiCl (73%), LiF (27%); NaCl (81%), Na (16%), NaF (3%); KCl (91%), K (5%), KF (4%); RbCl (93%), Rb (4%), RbF (3%); CsCl (92%), CsF (6%), Cs (2%). Likewise the major halogen species and the percentage distribution of each halogen are NaF (88%), KF (10%), LiF (2%); NaCl (89%), KCl (11%); NaBr (89%), KBr (10%), Br (1%); NaI (61%), I (30%), KI (9%). We predict the major halogen condensates and their condensation temperatures at P=0.01 bar are NaF (1115 K), LiF (970 K); NaCl (1050 K), KCl (950 K); KBr (750 K), RbBr (730 K), CsBr (645 K); and solid I2 (200 K). We also model disequilibrium chemistry of the alkalis and halogens in the volcanic plume. Based on this work and our prior modeling for Na, K, and Cl in a volcanic plume, we predict the major loss processes for the alkali halide gases are photolysis and/or condensation onto grains. Their estimated photochemical lifetimes range from a few minutes for alkali iodides to a few hours for alkali fluorides. Condensation is apparently the only loss process for elemental iodine. On the basis of elemental abundances and photochemical lifetimes, we recommend searching for gaseous KCl, NaF, LiF, LiCl, RbF, RbCl, CsF, and CsCl around volcanic vents during eruptions. Based on abundance considerations and observations of brown dwarfs we also recommend a search of Io's extended atmosphere and the Io plasma torus for neutral and ionized Li, Cs, Rb, and F. 相似文献
14.
Yehouda Enzel Rivka Amit Uri Dayan Onn Crouvi Ron Kahana Baruch Ziv David Sharon 《Global and Planetary Change》2008,60(3-4):165-192
Modern-day synoptic-scale eastern Mediterranean climatology provides a useful context to synthesize the diverse late Pleistocene (60–12 ka) paleohydrologic and paleoenvironmental indicators of past climatic conditions in the Levant and the deserts to its south and east. We first critically evaluate, extract, and summarize paleoenvironmental and paleohydrologic records. Then, we propose a framework of eastern Mediterranean atmospheric circulation features interacting with the morphology and location of the southeast Mediterranean coast. Together they strongly control the spatial distribution of rainfall and wind pattern. This cyclone–physiography interaction enforces the observed rainfall patterns by hampering rainfall generation south and southeast of the latitude of the north Sinai coast, currently at 31°15′.The proposed framework explains the much-increased rains in Lebanon and northern Israel and Jordan as deduced from pollen, rise and maintenance of Lake Lisan, and speleothem formation in areas currently arid and semiarid. The proposed framework also accounts for the southward and eastward transition into semiarid, arid, and hyperarid deserts as expressed in thick loess accumulation at the deserts' margins, dune migration from west to east in the Sinai and the western Negev, and the formation of hyperarid (< 80 mm yr− 1) gypsic–salic soils in the southern Negev and Sinai. Our climatic synthesis explains the hyperarid condition in the southern Negev, located only 200–250 km south of the much-increased rains in the north, probably reflecting a steeper rainfall gradient than the present-day gradient from the wetter Levant into its bordering southern and eastern deserts.At present, the rainiest winter seasons in Lebanon and northern and central Israel are associated with more frequent (+ 20%), deeper Cyprus Lows traversing the eastern Mediterranean at approximately the latitude of southern Turkey. Even these wettest years in northern Israel do not yield above average annual rainfall amounts in the hyperarid southern Negev. This region is mainly influenced by the Active Red Sea Troughs that produce only localized rains. The eastern Mediterranean Cyprus Lows also produce more dust storms and transport higher amounts of suspended dust to the loess area than any other atmospheric pattern. Concurrent rainfall and dust are essential to the late Pleistocene formation of the elongated thick loess zone along the desert northern margin. Even with existing dust storms, the lack of rain and very sparse vegetation account for the absence of late Pleistocene loess sequences from the southern Negev and the formation of hyperarid soils.When the north Sinai coast shifted 30–70 km northwest due to last glacial global sea level lowering, the newly exposed coastal areas supplied the sand and dust to these active eastern Mediterranean cyclones. This enforced the latitude of the northern boundary of the loess zone to be directly due east of the LGM shoreline. This shift of coast to the northwest inhibited rainfall in the southern Levant deserts and maintained their hyperaridity. Concurrently, frequent deep eastern Mediterranean Cyprus Lows were funneled along the northern Mediterranean increasing (probably doubling) the rains in central and northern Israel, Lebanon, southwestern Syria and northern Jordan. These storms and rains formed lakes, forests, and speleothems only a short distance north of the deserts in the southern Levant. 相似文献
15.
Philippe Stee 《Astrophysics and Space Science》2003,286(1-2):225-236
Interferometry in the visible provides milliarcsecond spatial resolution and thus has been used for studying the circumstellar
environment of active hot stars. In this paper I will illustrate how the visibility modulus and phase can be used to better
constrain the physics of Be disks through results from the VLA, the MkII and the GI2T interferometers. I will insist on the
importance and the potential of coupling high angular resolution with high spectral resolution to the study of Be shells.
Finally I will present a possible study of the circumstellar disk of Be stars using the VLTI.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
16.
The central compact object for some gamma-ray bursts (GRBs) may be a strongly magnetized millisecond pulsar. It can inject energy to the outer shock of the GRB by through the magnetic dipole radiation, and therefore causes the shallow decay of the early afterglow. Recently, from a large number of GRB X-ray afterglows observed by Swift/XRT(X-ray telescope), it is revealed that many of them exhibit the shallow decay about 102∼104 s after the burst prompt emission. We have fitted the X-ray afterglow light curves of 11 GRBs by using the energy injection model of a magnetar with the rotation period in the millisecond order of magnitude. The obtained result shows the validity and universality of the magnetar energy injection model in explaining the shallow decay of afterglows, and simultaneously provides some constraints on the magnetic field strength and rotation period of the central magnetar. 相似文献
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Using the method of apparent motion parameters, we have studied the relative motion of the components in 561 pairs of wide (ρ > 2″) and relatively nearby (Hipparcos parallaxes > 0.01″) visual double stars based on data from the WDS catalog. The minimum masses of the double stars have been calculated at given parallaxes. We have identified 358 optical pairs. For 11 stellar pairs, we have found the minimum mass to exceed the estimate corresponding to their spectral types and luminosities. This excess is 5–7 M ⊙ for two stars, ADS 7446 and 9701. 相似文献
18.
V. Cardoso M.C. Espírito Santo M. Paulos M. Pimenta B. Tom 《Astroparticle Physics》2005,22(5-6):399-407
According to recent conjectures on the existence of large extra dimensions in our universe, black holes could be produced during the interaction of Ultra High Energy Cosmic Rays with the atmosphere. However, and so far, the proposed signatures are based on statistical effects, not allowing identification on an event by event basis, and may lead to large uncertainties. In this note, events with a double bang topology, where the production and instantaneous decay of a microscopic black hole (first bang) is followed, at a measurable distance, by the decay of an energetic tau lepton (second bang) are proposed as an almost background free signature. The characteristics of these events and the capability of large cosmic ray experiments to detect them are discussed. 相似文献
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As shown by statistical results, in the 23rd solar activity cycle the variation of the latitudes of rotating sunspots with time exhibits a butterfly pattern. We have studied the variations with phase for the mean square errors among the 4 fitting curves of the 2 wings of the butterfly diagram of sunspots and the 2 wings of the butterfly diagram of rotating sunspots in the 23rd solar activity cycle. The results show that a systematic time delay exists not only between the northern and southern hemispheres of the butterfly diagram of sunspots, but also between the northern and southern hemispheres of the butterfly diagram of rotating sunspots, even between the butterfly diagrams of the sunspots and rotating sunspots in the same hemisphere. This means that the 23rd-cycle sunspot activities in the northern and southern hemispheres happened not simultaneously, that a systematic time delay or advance (phase difference) exists between the northern and southern hemispheres, that the southern hemisphere lags behind the northern hemisphere, that a phase difference exists between the butterfly diagram of rotating sunspots and the butterfly diagram of sunspots in the 23rd cycle, and that the butterfly diagram of rotating sunspots lags behind that of sunspots. The observed delay is a little less than the theoretical value predicted by the dynamo model. 相似文献