排序方式： 共有9条查询结果，搜索用时 140 毫秒
1
1.
给出红外点源IRAS 20231 3440附近恒星形成区近红外．JHK’和H2成像观测结果，以及与该IRAS点源成协的近红外点源IRS1的K波段分光观测结果．．JHK’观测显示该区域存在嵌埋的年轻星天体，H2窄波段观测揭示了若干个氢分子发射结点，其中有几个结点排列成线形，暗示分子氢喷流的存在．喷流的北部与已知观测的分子外流成协，表明二者之间存在联系．喷流的走向提示IRS1可能是其激发源，对IRS1的K波段分光观测给出了进一步的证据．从近红外、MSX及IRAS资料估计出IRS1的能谱分布，表明它是一个处于ClassI状态的中等质量的年轻星天体． 相似文献
2.
Carbon and Noble Gas Isotopes in the Tengchong Volcanic Geothermal Area, Yunnan, Southwestern China 总被引：1，自引：0，他引：1
Carbon and noble gas isotope analyses are reported for bubbling gas samples from the Tengchong volcanic geothermal area near the Indo-Eurasian suture zone. All samples contain a resolvable component of mantle-derived 3He. Occurrence of mantle-derived 3He coincides with surface volcanism. However, 3He occurs over a larger geographic areathan do surface volcanics. δ13C values for CO2 and CH4 vary from -33.4‰ to 1.6 ‰ and from -52.8‰ to -2.8‰, respectively. He and C isotope systematics indicate that CO2 and CH4 in the CO2-rich gases originated predominantly from magmatic component mixed with crustal CO2 produced from carbonate. However, breakdown of organic matter and near-surface processes accounts for the CH4 and CO2 in N2-rich gases. 3He/4He ratio distribution pattern suggests that mantle-derived He and heat sources of high-temperature system in central Tengchong originate from a hidden magma reservoir at subsurface. CO2-rich gases with the highest 3He/4He ratio (5.2 Ra) may be representative of the 相似文献
3.
Yoichi Shimatsu 《山地科学学报》2004,1(2)
1 Introduction: A Dissonant Fragment On entering Chichibu, many visitors feel as if they were passing through a time warp into another country or a bygone era as the train leaves behind Tokyo抯crowded suburbs and winds through steep slopes forested with oaks, beeches and cedars. The Oku Chichibu highlands, however, are a mere 70 kilometers northwest of Tokyo, or about 50 minutes by rail, less than the average two-hour of daily commute of 搒alarymen?within metropolitan area. The sense of s… 相似文献
4.
Xiang Hongfa Yasutaka Ikeda Zhang Wanxia Zhang Bingliang Guo Shunmin and He HonglinInstitute of Geology CSB Beijing China Tokyo University Tokyo Japan 《中国地震研究》1999,(4)
Based on trench excavation and detailed field investigation, the authors have ascertained that 6 paleoearthquake events have occurred in the Haizixia area of the Eastern Liupanshan Piedmont fault zone since 46Ka B.P. The recurrence time of 6 events were about 15000a, 20250a, 14750a, 12150a, 8550a and 4000a B.P., respectively, the recurrence intervals were about 15000a, 5500a, 2600a, 3600a and 4550a, respectively. According to M-D empirical relations, the vertical dislocation of events 1 and 2 corresponded to the dislocation of the earthquake with M8.0; the vertical dislocation of events 3-6, was corresponded to the dislocation of earthquakes with M6.5~7.5. 相似文献
5.
位于中国西南的小江 (Xiaojiang)断裂带作为康定 (Kangding)断裂带的南段 ,在青藏块体向SE方向挤出的过程中起着重要的作用。根据断错地貌以及这些断错地貌14 C年代或热释光年代 ,推算了小江断裂带第四纪晚期的左旋走滑速率。小江断裂带可以分为 3段 ,其中段由平行的两条断层组成。西支断层和东支断层的左旋走滑速率分别为 7.0～ 9.0mm/ yr和 6 .0～ 7.5mm/yr。简单相加 ,就可以推算出小江 (Xiaojiang)断裂带总的左旋走滑速率为 13 0～ 16 5mm/ yr,与康定断裂带北段的鲜水河 (Xianshuihe)断层的走滑速率大致相当 ,约等于康定 (Kangding)断裂带中段的安宁河 (Anninghe)断层及则木河 (Zemuhe)断层的两倍。这个结果可能暗示了在康定断裂带中段 ,可能存在着其他断层以解消另外一半的滑动速率。最有可能的断层是位于康定断裂带中段以东几十公里的普雄河 -布拖 (Puxionghe Butuo)断层 相似文献
6.
采用激光拉曼、阴极发光和电子探针技术,确认冀西北石榴角闪二辉麻粒岩锆石中保存早期高压变质包体矿物组合:石榴石(Grt)+单斜辉石(Cpx)+斜长石(Pl)+石英(Qtz)+金红石(Rt)、单斜辉石(Cpx)+斜长石(Pl)+石英(Qtz)和石榴石(Grt)+单斜辉石(Cpx)+斜长石(Pl)+石英(Qtz)。其中少量锆石具有继承性锆石的核,而多数锆石则形成于高压麻粒岩相变质阶段。利用TWQ方法限定石榴角闪二辉麻粒岩锆石中所保存的高压包体矿物组合的变质温度条件为750～820℃,压力为1.07～1.40 GPa。该项研究成果对于如何识别高压麻粒岩以及深入研究其成因机制均具有重要的科学意义。 相似文献
7.
Shingo Yamada Forecast Division Japan Meteorological Agency Tokyo Japan Shuhei Maeda Administration Division Climate Marine Department Japan Meteorological Agency Tokyo Japan K. Gambo c/o Department of Earth Planetary Physi 《大气科学进展》1997,(1)
ＮｏｔｅｓｏｎＥｘｔｅｎｄｅｄ－ＲａｎｇｅＡｔｍｏｓｐｈｅｒｉｃＰｒｅｄｉｃｔｉｏｎｉｎｔｈｅＮｏｒｔｈｅｒｎＨｅｍｉｓｐｈｅｒｅＷｉｎｔｅｒＳｈｉｎｇｏＹａｍａｄａＦｏｒｅｃａｓｔＤｉｖｉｓｉｏｎ，ＪａｐａｎＭｅｔｅｏｒｏｌｏｇｉｃａｌＡｇｅｎｃｙ... 相似文献
8.
9.
Eijiro Hiei 《中国天文和天体物理学报》2004,4(4):377-389
After surveying the spectra of 39 prominences observed by the Multichannel Infrared Solar Spectrograph at Purple Mountain Observatory and the 25 cm coronagraph at the Norikura Solar Observatory, we found that about 28% of them show small spatial scale (6"- 8") and short time scale (tens of seconds to a few minutes), unusual large broadening and large shift velocities in spectral lines including Hα, Hβ, Hε, Ca Ⅱ H, Ca Ⅱ K, Ca2Ⅱ 8542 A, He Ⅰ D3 and HeⅠ 10830 A. We present in detail two typical events observed respectively on 2002 May 27 and 1981 August 2. The full-width at half maximum of the widest profile of the 2001 prominence is 1.8 A for Ha and 2.9 A for He I 10830 A, while that of the 1981 prominence is 5.3 A for Hβ, 3.6 A for Ca Ⅱ K, 4.0 A for Ca Ⅱ H and 2.8 A for He Ⅰ D3. Such broadenings generally occur at a level of several-thousand kilometres above the chromosphere. Further, most of these prominences manifest a rotation of (0.4-1.35) ×10-2 rad s-1 pointing to the Sun and large line 相似文献
1