Turbulent interstellar plasma and ultrahigh angular resolution in radio astronomy

被引：0
|
作者：
V. I. Shishov
机构：
[1] Astro Space Center of the Lebedev Institute of Physics,Pushchino Radio Astronomy Observatory
来源：
Astronomy Reports | 2001年 / 45卷
关键词：
Image Reconstruction; Radio Wave; Radio Emission; Radio Source; Angular Resolution;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The effects of the modulation of radio waves during their passage through turbulent interstellar plasma on measurements of the structure of radio sources made with ultrahigh angular resolution using space radio interferometers are considered. Typical scattering anglesϑscat, pl for an extragalactic radio source at various wavelengths are estimated from scattering observations for pulsars and extragalactic sources. The (ϕ0λ) plane, where ϕ0 is the source size and λ is the wavelength of the radio emission, can be divided into five regions, in which different regimes of radio-wave modulation and image reconstruction are realized. Possibilities for image reconstruction in each of these regions are investigated.
引用
收藏
页码：195 / 202
页数：7
相关论文
共 50 条
  • [41] Turbulent equipartition and homogenization of plasma angular momentum
    Guercan, Oe. D.
    Diamond, P. H.
    Hahm, T. S.
    PHYSICAL REVIEW LETTERS, 2008, 100 (13)
  • [42] Radio scintillation due to discontinuities in the interstellar plasma density
    Lambert, HC
    Rickett, BJ
    ASTROPHYSICAL JOURNAL, 2000, 531 (02): : 883 - 901
  • [43] Double plasma resonance and its manifestations in radio astronomy
    Zheleznyakov, V. V.
    Zlotnik, E. Ya
    Zaitsev, V. V.
    Shaposhnikov, V. E.
    PHYSICS-USPEKHI, 2016, 59 (10) : 997 - 1020
  • [44] Ukraine Institute of Radio Astronomy high-resolution radars
    Vavriv, DM
    IEEE AEROSPACE AND ELECTRONIC SYSTEMS MAGAZINE, 2005, 20 (10) : 19 - 24
  • [45] Near Memory Acceleration on High Resolution Radio Astronomy Imaging
    Corda, Stefano
    Veenboer, Bram
    Awan, Ahsan Javed
    Kumar, Akash
    Jordans, Roel
    Corporaal, Henk
    2020 9TH MEDITERRANEAN CONFERENCE ON EMBEDDED COMPUTING (MECO), 2020, : 227 - 232
  • [46] Lightweight and High Angular Resolution X-ray Optics for Astronomy
    Zhang, William W.
    EUV AND X-RAY OPTICS: SYNERGY BETWEEN LABORATORY AND SPACE II, 2011, 8076
  • [47] High angular. resolution Mid-IR astronomy at Concordia
    Ferrari-Toniolo, Marco
    HIGHLIGHTS OF ASTRONOMY, VOL 13, 2005, 13 : 964 - 964
  • [48] THE IMPACT OF SEISMICITY ON HIGH ANGULAR RESOLUTION ASTRONOMY: THE CASE OF THE CANARY ISLANDS
    Eff-Darwich, A.
    Garcia-Lorenzo, B.
    Bonatto, L.
    Hernandez-Gutierrez, L.
    Vinas, R.
    Rodriguez-Losada, J. A.
    Blanco, M. J.
    Munoz-Tunon, C.
    OPTICAL TURBULENCE: ASTRONOMY MEETS METEOROLOGY, 2009, : 342 - +
  • [49] X-ray astronomy with ultra-high angular resolution
    Braig, C
    Predehl, P
    UV AND GAMMA-RAY SPACE TELESCOPE SYSTEMS, PTS 1 AND 2, 2004, 5488 : 601 - 612
  • [50] A review of high angular resolution observations of radio supernovae
    Marcaide, JM
    RADIO EMISSION FROM THE STARS AND THE SUN, 1996, 93 : 134 - 140
12345