共查询到20条相似文献，搜索用时 15 毫秒
1.
Jaroslav Střeštík Karel Prikner Karel Dobeš Reviewer M. Hvoždara 《Studia Geophysica et Geodaetica》1973,17(1):27-35
Summary The spectra of nearly 100 samples of Bpc3 pulsations were computed in the X and Y components of data from the Budkov Observatory. These spectra were used to study the daily variations of the fundamental characteristics of the pulsations, the frequency f
0
and amplitude A
0
of the main spectral peaks. The daily variation of the ellipticity of the polarization ellipses of oscillations in frequency f
0
was also studied in the XY-plane.Part of these results was reported at the XVth General Assembly of the IUGG, Moscow, August 1971. 相似文献
2.
Summary The method of two-component spectral analysis is described in two versions: as the so-called static analysis, in which the pulsation sample being studied is treated as a whole, and as the dynamic analysis, in which the given sample is processed piecewise in order to determine the time variations of various parameters. Both versions were applied to geomagnetic pi2 pulsations. The pi2 oscillations are resolved into several frequency components. The properties of these components are studied in dependence on the frequency and local time. The time variation of the amplitude (attenuation) and the polarization characteristics (precession) of pi2's are also studied. 相似文献
3.
Summary The dependence of the individual parameters of geomagnetic Pc3 pulsations, of their frequencies, amplitudes, phases, flattening of their polarization ellipses, the orientation of their major axis and the sense of rotation of the disturbance vector, are determined from the records made at the Budkov and Niemegk Observatories. Also their diurnal variations at both stations and the correlation of the numerical values between both stations are given. 相似文献
4.
Jaroslav Střeštík Karel Prikner Reviewer M. Hooždara 《Studia Geophysica et Geodaetica》1977,21(2):159-167
Summary The numerical method of Fourier's spectral analysis is used to treat 29 pairs of samples of pc3 pulsations recorded at the observatories of Budkov (Czechoslovakia) and Belsk (Poland). The amplitude, frequency and phase characteristics of their spectra are compared. The polarization characteristics of the spectral frequency components of pulsations recorded at both observatories are compared in a quasi-stationary approximation of a plane oscillation. 相似文献
5.
A.K. Agarwal B.P. Singh N. Nityananda 《Physics of the Earth and Planetary Interiors》1979,18(3):232-237
Variations recorded simultaneously at eight Indian stations during a magnetic storm are analysed to obtain the power spectra for each component using the fast Fourier transform. For two selected peaks, observed for H at all stations, at 49.5- and 70-min periods, a complex demodulation is performed for each component. From the variations thus obtained, horizontal polarization ellipses are drawn for four events of 49.5-min period. The variation of the demodulates and polarization ellipses at the stations shows a regional character which coincides with the physiographic grouping of the stations. Anomalously large Z variations are observed at the equatorial stations, which are near the sea. A distinct feature is the suppression of H at Trivandrum where the polarization ellipses confirm the E-W trend of the induced currents in this region. The overall similarity of the horizontal variations is demonstrated by these ellipses. Horizontal disturbance vectors at Annamalainagar, Trivandrum and Sabhawala confirm channelled currents located previously. At Shillong, the induced effects are evident and the currents are deduced to flow eastward, directly beneath the station.The overall regional similarities in variations are clearly manifested. 相似文献
6.
Karel Dobeš Karel Prikner Jaroslav Střeštík Reviewer M. Hvoždara 《Studia Geophysica et Geodaetica》1973,17(3):240-244
Summary A new method is presented of computer processing of amplitude-time records. The method is based on a two-component spectral analysis, suitable for investigating a planar stationary oscillatory event. The method is applied to the study of the fine structure of short-period geomagnetic pulsations. Apart from a semi-quantitative representation of the directional distribution of the pulsation event in the plane of oscillation, the proposed method enables one to obtain quantitative information on the frequency components, representing the pulsation — the distribution of the overall energy in the spectrum of the pulsation, the ellipticity of the polarization ellipses, the orientation of the major axes of the ellipses, and the sense of rotation of the disturbance vector. 相似文献
7.
《Journal of Atmospheric and Solar》2003,65(10):1161-1167
The ultra-low-frequency (ULF) geomagnetic pulsations observed at two nearly conjugate mid-latitude sites are examined to study their spatial structure and polarization, and learn about the role of ionospheric conductivity in forming their ground signatures. The data of 1999–2002 from Antarctica and New England (L of 2.4) are compared with the numerical results obtained in a simple plane model of ULF wave propagation through the ionosphere and atmosphere. The multi-layered model environment includes an anisotropic and parametrically time-dependent ionosphere, a uniform magnetosphere and a conducting Earth, all placed in a tilted geomagnetic field. The measured diurnal and seasonal variations in the orientation angle of the polarization ellipse are interpreted as effects of hydromagnetic wave propagation through the ionosphere and conversion to an electromagnetic field below. Essentially, the phase, amplitude and polarization of ULF waves observed at the ground are controlled by the wave's spatial structure in the magnetosphere and ionospheric transverse conductivities. The differences shown by the characteristics of simultaneous pulsations in conjugate areas arise mainly from different local ionospheric conditions, while the source waves of the pulsations are common to both sites. 相似文献
8.
Summary Wave diagnostics of several alternatives of a constructed model of the daytime and night ionosphere of the mid geomagnetic latitudes were carried out in the ULF range of electromagnetic waves. The altitude profiles of local wave parameters of the ionosphere, the wavelengths and wave attenuation, were analysed at a fixed frequency. The frequency dependence of the amplitude and polarization characteristics of the total wave at the Earth's surface were also analysed in dependence on the frequency-amplitude spectrum of geomagnetic pulsations. The effect of the low regions of the ionosphere (h<100 km) was tested on the damping of the propagating wave and on the frequency-amplitude and polarization characteristics of the wave at the Earth's surface. 相似文献
9.
《Journal of Atmospheric and Solar》2007,69(14):1747-1752
This paper is devoted to the morphology of Pc1 geomagnetic pulsations (frequency range 0.2–5.0 Hz). This study is based on the series of continuous observations of Pc1 pulsations during more than three solar cycles (July 1957–December 1995). The main attention is given to the temporal characteristics of Pc1 activity, i.e. daily, seasonal and cyclic variations, and also the relationship of Pc1 activity with magnetic storms, sector structure of the interplanetary magnetic field and parameters of the solar wind. The results may be used in the studies of medicobiologic aspects of the problem of solar–terrestrial relations. 相似文献
10.
S. Lepidi P. Francia U. Villante A. Meloni A. J. Lazarus R. P. Lepping 《Annales Geophysicae》1999,17(10):1245-1250
An analysis of the low frequency geomagnetic field fluctuations at an Antarctic (Terra Nova Bay) and a low latitude (L’Aquila, Italy) station during the Earth’s passage of a coronal ejecta on April 11, 1997 shows that major solar wind pressure variations were followed at both stations by a high fluctuation level. During northward interplanetary magnetic field conditions and when Terra Nova Bay is close to the local geomagnetic noon, coherent fluctuations, at the same frequency (3.6 mHz) and with polarization characteristics indicating an antisunward propagation, were observed simultaneously at the two stations. An analysis of simultaneous measurements from geosynchronous satellites shows evidence for pulsations at approximately the same frequencies also in the magnetospheric field. The observed waves might then be interpreted as oscillation modes, triggered by an external stimulation, extending to a major portion of the Earth’s magnetosphere. 相似文献
11.
A local approximation method based on piecewise sinusoidal models has been proposed in order to study the frequency and amplitude characteristics of geomagnetic pulsations registered at a network of magnetic observatories. It has been established that synchronous variations in the geomagnetic pulsation frequency in the specified frequency band can be studied with the use of calculations performed according to this method. The method was used to analyze the spectral–time structure of Pc3 geomagnetic pulsations registered at the network of equatorial observatories. Local approximation variants have been formed for single-channel and multichannel cases of estimating the geomagnetic pulsation frequency and amplitude, which made it possible to decrease estimation errors via filtering with moving weighted averaging. 相似文献
12.
Experiments on the generation of artificial electromagnetic pulsations constitute an important part of investigations of the
magnetosphere-ionosphere system with the use of an active action. The investigation of the generation of magnetic pulsations
in the Pc1 frequency range has shown that the response of the ionosphere to heating is detected only in a few experiments.
Although the primary perturbed parameter is the electron temperature, the efficiency of the generation of pulsations is determined
by the perturbations of the ionospheric conductivity. The magnitude of these hertz perturbations depends complexly on the
electron density profile and the parameters of a pump wave. The numerical experiment demonstrates the determining effect of
the electron density in the D region on the magnitude of perturbations of the ionospheric conductivity. Under conditions of a low electron density, it
is impossible to create a large perturbation of the conductivity in the Pc1 frequency range, although perturbations of the
electron temperature can be large in this case. In view of a large number of electrons at altitudes of 70–90 km, which absorb
a considerable fraction of the energy of a high-frequency wave, the electron temperature in the E region of the ionosphere cannot be sharply increased, but the amplitude of the variations of the ionospheric conductivity
in this case is larger than that for the profiles with a low electron density. In the presence of the developed D region, the efficiency of the modification of the conductivity in the indicated frequency range can be increased by choosing
the optimal frequency and polarization of the pump wave. A low efficiency of the experiments on the generation of artificial
magnetic pulsations in the Pc1 frequency range is apparently explained by the fact that they were performed in winter in the
absence of a well-developed D region of the ionosphere. 相似文献
13.
14.
O. M. Chugunova V. A. Pilipenko S. L. Shalimov M. Engebretson 《Geomagnetism and Aeronomy》2008,48(3):307-313
The variations in the daily average energy of geomagnetic pulsations and noise in the Pc3 (20–60 mHz) and Pc4 (10–19 mHz) frequency bands in the polar cap have been studied based on the data from P5 Antarctic station (corrected geomagnetic latitude ?87°) from November 1998 to November 1999. The daily average pulsation energy has been calculated using the method for detecting the wave packets, the spectral amplitude of which is higher than the threshold level, from the dynamic spectrum. A spectral analysis of the energy of pulsations and noise in the Pc3 and Pc4 bands, performed using the maximal entropy method, has revealed periodicities of 18 days in the local winter and 26, 13, and 7–9 days during the local summer. The simultaneous and coherent variations with periods of 26, 13, and 7–9 days in the solar wind velocity and IMF orientation indicate that the variations in the Pc3–4 wave energy in the polar cap at a sunlit ionosphere are mainly controlled by the parameters of the interplanetary medium. The variations in the Pc3–4 wave energy with a period of 18 days are observed only during the local winter and are supposedly related to the variations in the ionospheric conductivity modulated by planetary waves. 相似文献
15.
本文分析了1988年12月和1989年1月在长春、北京、兰州3个台站上观测的地磁脉动资料,研究了3个台站同时记录到的Pi2地磁脉动的频谱特征和偏振特性,进而对低纬Pi2地磁脉动的产生和传播机制做了理论研究. 相似文献
16.
本文对2008—2010年隆尧地磁台站的地磁水平分量H和磁偏角D的秒数据进行了短时快速傅里叶变换,按连续型地磁脉动Pc2—Pc6所对应的频率范围对频谱进行了频段划分,在此基础上研究了各频段频谱总幅值即短周期地磁扰动的时空分布特征.在时间变化上,同一年中不同频段的幅值具有相似的变化规律,每年的幅变特性与该年对应的Vr指数的时间分布也具有一致的变化形态,仅仅在变化的幅度上存在差异.磁偏角D的幅值和VrD均呈现出显著的季节变化特征,而水平分量H的幅值和VrH却不显著.在空间变化上,各频段幅值均随地磁纬度的增加而增大,随地方时变化呈现出双峰双谷的特征. 相似文献
17.
A series of experiments on modification of the ionosphere by a powerful ground HF transmitter was performed using the EISCAT
heating facility in order to generate artificial magnetic pulsations in the frequency range 0.1–3 Hz. In several cases, the
ionospheric electric field and the electron density vertical profile were measured with the EISCAT incoherent scatter radar.
The measurement of the background values of the ionospheric parameters made it possible to verify the numerical model for
generating artificial emissions. The calculated amplitudes of magnetic pulsations correspond to the values measured on the
Earth’s surface. However, the model cannot explain the sporadic nature of artificial signals, which indicates that this model
is incomplete. Disturbances of the neutral particle density in the upper atmosphere are one of the possible causes explaining
a difference between the calculations and the experimental values. The numerical simulation indicated that the amplitude variations
caused by such disturbances can be 20%. For artificial emissions whose intensity is comparable with the intensity of artificial
noise, variations in the neutral components can result in the disappearance of an artificial signal on the spectrogram. 相似文献
18.
The diurnal variations in the amplitude and parameters of polarization ellipses of the first Schumann resonance according
to three magnetic field components, observed on December 1–10, 2007, at the Barentsburg and Lovozero observatories, have been
studied. Ellipses have been constructed in the (H, D) and (H, Z) planes. The value of the minor axis, inclination of the major axis, ellipticity, and the rotation direction have been estimated.
The vertical magnetic component of the Schumann resonance is three to four times as small as the horizontal component. The
difference in the diurnal variations in the ellipse parameters between both observatories has been found. The effect can be
caused by a difference in the Earth’s conductivity in the vicinity of the observatories and by conductivity anisotropy. The
major axis inclination and ellipticity have semidiurnal components. The polarization vector mostly rotates from D to H in the horizontal plane and from Z to H in the vertical plane at both stations. 相似文献
19.
Spatial-temporal and spectral features of ground geomagnetic pulsations in the frequency range of 1–5 mHz at the initial phase of a strong magnetic storm of the 24th cycle of solar activity (August 5–6, 2011, with a Dst-variation in the storm maximum of ?110 nT) are analyzed. Large opposite in sign amplitudes of variations in IMF parameters (from ?20 to +20 nT) at a high velocity of the solar wind (～650 km/s) accompanied by intense bursts in solar-wind density (up to ～50 cm?3) were distinctive feature of interplanetary medium conditions causing the storm. Geomagnetic Pi3 pulsations global in longitude and latitude and in-phase in the middle and equatorial latitudes were found. The onset of pulsation generation was caused by a pulse of dynamic pressure of the solar wind (～20 nPa), i.e., by a considerable compression of the magnetosphere. The maximum (2–3 mHz) in the amplitude spectrum of near-equatorial pulsations coincided with the maximum of pulsations in the daytime polar cap. After the next jump of the dynamic pressure of the solar wind (～35 nPa), an additional maximum appeared in the pulsation spectrum in the frequency band of ～3.5–4.5 mHz. Global pulsations suddenly stopped after a sharp decrease in the solar-wind dynamic pressure and corresponding extension of the magnetosphere. The obtained results are compared with the time dynamics of the position and shape of the plasmapause. 相似文献
20.
The set of experiments in 2017 included the forecasting of geo- and heliophysical conditions in the ionosphere, the choice of heating regimes at a minimum critical frequency of the F2 ionospheric layer, analysis of the ionosphere radio sounding results and measurements of geomagnetic perturbations using ground-based facilities, study of the potential for higher efficiency and probability of artificial effects on the ionosphere, and the establishment of a correlation between geomagnetic field variations and the radio heating facility cyclogram. The experiments were carried out with a combination of new heating conditions (pulse ratio, period of action, two-frequency and continuous heating, variations in radiated power, polarization, shortwave radiation direction, etc.) in the intervals between recurrent magnetic storms. Geomagnetic field pulsations (in accordance with the cyclogram) and substorm effects were stimulated by the SURA facility against a background of quiet geophysical conditions. 相似文献