Scaling-laws of Radio Spike Bursts and Their Constraints on New Solar Radio Telescopestwo     

Tan Bao-lin  Cheng Jun  Tan Cheng-ming  Kou Hong-xiang 《Chinese Astronomy and Astrophysics》2019,43(1):59-74

Radio observation is one of important methods in solar physics and space science. Sometimes, it is almost the sole approach to observe the physical processes such as the acceleration, emission, and propagation of non-thermal energetic particles, etc. So far, more than 100 solar radio telescopes have been built in the world, including solar radiometers, dynamic spectrometers, and radioheliographs. Some of them have been closed after the fulfillment of their primary scientific objectives, or for their malfunctions, and thus replaced by other advanced instruments. At the same time, based on some new technologies and scientific ideas, various kinds of new and much more complicated solar radio telescopes are being constructed by solar radio astronomers and space scientists, such as the American E-OVSA and the solar radio observing system under the framework of Chinese Meridian Project II, etc. When we plan to develop a new solar radio telescope, it is crucial to design the most suitable technical parameters, e.g., the observing frequency range and bandwidth, temporal resolution, frequency resolution, spatial resolution, polarization degree, and dynamic range. Then, how do we select a rational set of these parameters? The long-term observation and study revealed that a large strong solar radio burst is frequently composed of a series of small bursts with different time scales. Among them, the radio spike burst is the smallest one with the shortest lifetime, the narrowest bandwidth, and the smallest source region. Solar radio spikes are considered to be related to a single magnetic energy release process, and can be regarded as an elementary burst in solar flares. It is a basic requirement for the new solar radio telescope to observe and discriminate these solar radio spike bursts, even though the temporal and spatial scales of radio spike bursts actually vary with the observing frequency. This paper presents the scaling laws of the lifetime and bandwidth of solar radio spike bursts with respect to the observing frequency, which provide some constraints for the new solar radio telescopes, and help us to select the rational telescope parameters. Besides, we propose a spectrum-image combination mode as the best observation mode for the next-generation solar radio telescopes with high temporal, spectral, and spatial resolutions, which may have an important significance for revealing the physical essence of the various non-thermal processes in violent solar eruptions.  相似文献   

两郧断裂郧县盆地段地质与地球物理特征研究     

林松  李媛  王薇  廖武林  乔岳强 《大地测量与地球动力学》2019,39(2):148-152

通过野外地质调查，结合地球物理探测手段，研究两郧断裂郧县盆地段地质与地球物理特征；参照两郧断裂带多个位置采集断层物质的SEM、TL测试成果，并结合本次对断层上断点沉积物OSL测年数据，对两郧断裂该段第四纪活动性进行分析。研究结果表明，两郧断裂在郧县盆地段埋深相对较深；断裂特征主要为逆断层，部分分支断裂显示为正断性质；断裂带最新活动时代为中更新世晚期-晚更新世早期。  相似文献   

福建大田—漳平地区构造-热对煤系石墨成矿及赋存的控制探讨     

丁正云  王路  曾欢  李阳  陈泉霖  邓瑞锦  程乔  林晓炎  曹代勇 《煤田地质与勘探》2020,48(1):55-61

福建省大田—漳平地区位于东部滨太平洋构造带上，不同时期的岩浆热液作用和复杂多变的构造形变格局，为该地区形成丰富的石墨矿床提供了良好的成矿条件。为了查明大田—漳平地区煤系石墨的成矿控制因素及分布规律，通过工业分析、元素分析、X射线衍射和激光拉曼光谱等实验，对不同矿区不同变质程度的煤和煤成石墨的化学组成及微观结构特征等煤成石墨化特征进行了研究，并将不同变形特征的样品划分为煤成石墨、煤成半石墨和石墨化无烟煤三大类。研究表明:煤的变形特征与煤成石墨的演化类型基本一致，且韧性变形样品的石墨化程度最高，说明构造应力作用能促进煤的石墨化作用；煤成石墨的分布受到岩浆-构造活动的控制，石墨矿床多产出于岩浆岩侵入体外接触带或附近断裂带的有利围岩地层中，且大田—漳平地区煤系石墨矿具有明显的成区、成带分布特点，煤成石墨成矿区主要集中在闽西南坳陷南部的漳平一带；而北部大田一带分布的矿区矿体石墨化程度较漳平一带低，多为煤成半石墨或石墨化无烟煤，研究结果可为该地区煤系石墨矿产综合勘探开发利用提供有利依据。   相似文献   

A shift towards wetter and windier conditions in southern Sweden around the prominent solar minimum 2750 cal a BP          下载免费PDF全文

ANETTE MELLSTRÖM  NATHALIE VAN DER PUTTEN  RAIMUND MUSCHELER  RIXT DE JONG  SVANTE BJÖRCK 《第四纪科学杂志》2015,30(3):235-244

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长蛸的盐度耐受性及盐度胁迫对其血细胞和体内酶活力的影响   总被引：1，自引：0，他引：1  

张玉玉  王春琳  李来国 《台湾海峡》2010,29(4):452-459

通过控制暂养水体盐度,用盐度突变与盐度渐变2种方法测定长蛸的盐度耐受性.测定了长蛸血细胞密度、各类血细胞数量比例以及各种酶的活力几组数据,并分析其血细胞与体内酶活力的变化.结果表明：长蛸的生存盐度范围为7.0~30.3,适宜盐度范围为16.3~27.3,最适盐度范围为18.3~24.3,对盐度的适应范围较广,有利于长蛸大规模养殖的开展.在盐度胁迫下,长蛸血细胞密度,各种血细胞数量比例均发生显著改变,长蛸个体也随着胁迫加大变得越来越不适应,出现喷墨、休克、甚至死亡,这表明长蛸的免疫机能降低.无论在低盐度还是高盐度胁迫情况下,受渗透压的影响,长蛸肌体大量吸水和失水,呼吸作用减弱,体内供氧降低,导致长蛸体内有氧呼吸降低和无氧呼吸提高,于是催化有氧呼吸的LDH酶活力降低.同时,细胞内与免疫和消化相关的细胞器由于细胞吸水或失水作用功能受到影响,保护酶（SOD、POD、CAT）、磷酸酶（ACP、AKP）和消化酶（蛋白酶和脂肪酶）的活力均呈下降趋势.由此可见,盐度胁迫对长蛸的影响是显著的.  相似文献   

Symbiotic stars with spectral indication of bipolar ejection and stellar wind     

N.A. Tomov  M.T. Tomova  D.V. Bisikalo 《Astronomische Nachrichten》2014,335(2):178-188

Four out of a total of five symbiotic systems whose optical spectral lines contain satellite components indicating collimated ejection have an additional absorption of P Cyg type with different velocity. These systems are Z And, Hen 3‐1341, StHα 190, and BF Cyg. It is shown that the line profiles of every of these systems can be interpreted in the framework of a model of a collimated stellar wind from the hot compact component proposed initially to interpret the line profiles of Z And, observed during its last active phase after 2000. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Seven years photometry of the W UMa‐type eclipsing binary V2612 Oph     

O. zdarcan  G. Ta 《Astronomische Nachrichten》2014,335(8):833-840

We present the first long‐term Johnson UBVR observations and comprehensive photometric analysis of the W UMa‐type eclipsing binary V2612 Oph. Observations in the time interval between 2003 and 2009 enabled us to reveal the seasonal and long‐term variations of the light curve. Hence, we found that the mean brightness level of the light curve shows a variation with a period of 6.7 years. Maximum and minimum brightness levels of the light curve exhibit a variation from year to year which we attribute to a solar‐like activity. The O – C variation of eclipse timings of the system shows a decreasing parabolic trend and reveals a period decrease at a rate of P = 6.27×10^‐7 day yr^‐1 with an additional low‐amplitude sinusoidal variation that has a similar period as the long‐term brightness variations. Our light curve analysis shows that the system is a W‐subtype W UMa eclipsing binary. We calculated masses and radii of the primary and secondary components as M₁ = 1.28 M_⊙, M₂ = 0.37 M_⊙ and R₁ = 1.31 R_⊙, R₂ = 0.75 R_⊙, respectively. The derived absolute photometric parameters allow us to calculate a distance of 140 pc, which confirms that the system is a foreground star in the sky field of the Galactic open cluster NGC 6633. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Digitization of sunspot drawings by Spörer made in 1861–1894     

A. Diercke  R. Arlt  C. Denker 《Astronomische Nachrichten》2015,336(1):53-62

Most of our knowledge about the Sun's activity cycle arises from sunspot observations over the last centuries since telescopes have been used for astronomy. The German astronomer Gustav Spörer observed almost daily the Sun from 1861 until the beginning of 1894 and assembled a 33‐year collection of sunspot data covering a total of 445 solar rotation periods. These sunspot drawings were carefully placed on an equidistant grid of heliographic longitude and latitude for each rotation period, which were then copied to copper plates for a lithographic reproduction of the drawings in astronomical journals. In this article, we describe in detail the process of capturing these data as digital images, correcting for various effects of the aging print materials, and preparing the data for contemporary scientific analysis based on advanced image processing techniques. With the processed data we create a butterfly diagram aggregating sunspot areas, and we present methods to measure the size of sunspots (umbra and penumbra) and to determine tilt angles of active regions. A probability density function of the sunspot area is computed, which conforms to contemporary data after rescaling. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Multi‐frequency solar observations at Metsähovi Radio Observatory and KAIRA     

J. Kallunki  M. Uunila  D. McKay‐Bukowski 《Astronomische Nachrichten》2015,336(6):566-569

We describe solar observations carried out for the first time jointly with Kilpisjärvi Atmospheric Imaging Receiver Array (KAIRA) and Aalto University Metshovi Radio Observatory (MRO). KAIRA is new radio antenna array observing the decimeter and meter wavelength range. It is located near Kilpisjärvi, Finland, and operated by the SodankyläGeophysical Observatory, University of Oulu. We investigate the feasibility of KAIRA for solar observations, and the additional benefits of carrying out multi‐instrument solar observations with KAIRA and the MRO facilities, which are already used for regular solar observations. The data measured with three instruments at MRO, and with KAIRA during time period 2014 April–October were analyzed. One solar radio event, measured on 2014 April 18, was studied in detail. Seven solar flares were recorded with at least two of the three instruments at MRO, and with KAIRA during the chosen time period. KAIRA is a great versatile asset as a new Finnish instrument that can also be used for solar observations. Collaboration observations with MRO instruments and KAIRA enable detailed multi‐frequency solar flare analysis. Flare pulsations, flare statistics and radio spectra of single flares can be investigated due to the broad frequency range observations. The Northern locations of both MRO and KAIRA make as long as 15‐hour unique solar observations possible during summer time. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Correlation Between Total Lightning Activity and Precipitation Particle Characteristics Observed from 34 Thunderstorms     

ZHENG Dong  MENG Qing  ZHANG Yijun  DAI Jianhu  ZHONG Min 《Acta Meteorologica Sinica》2010,24(6):776-788

A total of 34 thunderstorms around Shanghai and Wuhan of China are analyzed in order to determine the relationship between total lightning activity and precipitation particle characteristics.Precipitation particle concentration data are obtained from the 2A12 product of TRMM/TMI(Tropical Rainfall Measuring Mission/TRMM Microwave Image) and lightning activity data are from the TRMM/LIS(Lightning Imaging Sensor) and SAFIR3000(Surveillance et Alerte Founder par Interferometric Radioelectirque).On a spatial ...  相似文献