共查询到20条相似文献，搜索用时 26 毫秒
1.
The empirical model of variations in the atomic oxygen emission intensity depending on different heliogeophysical conditions such as nighttime, lunar time, lunar phase age, season, year, and solar activity level during the 11-year cycle, as well as on cyclic aperiodic activity variations, level of geomagnetic disturbances, and their manifestations in the form of midlatitude subauroral red arcs, has been developed based on the long-term measurements of this emission intensity. 相似文献
2.
The data on regular variations in the emission intensity of the molecular oxygen Atmospheric system excited in the region of the lower thermosphere have been systematized based on the long-term studies. The empirical approximations of the emission behavior are presented. 相似文献
3.
The Bronze ceramics of the Baeza archeological monument in Spain is studied by archaeomagnetic methods. In the 19th and 18th centuries B.C, the intensity of the geomagnetic field varied from 40 to 60 mkT. The variations are smooth; they attained their maximum in the 16th to 15th centuries B.C. The obtained data on the variations in the geomagnetic intensity perfectly agree with the results of previous investigations for the ceramics from the Bronze Age multilayered archeological monuments Azuer and Ubeda. The temperature in the region of the Baeza monument is estimated in the interval from the 18th to the 13th centuries B.C. It experiences wave-like variation, ranging from ??15 to 23°C and attains its maximum in the 16th century B.C. 相似文献
4.
The empirical model of variations in the emitting layer height and parameters has been developed based on an analysis of the rocket measurements of the vertical distributions in the 630 nm intensity. The dependences on the solar zenith angle during a day are most substantial. This dependence is responsible for the character of seasonal variations at different latitudes. The height of the emitting layer increases with increasing solar activity, reflecting a temperature rise in the upper atmosphere. The negative trend—0.35 km yr?1 in the interval 1964–1990—has been revealed. 相似文献
5.
The ground-based and satellite measurements of the upper-atmosphere continuum (continuous emission) intensity in the visible and near IR spectral regions have been analyzed. The data were obtained at the geophysical stations, located in different regions of the globe, and at Mir Space Station. The regularities in the spectral distribution of the continuum emission intensity and emission variations have been revealed for different heliogeophysical conditions. 相似文献
6.
Based on the measurements of the ortho helium 1083 nm emission intensity during twilights and on the calculation of its variations depending on the solar zenith angle, the method for determining the atmospheric temperature at heights of 300–1000 km during the nighttime period of day has been developed, taking into account the diurnal and seasonal conditions. 相似文献
7.
I. E. Nachasova K. S. Burakov A. J. Lorrio 《Izvestiya Physics of the Solid Earth》2007,43(10):830-835
Data on the geomagnetic field intensity in the first millennium BC and the 8th–10th centuries AD are obtained from the study of materials from the El Molon archaeological monument (Spain). A 75-yr averaged curve of the variation in the geomagnetic field intensity in the area of the zero meridian over the last three millennia is constructed from a set of new and previously obtained data on the geomagnetic intensity variations in Spain and France. The field intensity smoothly decreases in the time interval studied, and variations a few centuries long are superimposed on this trend. Unlike the present-day relationship, the average level of the geomagnetic field intensity in Spain in the first millennium BC was higher than in the Caucasus. 相似文献
8.
Galactic cosmic rays-clouds effect and bifurcation model of the Earth global climate. Part 1. Theory
Vitaliy D. Rusov Alexandr V. Glushkov Vladimir N. Vaschenko Оksana T. Myhalus Yuriy A. Bondartchuk Vladimir P. Smolyar Elena P. Linnik Strachimir Cht. Mavrodiev Boyko I. Vachev 《Journal of Atmospheric and Solar》2010,72(5-6):398-408
9.
Rotational temperatures of the 1.58-μm (0–1) band of the Infrared Atmospheric system of molecular oxygen (IRAO2), measured in Zvenigorod (56° N, 36° E), are systematized and analyzed. An empirical dependence of variations in the temperature of the 1.58-μm emission on the solar zenith angle is derived. The use of parameters of the altitude distribution of emission intensity 1.27 μm of middle atmosphere temperature profiles, received from the AURA satellite, allowed for the study of daily variations in the temperature of the 1.58-μm emission. It is revealed that the behavior of these variations corresponds to daily variations in the atmospheric temperature at altitudes of the radiating layer of IRAO2, received from the AURA satellite. 相似文献
10.
Results from joint work between the Geophysical Institute (Sofia, Bulgaria), and the Geomagnetic Institute (Grocka, Yugoslavia) on the geomagnetic field variation in the prehistoric past are presented. Preliminary curves of variation of the three geomagnetic elements: declination, inclination and intensity are presented. The movement of the virtual pole position for the 6500 years time period B.C. is derived. The curves and the virtual pole positions provide a dating tool for archaeological purposes and determination of the periodicities in the geomagnetic secular variations in southeastern Europe. 相似文献
11.
I. E. Nachasova K. S. Burakov F. Molina J. A. Cámara 《Izvestiya Physics of the Solid Earth》2007,43(2):170-176
The geomagnetic intensity variation from the middle of the 4th millennium BC to the beginning of the 2nd millennium BC is reconstructed from the archaeomagnetic study of ceramic material taken from 24 layers of the Los Castillejos monument (Montefrio, Spain). The general patterns of the geomagnetic intensity variation reconstructed by studying materials from the Cendres Cave and Los Castillejos monuments (Spain) are similar. The intensity level is revised in the time interval including the minimum of the “fundamental” oscillation of the geomagnetic field; the characteristics of geomagnetic intensity variations whose superposition can provide the intensity variation observed in the study time interval are determined. Constraints on the climate humidity variation over the settlement lifetime are obtained from heating-induced variations in the magnetic susceptibility of the ceramics. 相似文献
12.
G. A. Nasyrov 《Geomagnetism and Aeronomy》2009,49(4):528-531
The spatial variations in the emission intensity, related to internal gravity waves (IGWs) generated in the troposphere when the air flows around the Kopet Dagh mountain range, and the regularities of these variations have been detected for the first time based on the photometric measurements of the spatial distribution of the atomic oxygen 630 nm emission intensity, performed in 1967 at Vannovskii station of the Physicotechnical Institute, Academy of Sciences of the Turkmen SSR. 相似文献
13.
Changes in total geomagnetic field intensity, of 2–3 nT, were observed prior to the 1995 Hyogo-ken Nanbu (Kobe) earthquake at the Amagase (AMG) site, located approximately 70 km from the epicenter. We examined whether the observed variations are local signals arising from the Earth's crust, or global variations that are unlikely to originate from the crust. To remove global-scale variations in total geomagnetic intensity data, we employed a regional geomagnetic field model. Using data recorded at five reference sites in Japan, we estimated global-scale variations in total geomagnetic intensity, and removed them from the observed total geomagnetic intensity at the AMG site. The reminder still showed variations during the period prior to the Kobe earthquake. In addition, these pre-seismic variations include two of the largest shifts recorded during the entire observation period at the AMG site, raising the possibility that these variations were indeed related to the earthquake. These variations cannot be interpreted as signals arising from the area close to the seismic source because of the large distance between the epicenter and the site. Therefore, our results raise the possibility that the physical state of the Earth's crust shows marked changes over a wide region in the lead-up to a seismic event. 相似文献
14.
Based on the measurements of 656.3-nm emission of atomic hydrogen, we constructed a model of variations in its intensity,
which describes the dependence of diurnal, lunar, seasonal, latitudinal, and long-term variations, during the 11-year cycle
of solar activity, cyclic aperiodic variations, and variations after geomagnetic disturbances. 相似文献
15.
O. I. Akhmetov 《Geomagnetism and Aeronomy》2009,49(5):664-669
The seasonal effect of the daily variations in the cosmic ray intensity on the conductivity of the Earth-high-conductivity layer column has been analyzed based on the observations of the cosmic ray intensity, atmospheric current, and electric field vertical component, performed from summer 2006 to spring 2007 at Apatity station. The method for correcting the measurements of the atmospheric current and electric field vertical component under complex tropospheric conditions by numerically simulating the spatial structure of the current and field lines in the observation region has been proposed. It has been indicated that cosmic rays are the main source of ions in the winter polar lower atmosphere and are responsible for the type of daily variations in the conductivity, whereas the daily variations in the atmospheric current more depends on the conductivity rather than on the vertical electric field. 相似文献
16.
为将雷达技术应用于地震预测,在实验室对花岗岩等不同岩性的27个岩石试样进行了加压实验观测研究,使用的雷达测量仪器是美国HP公司生产的专用RSC测量系统,观测8mm,2cm,3cm和5cm四个雷达波段,在加压的过程中自动连续测量岩石试样的雷达波反射强度随压力的变化,实验表明：反映岩石试样微波反射特性的雷达波反射强度随压力变化而变化,在实验的27个岩石试样中,无一例外,只是在不同试样、不同波段或不同极化方式的实验中存在变化幅度和趋势的差异. 岩石试样反射波强度的相对变化量为百分之几到百分之十几,花岗岩的最大变化量达到202%(113号试样),砂岩的最大变化量达到279%(212号试样). 实验结果为将雷达技术应用于地震预测、岩体及岩土工程稳定性监测和稳定性评价提出了实验依据,奠定了物理基础. 相似文献
17.
On the basis of the data of ground-based spectrometric observations in Zvenigorod (55.7°N, 36.8°E) and published results of measurements of the intensity of the Infrared Atmospheric system of molecular oxygen obtained at other stations, empirical relations describing variations in the intensity of the 1.58-μm emission for various solar and geophysical conditions are calculated. 相似文献
18.
A. I. Semenov N. N. Shefov I. V. Medvedeva A. B. Beletsky 《Geomagnetism and Aeronomy》2012,52(2):248-253
On the basis of correlations between seasonal variations in the intensity and temperature of 557.7-nm emission, the mean monthly
longitudinal variations in temperature are drawn. A comparison is performed with the data of interferometer and lidar measurements
of temperature performed at various stations, as well as with the results of satellite studies. The dependences of the amplitudes
of seasonal variations in temperature on latitude are obtained. 相似文献
19.
T. Sergienko I. Kornilov E. Belova T. Turunen J. Manninen 《Journal of Atmospheric and Solar》1997,59(18):2401-2407
Ionospheric heating experiments were done by the EISCAT Heater in Tromsø on 15–19 November, 1993. A low-light TV camera was installed at the VLF receiving station at Porojärvi about 100 km to the south-east of Tromsø. The spectral analysis of the auroral luminosity variations showed that the brightness of the aurora varied at the modulation frequency of the heating wave. The results of this analysis and the numerical simulations of the auroral luminosity variations caused by the HF heating are shown. The variations of the optical emission intensity at the heating frequency occur during the auroral ionosphere modification. The observed intensity variation of the auroral green line during the interval of enhanced electron temperature is explained by a decreasing rate of the O2+ ion dissociative recombination when the electron temperature increases. The brightness variation depends on the characteristic energy and the intensity of the auroral electron flux and the heating wave parameters. The artificial luminosity pulsations caused by HF heating are estimated. 相似文献
20.
J. PHILIP O'KANE 《水文科学杂志》2013,58(2):147-150
ABSTRACT The snowmelt runoff process from small basins is discussed. A differentiation is made between overland flow in the snowpack and groundwater flow induced by infiltrating meltwater. The effect of variations of the snowmelt intensity on streamflow is studied. It is shown that the runoff is high from the first day of snowmelt runoff if the streamflow is caused by overland flow, and that there are pronounced peaks every day, which almost correspond with the snowmelt intensity during daytime. Streamflow originating from groundwater, on the other hand, increases continuously during the snowmelt and shows only small daily peaks in the flow. Simultaneous overland and groundwater flow are also discussed. Observed runoff hydrographs from small basins are analysed in some detail. For the open fields studied the runoff shows the typical character of overland flow. For a rather large forested area the surface runoff also constitutes an important part of the runoff, but the groundwater baseflow is considerable. 相似文献