Storing, processing, and transmitting state confidential information are strictly prohibited on this website
WANG Chen, HAN Jin-lin, SUN Xiao-hui, SHI Wei-bin, CHEN Mao-zheng, MA Jun. The Total Power Response to the Ground Radiation at 6cm Wavelength of the Urumqi 25m Radio Telescope at Nanshan Station[J]. Astronomical Research and Technology, 2007, 4(2): 181-187.
Citation: WANG Chen, HAN Jin-lin, SUN Xiao-hui, SHI Wei-bin, CHEN Mao-zheng, MA Jun. The Total Power Response to the Ground Radiation at 6cm Wavelength of the Urumqi 25m Radio Telescope at Nanshan Station[J]. Astronomical Research and Technology, 2007, 4(2): 181-187.

The Total Power Response to the Ground Radiation at 6cm Wavelength of the Urumqi 25m Radio Telescope at Nanshan Station

More Information
  • Received Date: April 27, 2006
  • Revised Date: September 14, 2006
  • Published Date: April 14, 2007
  • We present the result of intensive observations of the ground radiation around the Nanshan Station using the 6cm system of Urumqi 25m radio telescope.The response of the system to the ground radiation varies significantly in different directions of the sky.The response in the southwest direction, where there are many mountains, was saturated when the telescope pointed to the elevation of 8°;at the elevation of 60°, the response to the ground radiation still varied at a level of 0.3 K, larger than the system response to the Galactic Plane of 0.01~0.1K.Therefore the ground radiation affects the radio observation seriously.Using the observational data, we constructed a simple template of the ground radiation of the 6cm system in the directions of the sky.However, the accuracy of the template remains inadequate for real observations.
  • Articles Related

    [1]Sun Zhengxiong, Wang Jinqing, Yu Linfeng, Jiang Yongbin, Zhao Rongbing, Gou Wei, Wang Guangli. The High Precision Pointing Model Establishment of Tianma 13 m Radio Telescope [J]. Astronomical Techniques and Instruments, 2023, 20(1): 24-30. DOI: 10.14005/j.cnki.issn1672-7673.20220625.001
    [2]Fu Xiachuan, Wu Chao, Huang Maohai, Zhang Mo, Lu Xiaomeng. Research and Implementation of Transient Quick Response and Automatic Observation System [J]. Astronomical Research and Technology, 2017, 14(4): 452-460.
    [3]Zhu Shiyu, Wang Zhuang, Wang Mengnan, Dong Liang. Model-Based Mitigation of the Moving RFI in Radio Astronomy [J]. Astronomical Research and Technology, 2017, 14(3): 297-303.
    [4]Du Jing, Yan Yihua, Xu Zhicai, Yin Xinghui, Wang Wei, Tan Chengming, Chen Zhijun. Upgrading the Solar Radio Flux Telescope with the Frequency of 2.84GHz [J]. Astronomical Research and Technology, 2016, 13(1): 52-57.
    [5]Liu Bin, Li Jianbin, Dong Liang, Shi Shuobiao, Gao Guannan, Wang Min, Liu Lijia, Peng Bo. Observations of Extragalactic Radio Sources with the 40m Radio Telescope of the Yunnan Observatory [J]. Astronomical Research and Technology, 2012, 9(1): 7-13.
    [6]Song Qian, Cao Wenda. An Interpretation of a Radiation Damage Phenomenon of the Solar-ACCD [J]. Publications of the Yunnan Observatory, 1999, 0(S1): 139-142.
    [7]Chen Guoqiang. Reconstruction of the Local Oscillator with the Solar Radio Telescope at 2000Mc Wavelengths [J]. Publications of the Yunnan Observatory, 1995, 0(1): 42-46.
    [8]Huang Chaosong, Li Jun. NONLINEAR IONOSPHERIC RESPONSE TO THE ATMOSPHERIC GRAVITY WAVES [J]. Publications of the Yunnan Observatory, 1990, 0(S1): 44-48.
    [9]Pan Liande, Wang Suqin, Ma Lanxiang. STUDY ON THE RESPONSE OF THE D-REGION OF THE IONOSPHERE TO THE SOLAR BURSTS [J]. Publications of the Yunnan Observatory, 1990, 0(4): 263-266.
    [10]Zhong Lingsheng, Shan Yong, Qiu Zhengliu. The Ground-Based Spectrophotometry of Solar Radiation and Its Application [J]. Publications of the Yunnan Observatory, 1987, 0(1): 102-110.

Catalog

    Article views (109) PDF downloads (10) Cited by()

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return