Identification of the interstellar cyanomethyl radical (CH2CN) in the molecular clouds TMC-1 and Sagittarius B2

We report the astronomical identification of the cyanomethyl radical, CH2CN, the heaviest nonlinear molecular radical to be identified in interstellar clouds. The complex fine and hyperfine structures of the lowest rotational transitions at about 20.12 and 40.24 GHz are resolved in TMC-1, where the abundance appears to be about 5 x 10(-9) relative to that of H2. This is significantly greater than the observed abundance of CH3CN (methyl cyanide) in TMC-1. In Sgr B2 the hyperfine structure is blended in the higher frequency transitions at 40, 80, and 100 GHz, although the spin-rotation doubling is clearly evident. Preliminary searches in other sources indicate that the distribution of CH2CN is similar to that for such carbon chain species as HC3N or C4H.     

Chemical abundances in cold, dark interstellar clouds

The Sun may well have formed in the type of interstellar cloud currently referred to as a cold, dark cloud. We present current tabulations of the totality of known interstellar molecules and of the subset which have been identified in cold clouds. Molecular abundances are given for two such clouds which show interesting chemical differences in spite of strong physical similarities, Taurus Molecular Cloud 1 (TMC-1) and Lynd's 134N (L134N, also referred to as L183). These regions may be at different evolutionary stages.     

南沙他国侵占岛礁战略价值及空间格局评价

从建岛潜力、岛礁辐射能力和岛礁承载能力3个方面选取26个指标,采用主客观综合赋权法确定各因子权重,利用线性加权法获得被越南、菲律宾、马来西亚、文莱等国所侵占的南沙44个岛礁的战略价值,并对结果进行空间插值,分析其空间格局特征。结果表明：1）被马来西亚侵占的弹丸礁、越南侵占的南威岛、以及菲律宾侵占的中业岛,其战略价值位列前3,评价得分分别为100、98.42和97.09。2）岛礁辐射能力空间分布格局呈现“NW—SE条带式”,“最高”和“高”等级的区域由研究区西北延伸至东南,然后向东北、西南两侧递减,辐射能力格局中有2个核心区域和2个次级核心区域。承载能力空间分布格局呈现“横向条带式”,由北向南越来越低,有1个核心区域和2个次级核心区域。建岛潜力空间分布格局有3个核心区域及2个次级核心区域。3）岛礁战略价值空间分布格局有3个核心区域,分布于研究区中部、北部及南部,与越南、菲律宾、马来西亚密切相关的核心区域各有1个。越南侵占岛礁最多且空间分布较广,有2个次级核心区域也与越南密切相关,越占岛礁若进一步建设,将形成多核心协同的战略格局,需密切关注。     

A search for millimeter wave spectral lines from comet Sugano-Saigusa-Fujikawa (1983e)

The search for radio spectral lines from Comet Sugano-Saigusa-Fujikawa (1983e) was conducted using the 45-m telescope of Nobeyama Radio Observatory. The frequency ranges of 44.0–46.0 and 47.5–49.5 GHz were surveyed down to $\text{ΔT}{}_{\mathrm{<mtext>A</mtext>}}{}^1\text{(}\text{rms}\text{) = 20–30}\text{mK}$, with a beam size of ～35 arc sec. Upper limits have been established for spectral lines of atomic hydrogen, CS, OCS, SO₂, H₂CO, CH₃OH, HCCCCCN, HCOOCH₃, CH₃OCH₃, and CH₃CH₂CN. The J = 5?4 line from HCCCN in the vibrational ground state possibly has been detected but not confirmed. The suggested total amount of HCCCN in the coma is consistent with the possible picture that HCCCN is the main parent molecule of CN.     

以“多规合一”村庄规划为抓手探索乡村振兴困境和对策

近年来,我国已初步构建起乡村振兴战略的“四梁八柱”,然而,乡村振兴战略行动计划实施以来,因缺乏科学规划的引领,乡村振兴内生动力不足、成效不显著。旨在厘清“多规合一”村庄规划对实施乡村振兴意义的基础上,分析目前乡村振兴战略在指导乡村发展的过程中存在的难点和堵点,探索以编制“多规合一”村庄规划为抓手,从规划理念、规划内容、规划管控、规划方式、规划队伍、规划支撑、规划指导等方面探索解决问题的途径。     

准噶尔盆地深层致密油储层特征及致密化成因——以莫索湾—莫北地区侏罗系八道湾组为例

综合利用岩心、岩石薄片、扫描电镜及测井等资料,对准噶尔盆地莫索湾—莫北地区侏罗系八道湾组致密油储层特征及其致密化成因进行研究。结果表明:八道湾组储层为低—特低孔、低—特低渗储层,属典型的深层致密砂岩储层;储层砂体主要为三角洲前缘水下分流河道细砂岩、中—细砂岩,成分成熟度低,具有岩屑和塑性岩屑含量高及胶结物含量低的"两高一低"特征;垂向上以4 100和4 500m为界,可划分为减小原生孔、稳定混合孔及增加次生孔3个孔隙演化带;孔隙主要为中—小孔,孔喉类型以分选较差的中-细孔—细喉型为主,连通性和渗流能力相对较差,结构相对较差。储层致密化主要受控于沉积环境相对稳定性、岩石主要成分、储层埋藏深度及胶结物赋存状态4个因素,构成了致密化的背景、内因和外因;相对稳定的沉积环境、低成分成熟度、高岩屑和塑性岩屑含量、储层埋深大、压溶作用大量减孔,以及不同类型胶结物以4种状态充填孔喉,形成了八道湾组致密储层。     

High sensitivity SiO maser survey for mira variables

Simultaneous observations of the six transitions of SiO for 106 late-type stars were made. The SiO maser emission was detected in 83 stars. Thev=3 maser emission was detected in eight stars, and the²⁹SiOv=0 emission in six stars. The²⁹SiOv=0 emission is stronger and narrower than that of²⁸SiO, suggesting that the²⁹SiO emission is masing.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984.     

Laboratory detection of a new interstellar free radical CH2CN(2B1)

An asymmetric-top free radical CH2CN, which as a 2B1 ground state, was detected for the first time by laboratory microwave spectroscopy. The radical was produced in a free-space absorption cell by a DC glow discharge in pure CH3CN gas. About 60 fine-structure components were observed for the N = 11-10 to 14-13 a-type rotational transitions in the frequency region of 220-260 GHz, and many hyperfine resolved components for the N = 4-3 and 5-4 transitions in the 80 and 100 GHz regions, respectively. The molecular constants, including the rotational constants, centrifugal distortion constants, and spin-rotation coupling constants with centrifugal distortion correction terms were determined from the fine-structure resolved transitions, and the hyperfine coupling constants due to the hydrogen and nitrogen nuclei were obtained from the low-N transitions. As a result we assigned U100602 and U80484 from Sgr B2, and U40240 and U20120 from TMC-1, to the N = 5-4, 4-3, 2-1, and 1-0 transitions with K-1 = 0 of the CH2CN radical.     

卡尔曼滤波在短期气候预测中的应用

用PRESS准则和最优子集回归选取预测因子，建立河西走廓东部月平均气温的卡尔曼滤波预测模型，经实际使用发现，该预测方法的精度较高，稳定性较好，为短期气候提供了一种新的思路和方法。     

几次地震前的电磁波异常变化

1.震前电磁波异常的观测据有关研究,震前辐射的电磁波频谱很宽,从超极低频到超高频都可能存在。因此,观测震前电磁波异常最好采用多频段接收方式。但是目前我们只能接收某频段的电磁波。一般测点都远离震中,因此,采用低频甚至超低频观测系统是比较合适的。我们使用GCI-1A型磁场传感器作接收天线,与DJ-1型地震仪配合。这种传感器是采用一种高导磁