Observing Forbush decreases in cloud at Shetland

被引:37
作者
Harrison, R. Giles [1 ]
Ambaum, Maarten H. P. [1 ]
机构
[1] Univ Reading, Dept Meteorol, Reading RG6 6BB, Berks, England
基金
美国国家科学基金会;
关键词
Cosmic rays; Diffuse fraction; Atmospheric electricity; Solar climate; GLOBAL ELECTRIC-CIRCUIT; GALACTIC COSMIC-RAYS; ATMOSPHERIC ELECTRICITY; AEROSOL-PARTICLES; SOLAR-WIND; CLIMATE; CONDENSATION; VARIABILITY; ENHANCEMENT; TROPOSPHERE;
D O I
10.1016/j.jastp.2010.09.025
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Meteorological measurements from Lerwick Observatory, Shetland (60 degrees 09'N, 1 degrees 08'W), are compared with short-term changes in Climax neutron counter cosmic ray measurements. For transient neutron count reductions of 10-12%, broken cloud becomes at least 10% more frequent on the neutron minimum day, above expectations from sampling. This suggests a rapid time scale (similar to 1 day) cloud response to cosmic ray changes. However, larger or smaller neutron count reductions do not coincide with cloud responses exceeding sampling effects. Larger events are too rare to provide a robust signal above the sampling noise. Smaller events are too weak to be observed above the natural variability. (C) 2010 Elsevier Ltd. All rights reserved.
引用
收藏
页码:1408 / 1414
页数:7
相关论文
共 50 条
  • [31] Precursory Signals of Forbush Decreases Not Connected with Shock Waves
    D. Lingri
    H. Mavromichalaki
    M. Abunina
    A. Belov
    E. Eroshenko
    I. Daglis
    A. Abunin
    Solar Physics, 2022, 297
  • [32] Large Forbush Decreases and their Solar Sources: Features and Characteristics
    M. Papailiou
    M. Abunina
    A. Belov
    E. Eroshenko
    V. Yanke
    H. Mavromichalaki
    Solar Physics, 2020, 295
  • [33] Large Forbush Decreases and their Solar Sources: Features and Characteristics
    Papailiou, M.
    Abunina, M.
    Belov, A.
    Eroshenko, E.
    Yanke, V
    Mavromichalaki, H.
    SOLAR PHYSICS, 2020, 295 (12)
  • [34] Precursory Signals of Forbush Decreases Not Connected with Shock Waves
    Lingri, D.
    Mavromichalaki, H.
    Abunina, M.
    Belov, A.
    Eroshenko, E.
    Daglis, I
    Abunin, A.
    SOLAR PHYSICS, 2022, 297 (02)
  • [35] Model of optical response of marine aerosols to Forbush decreases
    Bondo, T.
    Enghoff, M. B.
    Svensmark, H.
    ATMOSPHERIC CHEMISTRY AND PHYSICS, 2010, 10 (06) : 2765 - 2776
  • [36] Forbush decreases caused by paired interacting solar wind disturbances
    Shlyk, N. S.
    Belov, A., V
    Abunina, M. A.
    Abunin, A. A.
    Oleneva, V. A.
    Yanke, V. G.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2022, 511 (04) : 5897 - 5908
  • [37] Coronal Mass Ejections and Non-recurrent Forbush Decreases
    Belov, A.
    Abunin, A.
    Abunina, M.
    Eroshenko, E.
    Oleneva, V.
    Yanke, V.
    Papaioannou, A.
    Mavromichalaki, H.
    Gopalswamy, N.
    Yashiro, S.
    SOLAR PHYSICS, 2014, 289 (10) : 3949 - 3960
  • [38] Features of Forbush Decreases According to Satellite and Ground Based Detectors
    Lagoida, I. A.
    Voronov, S. A.
    Mikhailov, V. V.
    PHYSICS OF ATOMIC NUCLEI, 2024, 87 (02) : 86 - 92
  • [39] Coronal Mass Ejections and Non-recurrent Forbush Decreases
    A. Belov
    A. Abunin
    M. Abunina
    E. Eroshenko
    V. Oleneva
    V. Yanke
    A. Papaioannou
    H. Mavromichalaki
    N. Gopalswamy
    S. Yashiro
    Solar Physics, 2014, 289 : 3949 - 3960
  • [40] High-rigidity Forbush decreases: due to CMEs or shocks?
    Arunbabu, K. P.
    Antia, H. M.
    Dugad, S. R.
    Gupta, S. K.
    Hayashi, Y.
    Kawakami, S.
    Mohanty, P. K.
    Nonaka, T.
    Oshima, A.
    Subramanian, P.
    ASTRONOMY & ASTROPHYSICS, 2013, 555