Magnetic Field Strengths and Structures from Radio Observations of Solar Active Regions     

Chang－XiZhang  G.B.Gelfreikh 《中国天文和天体物理学报》2002,2(3):266-276

Radio observations of some active regions (ARs) obtained with the Nobeyama radioheliograph at λ=1.76cm are used for estimating the magnetic field strength in the upper chromosphere, based on thermal bremsstrahlung. The results are compared with the magnetic field strength in the photosphere from observations with the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station of Beijing Astronomical Observatory. The difference in the magnetic field strength between the two layers seems reasonable. The solar radio maps of active regions obtained with the Nobeyama radioheliograph, both in total intensity (I-map) and in circular polarizations (V-map), are compared with the optical magnetograms obtained with the SMFT. The comparison between the radio map in circular polarization and the longitudinal photospheric magnetogram of a plage region suggest that the radio map in circular polarization is a kind of magnetogram of the upper chromosphere. The comparison of the radio map in total intensity with the photospheric vector magnetogram of an AR shows that the radio map in total intensity gives indications of magnetic loops in the corona, thus we have a method of defining the coronal magnetic structure from the radio I-maps at λ=1.76 cm. Analysing the I-maps, we identified three components: (a) a compact bright source; (b) a narrow elongated structure connecting two main magnetic islands of opposite polarities (observed in both the optical and radio magnetograms); (c) a wide, diffuse, weak component that corresponds to a wide structure in the solar active region which shows in most cases an S or a reversed S contour, which is probably due to the differential rotation of the Sun. The last two components suggest coronal loops on different spatial scales above the neutral line of the longitudinal photospheric magnetic field.  相似文献   

H II regions and radio visibility of quasar nuclei     

L. I. Matveenko 《Astronomy Letters》2001,27(11):686-690

The core (injector) and the jet (relativistic plasma outflow) of AGN objects are surrounded by an ionized medium, an H II region observed in emission lines. The synchrotron radiation from the core and the jet is observed through a thin screen that cocoons the structure under consideration. The screen transparency depends on wavelength and distance from the injector. We consider the objects 3C 345 and 1803+784 whose core emission at decimeter wavelengths is absorption by more than 25 dB. The visible bright compact component is the bright nearby portion of the jet that extends outside the dense part of the screen. We explore the possibility of measuring the screen transparency from absorption in Hα recombination lines with different quantum numbers at centimeter wavelengths.  相似文献   

High-speed outflows driven by the 30 Doradus starburst     

M. P. Redman  Z. A. Al-Mostafa  J. Meaburn  M. Bryce 《Monthly notices of the Royal Astronomical Society》2003,344(3):741-747

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The Eye of the Tornado – an isolated, high-mass young stellar object near the Galactic Centre     

M. G. Burton  J. S. Lazendic †  F. Yusef-Zadeh  M. Wardle 《Monthly notices of the Royal Astronomical Society》2004,348(2):638-646

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Mid-infrared observations of methanol maser sites and ultracompact H ii regions: signposts of high-mass star formation     

A.J. Walsh  F. Bertoldi  M.G. Burton  T. Nikola 《Monthly notices of the Royal Astronomical Society》2001,326(1):36-56

N -band (10.5 μm) and/or Q -band (20.0 μm) images taken with MANIAC on the ESO/MPI 2.2-m telescope are presented for 31 methanol maser sites and 19 ultracompact (UC) H  ii regions. Most of the maser sites and UC H  ii regions are coincident with mid-infrared (MIR) sources to within the positional uncertainties of ∼ 3 arcsec, consistent with the maser emission being powered by the MIR source. The IRAS source positions, however, do not always coincide with the MIR sources.
Based on an average infrared spectral energy distribution, we deduce that the MIR objects are luminous enough that they should also produce a strong ionizing radiation. Some sources are consistent with stars of later spectral type, but not all can be. A number of maser sites show no detectable radio continuum emission associated with MIR emission, despite a powering source luminous enough potentially to produce an UC H  ii region. Since no signs of an UC H  ii region are detected here, these maser sites might be produced during a very early stage of stellar evolution.
We present objects that show evidence of outflow activity stemming from a maser site, exhibiting CO and/or CS line profiles indicative of outflows coincident with the MIR source. These cases are promising examples of maser sites signposting the earliest stages of high-mass star formation.  相似文献   

Diffuse radiation,twilight, and photochemistry — I     

D. J. Lary  J. A. Pyle 《Journal of Atmospheric Chemistry》1991,13(4):373-392

A photochemical scheme which includes a detailed treatment of multiple scattering up to solar zenith angles of 96° (developed for use in a GCM) has been used to study partitioning within chemical families. Attention is drawn to the different zenith angle dependence of diffuse radiation for the two spectral regions <310 nm and >310 nm. The effect that this has on the so-called 40 km ozone problem is discussed. The importance of correctly including multiple scattering for polar ozone studies is emphasised.  相似文献   

Salmon lice, Lepeophtheirus salmonis (Kroyer), infestation in sympatric populations of Arctic char, Salvelinus alpinus (L.), and sea trout, Salmo trutta (L.), in areas near and distant from salmon farms     

Bjorn  Pal Arne; Finstad  Bengt 《ICES Journal of Marine Science》2002,59(1):131-139

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Growth of polar cod, Boreogadus saida (Lepechin), in the Barents Sea     

Gjosaeter  Harald; Ajiad  Adnan M. 《ICES Journal of Marine Science》1994,51(1):115-120

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用于极地的中尺度大气模式Polar MM5的改进和检验   总被引：1，自引：0，他引：1  

马艳  陈尚  张庆华 《海洋科学进展》2007,25(1):9-14

介绍了一个用于极地研究的中尺度大气模式———Polar MM5,阐述了该模式区别于标准的中尺度大气模式MM5的动力学和物理特征。利用Polar MM5获得了10 d的模拟结果表明,Polar MM5能较好地模拟高纬度地区近地面气象变量特征,尤其是对近地面温度和水汽混合比可得到高精度模拟结果,证实了在高纬度地区对标准MM5所进行的物理参数化方案的改进是切实有效的。  相似文献   

Organochlorine contaminants in fish and polycyclic aromatic hydrocarbons in sediments from the Barents Sea   总被引：2，自引：0，他引：2  

Stange  Kari; Klungsoyr  Jarle 《ICES Journal of Marine Science》1997,54(3):318-332

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