Latitudinal profile of the ionospheric disturbance dynamo magnetic signature: comparison with the DP2 magnetic disturbance

被引:23
|
作者
Zaka, K. Z. [1 ]
Kobea, A. T. [1 ]
Assamoi, P. [1 ]
Obrou, O. K. [1 ]
Doumbia, V. [1 ]
Boka, K. [1 ]
Adohi, B. J. -P. [1 ]
Mene, N. M. [1 ]
机构
[1] Univ Cocody, Lab Phys Atmosphere, Abidjan 22, Cote Ivoire
关键词
Ionosphere; Equatorial ionosphere; Ionosphere-magnetosphere interactions; Ionospheric disturbances; ELECTRIC-FIELD; MAGNETOSPHERIC CONVECTION; INTERPLANETARY; STORMS; TIME; FLUCTUATIONS; PENETRATION; PARAMETERS; MODEL;
D O I
10.5194/angeo-27-3523-2009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
During magnetic storms, the auroral electrojets intensification affects the thermospheric circulation on a global scale. This process which leads to electric field and current disturbance at middle and low latitudes, on the quiet day after the end of a storm, has been attributed to the ionospheric disturbance dynamo (Ddyn). The magnetic field disturbance observed as a result of this process is the reduction of the H component amplitude in the equatorial region which constitutes the main characteristic of the ionospheric disturbance dynamo process, associated with a westward electric current flow. The latitudinal profile of the Ddyn disturbance dynamo magnetic signature exhibits an eastward current at mid latitudes and a westward one at low latitudes with a substantial amplification at the magnetic equator. Such current flow reveals an "anti-Sq" system established between the mid latitudes and the equatorial region and opposes the normal Sq current vortex. However, the localization of the eastward current and consequently the position and the extent of the "anti-Sq" current vortex changes from one storm to another. Indeed, for a strong magnetic storm, the eastward current is well established at mid latitudes about 45 degrees N and for a weak magnetic storm, the eastward current is established toward the high latitudes (about 60 degrees N), near the Joule heating region, resulting in a large "anti-Sq" current cell. The latitudinal profile of the Ddyn disturbance as well as the magnetic disturbance DP2 generated by the mechanism of prompt penetration of the magnetospheric convection electric field in general, show a weak disturbance at the low latitudes with a substantial amplification at the magnetic equator. Due to the intensity of the storm, the magnitude of the DP2 appears higher than the Ddyn over the American and Asian sector contrary to the African sector.
引用
收藏
页码:3523 / 3536
页数:14
相关论文
共 49 条
  • [1] Magnetic signature of the ionospheric disturbance dynamo at equatorial latitudes:: "Ddyn" -: art. no. A10301
    Le Huy, M
    Amory-Mazaudier, C
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2005, 110 (A10)
  • [2] Magnetic Signatures of Ionospheric Disturbance Dynamo for CME and HSSWs Generated Storms
    Younas, Waqar
    Amory-Mazaudier, C.
    Khan, Majid
    Le Huy, M.
    [J]. SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS, 2021, 19 (09):
  • [3] Planetary magnetic signature of the storm wind disturbance dynamo currents:: Ddyn
    Le Huy, Minh
    Amory-Mazaudier, Christine
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2008, 113 (A2)
  • [4] PARTIAL CRITICISMS OF DYNAMO THEORY OF MAGNETIC DISTURBANCE
    COLE, KD
    [J]. JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1962, 24 (JUN): : 541 - &
  • [5] MORPHOLOGY OF IONOSPHERIC DISTURBANCE ASSOCIATED WITH MAGNETIC ACTIVITY
    MARTYN, DF
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1950, 55 (02): : 195 - 195
  • [6] An ionospheric conductance model based on ground magnetic disturbance data
    Ahn, BH
    Richmond, AD
    Kamide, Y
    Kroehl, HW
    Emery, BA
    de la Beaujardiere, O
    Akasofu, SI
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1998, 103 (A7): : 14769 - 14780
  • [7] SIGNATURE OF SUBSTORM MAGNETIC DISTURBANCE CO-ROTATING WITH EARTH
    SUZUKI, A
    KIM, JS
    SUGIURA, M
    [J]. TRANSACTIONS-AMERICAN GEOPHYSICAL UNION, 1978, 59 (12): : 1167 - 1167
  • [8] Magnetic storm associated disturbance dynamo effects in the low and equatorial latitude ionosphere
    Abdu, M. A.
    de Souza, J. R.
    Sobral, J. H. A.
    Batista, I. S.
    [J]. RECURRENT MAGNETIC STORMS: COROTATING SOLAR WIND STREAMS, 2006, 167 : 283 - +
  • [9] The effect of ionospheric inhomogeneity on magnetic pulsation polarization: magnetic disturbance on the ground as a function of inhomogeneity magnitude
    Belova, E
    Pchelkina, E
    Lyatsky, W
    Pashin, A
    [J]. JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 1997, 59 (15) : 1945 - 1952
  • [10] NEUTRAL AND ION COMPOSITION DISTURBANCE IN F2 IONOSPHERIC REGION DURING MAGNETIC STORM
    ROMANOVSKII, YA
    [J]. TRANSACTIONS-AMERICAN GEOPHYSICAL UNION, 1977, 58 (08): : 755 - 755