Mediciones Geomagneticas en la region de la Peninsula Antartica,Islas adyacentes y Mar de Weddell en 1951–56

Resumen Se exponen los resultados de cuatro campañas geomagnéticas llevadas a cabo entre 1951 y 1956 en la mencionada región del Antártico señalando el éxito obtenido mediante el uso del equipo instrumental compuesto por bien contrastados magnetómetros de QHM y BMZ en lugares de difícil acceso y condiciones severas. El campo medido se presenta con la existencia de muchas anomalías, a veces bastante fuertes, que se observan generalmente en las componentes de la intensidad. Es además notable el hecho de que los datos medidos directamente en la parte meridional extrema del Mar de Weddell, difieren de los que dan las cartas magnéticas mundiales extrapolados o calculados parcialmente en base a la teoría del potencial. Se confirma el rápido cambio secular en las intensidades, especialmente en la componente vertical, siendo en vez lento el cambio en la declinación. La situación de los puntos de observación y los resultados numéricos se dan en un mapa y una tabla de valores respectivamente.

---

Summary This report covers four geomagnetic campaigns in the region of the Antarctic Peninsula, the adjacent islands and the Weddell Sea during the summer seasons of the years 1951 to 1956. The instrumental equipment was slightly modified to meet antarctic conditions in general, specially for transport to stations distant from the bases. In most antarctic points observations were made with both magnetometers QHM and BMZ which were compared at observatory and base stations by means of theodolite and earth inductor. The field measurements show the presence of many anomalies, some of which quite strong. The values observed in the southernmost area of the Weddell Sea differ appreciably from the figures given on world magnetic charts, which for some regions seem to be based on extrapolation or potencial computations. The secular change in declination is small but those in intensities are rapid, especially in the vertical component, confirming some previous indications. The results are tabulated and the position of the observation stations is shown on a map.

---

---

Contribution del Instituto Antártico Argentino N 3.     

Relaciones entre operaciones diferenciales del Cálculo vectorial y paréntesis de Lagrange,con aplicatión a la Hidrodinámica

Resumen Como aplicación hidrodinámica de un problema más general, tratado al principio, demostraremos el siguiente teorema:El rotacional del campo de la variación unitaria del torbellino de las partículas que se mueven rotacionalmente en líquidos ideales y homogéneos puede representarse por medio de paréntesis deLagrange.

---

Zusammenfassung Als hydrodynamische Anwendung eines eingangs behandelten allgemeineren Problems wird folgender Satz bewiesen:Der Rotor des Feldes der individuellen Ableitung des Wirbelvektors der sich drehend bewegenden Partikel idealer und homogener inkompressibler Flüssigkeiten läßt sich mittels der Klammersymbole vonLagrange darstellen.

     

Lateral variations of the local magnitude at Ebre station,Northeastern Iberian Peninsula

Since 1984, a seismic surveillance at the Baix Ebre Region (NE of the Iberian Peninsula) has been carried out from a seismic network consisting of two digital and one analog stations. Large discrepancies between the recorded amplitudes and the magnitude estimates given by different agencies have been observed. To explain these discrepancies, that consist of a large reduction of amplitude and a strong dependence of the azimuth, a local magnitude formula for the area has been computed, using the analog records obtained at EBR short-period station. Global results show an average station correction factor between the computed local magnitude and the reported magnitude of the order of 1, presenting large variations around the mean value with a clear dependence on the azimuth. A detailed analysis of this variation around the mean value reveals that earthquakes can be classified according to their location in different geological units, thus obtaining for each zone a distinct station correction factor that can fluctuate as much as 0.6 around the average. These large lateral variations of the magnitude are in good agreement with previous studies of coda-Q attenuation.     

Variación secular geomagnética en Sudamérica y alrededores con relación a todo el Hemisferio Sur

Resumen Se aplica el análisis de energía de espectro a los datos de la variación secular geomagnética para tres observatorios del Hemisferio Sur: Pilar, Amberley, Mauritius. Las figuras 2–10 indican generalmente tres tipos de picos: a) de periodos de menos de 10 años; b) del periodo aproximado de la actividad solar de 10–11 años; c) de una fluctuación de 40–60 años. Los coeficientes de la expansión esférico-armónica de la variación secular muestran también una fluctuación del último tipo.

---

Summary The power spectrum analysis is applied to geomagnetic secular variation data of three southern magnetic observatories: Pilar, Amberley, Mauritius. The figures 2–10 indicate in general three types of peaks: a) of periods less than 10 years; b) of approximately solar activity cycle; c) of 40–60 years fluctuation. Also the coefficients of spherical harmonic expansion of SV show the last type fluctuation.

     

Strahlungsmessungen mit dem Bellani-Kugelpyranometer in El Salvador (Mittelamerika)

Zusammenfassung Der Jahresverlauf der Zirkumglobalstrahlung in El Salvador wird in seiner Abhängigkeit vom Jahresgang der Sonnenhöhe, den Bewölkungs- und Trübungsverhältnissen diskutiert. Der Zusammenhang zwischen dem Strahlungsgenuss einer Kugel und einer horizontalen Fläche wird im Hinblick auf die jahreszeitlich wechselnde Sonnenhöhe untersucht; es zeigt sich, dass die Globalstrahlung mit befriedigender Genauigkeit aus Messungen der Zirkumglobalstrahlung zu bestimmen ist. Die Beziehung zwischen Zirkumglobalstrahlung und Sonnenscheindauer bzw. Bewölkungsverhältnissen wechselt jahreszeitlich, entsprechend den mittleren Sonnenhöhen, und gestattet, lückenhafte Messreihen der Zirkumglobalstrahlung nach Registrierungen der Sonnenscheindauer zu reduzieren.

---

Summary The annual variation of circumglobal radiation in El Salvador, depending on the seasonal change of solar height, cloudiness and turbidity, is discussed. The relation between the radiation received on a sphere and a horizontal surface on the other hand, is examined with respect to seasonal change of solar height; global radiation is to be determined from measurements of circumglobal radiation with satisfactory accuracy. The relation between circumglobal radiation and sunshine duration or cloud conditions, changes throughout the year, according to mean solar height; uncomplete series of circumglobal radiation can be reduced after records of the duration of sunshine.

---

Resumen El transcurso anual de la radiación circumglobal en El Salvador es discutido con referencia a la variación anual de la altura del Sol, la nubosidada y la turbiedad. La relación entre la cantidad de radiación recibida por una esfera y una superficie horizontal, por otra parte, es investigada con respecto al cambio estacional de la altura del sol; resulta que la radiación global es a determiner con satisfactoria exactitud. a base de mediciones de la radiación circunglobal. La relación entre radiación circunglobal y duración del brillo solar o nubosidad, respectivamente, varía segun la estación del año, correspondientemente a la altura media del sol; series cortos o incompletos de la radiación circunglobal pueden ser reducidas segun registros de la duración de la luz solar.

     

The mean density of the earth

Résumé La densité moyenne de la Terre et la densité moyenne de la couche superficielle, jusqu'à1450 m, furent déterminées `a partir des observations du gradient vertical de la pesanteur, dans la mine Anna à Píbram. Les calculs furent effectués selon les formules(6) et(7), déduites sous la supposition que la Terre soit un ellipsoïde de révolution. Les résultats furent comparés aux valeurs déduites pour l'ellipsoïde astronomique et aux valeurs des densités obtenues des prises de roches dans la mine et on a constaté un bon accord.     

Local magnitude,surface wave magnitude and seismic energy

Summary The local magnitude M_L at the seismological station Pruhonice (PRU) was converted into surface wave magnitude M_S using the formula M_S=–3.2+1.45 M_L and the seismic wave energy was estimated using the relation log E (Joule)=1.2+2.0 M_L. It was proposed to apply the same conversion formulae at seismological stations Kaperské Hory (KHC) and Berggiesshübel (BRG) where the calibrating functions for local magnitudes were determined for the same set of earthquakes with common reference magnitudes as in the case of the PRU station.     

Earthquakes in the Czech Republic and Surrounding Regions in 1995–1999

In the time span from January 1995 to December 1999 the Czech National Seismological Network (CNSN), consisting of ten permanent digital broadband stations, several local networks and two data centers, detected and recorded 9530 regional natural seismic events, 27 greater than magnitude 2. Most of these events were located by the Czech Seismological Service (CSS), and the most prominent of them were analyzed in detail. A large number of quarry blasts were recorded as well but were not included in the analysis. We provide basic information on the configuration of the CNSN and on the way of routine data processing employed by the CSS in this paper. The over-all regional seismicity monitored by the CNSN in 1995–1999 is briefly reviewed. The main results of observations and evaluation of the local (NW-Bohemia/Vogtland, South Bohemia, Sudeten) and induced (Kladno, Píbram, Upper Silesia, Lubin/Poland) seismic activity within this period are presented in a condensed form. Finally, a summary on macroseismic observations on the territory of the Czech Republic in 1995–1999 is also presented.     

Der Tagesgang von Temperatur und Luftfeuchtigkeit in San Salvador

Zusammenfassung Der Tagesgang von Temperatur und Luftfeuchtigkeit in San Salvador zeigt deutliche jahreszeitliche Verschiedenheiten, die wesentlich durch Strahlungsgenuss, Sonnenauf- und Untergangszeiten und ein tageszeitliches mittelräumiges Windsystem bestimmt ist.

---

Summary The daily variation of air temperature and humidity shows clear seasonal differences, which are essentially determined by incoming radiation, sunrise and sunset and a diurnal meso-scale wind system.

---

Resumen El transcurso diurno de la temperatura y de la humedad del ambiente en San Salvador demuestra netamente diferencias segun la estación del año, las cuales se deben a las condiciones de radiación, salida y puesta del sol y un sistema diurno de viento.

     

Calibration of Local Magnitude M<Subscript>L</Subscript> in the Azores Archipelago Based on Recent Digital Recordings

—The development of the digital seismic network in the Azores Archipelago during recent years made it possible to obtain the amplitudes (waveform) of recorded motion in a large set of stations. With this new data, maximum amplitudes of the Wood Anderson seismograph are computed, for each station/component, which, together with epicentral distances, allows for the estimation of local magnitude M _L . We used data recorded in 8 digital permanent three-component stations, with inter-stations distances up to 300 km, in the period June 1998 – June 2000, corresponding to a set of 1315 events with magnitude (M _L or M _D ) 2<M<5.8 and epicenters located in the Azores region, to estimate the coefficients of the equation to compute M _L , as well as to determine the corrections to be applied to each station. The new set of parameters, formed by attenuation coefficients and station corrections, were introduced in the calculations of the M _L , leading to smaller dispersions in the analyzed dataset. We also conclude that the attenuation in the first 150 km is similar to the California values, although higher for longer distances.     

Underwater Explosion (UWE) Analysis of the ROKS Cheonan Incident

The underwater explosion (UWE) resulting in the sinking of the South Korean warship, ROKS Cheonan occurred on March 26 2010. Raw data was analyzed from several 3-component stations—Baengyeong-do Korea Meteorological Administration (KMA) station (BAR), Ganghwa KMA station (GAHB), Incheon Incorporated Research Institutions for Seismology (IRIS) station (INCN), the short-period station—Deokjeok-do KMA station (DEI), as well as from the seismo-acoustic array Baengyeong-do Korea Institute of Geoscience and Mineral Resources (KIGAM) station (BRDAR). The ROKS Cheonan incident has been investigated by both the Multinational Civilian-Military Joint Investigation Group (Ministry of National Defense, 2010) and Hong (Bull Seism Soc Am 101:1554–1562, 2011). Their respective methods and conclusions are also presented in this study. One of the main differences between their findings and ours is that we deducted that the fundamental bubble frequency was 1.01 Hz with a subsequent oscillation of 1.72 Hz. Also, in contrast to findings by the MCMJIG and Hong, our analysis shows the first reverberation frequency to be 8.5 Hz and the subsequent one to be ≈25 Hz. The TNT-equivalent charge weight (seismic yield) and seismic magnitude were estimated from an observed bubble frequency of 1.01 Hz and the analytical model of a bubble pulse. From the data analyzed, we deducted that the seismic yield would be about 136 kg of TNT, which is equivalent to the individual yield of a large number of land control mines (LCM) which were abandoned in the vicinity of the ROKS Cheonan incident by the Republic of Korea (ROK) Navy in the 1970s (Ministry of National Defense 2010). Also, whereas both the MCMJIG and HONG estimated the local magnitude at 1.5, our findings came to the conclusion of a local magnitude of approximately 2.04 based on the bubble frequency of 1.01 Hz measured on the vertical component of BAR station data considering the empirical relationship between charge weight (TNT yield) and underwater explosion magnitude. Strong high-frequency signals collected at the 3-component BAR station approximately 30 s after P-wave arrivals and infrasound records at BRDAR clearly indicate powerful acoustic phases and N-waves caused by a relatively shallow UWE. T-phases are also observed on seismograms and spectra at 15–17 Hz on the DEI, GAHB, and INCN stations.     

Diurnal and Seasonal Variations in Trends in the <Emphasis Type="Italic">E</Emphasis>-Layer Critical Frequency

Long-term changes in the E-layer critical frequency foE at three stations in the European region (Juliusruh, Slough, and Rome) are analyzed by the method described in detail in the previous paper by the authors. It is found that two former stations demonstrate a well-pronounced change in foE (a trend) during the two previous decades. At the same time, the same features of the behavior of the aforementioned trend k(foE) are obtained for both stations. The trend is positive and negative in the morning and evening hours, respectively. It is minimal near the local noon. That explains the small value of k(foE) obtained in the previous paper for 1200 LT. A well-pronounced seasonal behavior of k(foE) is detected: the trend is minimal and maximal in the summer period and at the end of fall—beginning of winter, respectively. The trend maximal amplitude in the morning hours reaches +0.04 MHz per year, whereas the minimal amplitude in evening hours is–0.06 MHz per year. No systematic changes in foE exceeding 0.01 MHz in magnitude per year are found for Rome station.     

区域台网地震监测能力评估算法的Matlab实现

采用近震震级公式方法,在已知台站噪声水平和震中距的情况下,计算出该台能记录到的最小地震震级,在震中距最近的6个台中,通过组合排序法选取布局最优的4个台进行定位,并取这4个台站中震级最大值作为最小监测能力震级,从而得到局域台网的地震监测能力。运用Matlab软件来实现该算法,并对其中的核心处理技巧进行说明。     

Moment magnitude determination of local seismic events recorded at selected Polish seismic stations

The paper presents the method of local magnitude determination used at Polish seismic stations to report events originating in one of the four regions of induced seismicity in Poland or its immediate vicinity. The method is based on recalculation of the seismic moment into magnitude, whereas the seismic moment is obtained from spectral analysis. The method has been introduced at Polish seismic stations in the late 1990s but as of yet had not been described in full because magnitude discrepancies have been found between the results of the individual stations. The authors have performed statistics of these differences, provide their explanation and calculate station corrections for each station and each event source region. The limitations of the method are also discussed. The method is found to be a good and reliable method of local magnitude determination provided the limitations are observed and station correction applied.     

Berechnung der Funktionen einfacher Streuung auf Trübungsteilchen in der Atmosphäre

Summary In 1967, a series of observations were carried out at Lomnický tít of the intensity of light of the clear sky. Using the de Bary method[1], the observations were used to determine the function of simple dispersion on turbind particles in the atmosphere and compared with theoretical functions, which hold for Jung's power distribution of the particles according to size[7] and for the logarithmic Gauss distribution of the particles[8].     

First observation of quasi-2-day oscillations in ionospheric plasma frequency at fixed heights

The existence and development of the quasi-2-day oscillations in the plasma frequency variations of the F region at northern middle latitudes are investigated. A new approach to study the quasi-2-day oscillations is presented, using a methodology that allows us to do such a study at fixed heights. The hourly values of plasma frequency at fixed heights, from 170 km to 220 km at 10 km step, obtained at the Observatori de lEbre station (40.8°N, 0.5°E) during 1995 are used for analysis. It is found that quasi-2-day oscillations exist and persisted in the ionospheric plasma frequency variations over the entire year 1995 for all altitudes investigated. The dominant period of oscillation ranges from 42 to 56 h. The amplitude of oscillation is from 0.1 MHz to 1 MHz. The activity of the quasi-2-day oscillation is better expressed during the summer half year when several enhancements, about 15–30 days in duration, were observed. The largest enhancements of the oscillation occurred during early June, July and early August; i. e., near and after the summer solstice when the 2-day wave in the middle neutral atmosphere typically displays its largest activity in the Northern Hemisphere. The results obtained may help us understand better the possible influencing mechanisms between the 2-day wave in the middle neutral atmosphere and the ionospheric quasi-2-day oscillations.     

Winter Anomaly in the Critical Frequency of the <Emphasis Type="Italic">E</Emphasis>-Layer in the Nighttime Polar Cap

With the medians of the E-layer critical frequency foE measured at Resolute Bay and Casey ionospheric stations located in the polar caps of the Northern and Southern Hemispheres, it is found that these medians are higher at the nighttime hours (2100–0300 LT) in the local winter than in local summer. For Resolute Bay station, which is located above the Arctic Circle, the latter means that the foE median is higher at polar night than at polar day. Thus, the effect of a winter anomaly in the foE median in the nighttime polar cap is detected. The amplitude of that anomaly (the ratio of the local winter foE values to local summer values) could reach 15–20% and 10–15% for Resolute Bay and Casey stations, respectively. It is assumed that the winter anomaly in the foE median in the nighttime polar cap is caused by the winter–summer asymmetry in the accelerated electron energy fluxes precipitating into this region.     

The February 1996 earthquake sequence in the eastern Pyrenees: first results

An earthquake with local magnitude (ML) 5.2 occurred February 18, 1996 in the eastern Pyrenees (France) near the town of Saint-Paul de Fenouillet. This event is the first of this magnitude in France to be well recorded instrumentally. Less than 24 hours after the main shock, we installed a temporary network of 30 seismological stations in the epicentral area to record the aftershock sequence. In this paper, we analyse the main shock and present the 37 largest aftershocks (1.8 Ml 3.4) in the two months following the main shock. These events are located using data from the permanent Pyrenean seismological network and the temporary network when available. We also determined eight fault plane solutions using the P-wave first motions. The main shock and the aftershocks are located inside the small Agly massif. This Hercynian structure sits some 8 km north of the North Pyrenean Fault, which is usually considered to be the suture between the Iberian and Eurasian plates. The mechanism of the main shock is a left-lateral strike-slip on an E–W trending fault. The fault plane solutions of the aftershocks are mostly E–W striking reverse faults, in agreement with the general north-south shortening of the Pyrenees. The aftershocks located down to 11 km depth, indicating that the Agly massif is deeply fractured. The main interpretations of these results are: (i) The main shock involved an E–W trending fault inside the highly fractured Agly massif, relaying the North Pyrenean Fault which had, at least in the last 35 years, a poor seismic activity along this segment; (ii) The Saint-Paul de Fenouillet syncline to the north and the North Pyrenean Fault to the south delimit a 15 km wide senestral shear zone. Such a structure is also suggested by the highly fractured pattern of the Agly massif and by small en echelon faults and secondary folds in the Saint-Paul de Fenouillet syncline; (iii) we suggest that the North Pyrenean Frontal Thrust, located less than 10 km north of the Agly massif, has a ramp geometry at depth below the Agly massif.     

天津测震台网地震监测能力分析

通过计算地震台站最小监控震级,得到天津测震台网地震监测能力。采用经典谱估计中的Welch算法,计算天津测震台网31个地震台站噪声水平。取噪声水平有效值的30倍作为能检测到最小地震S波的最大振幅,通过近震震级公式,计算各台站地震震级,取第4个能被检测到的台站地震震级作为最小监控震级。     

To the problem of earthquake magnitudes determination

Summary Causes of inconsistency in magnitudes determined by broad-band and short-period instruments and by different systems of observations are elucidated. In so doing, both observations of standard stations of USSO of the USSR and those of Soviet frequency selecting seismic stations () are employed. On the basis of large statistic material of the stationare network of USSO, a dependence of spectral constitution ofP waves and frequency-temporal fields constructed for some earthquakes have been revealed as well as a dependence of magnitude values upon an arrival time of maximal particle velocity. It has been shown that the range of measuring (A/T) _max should be enlarged at least to 15 sec. A conclusion is drawn that the most stable magnitude consistent with the Catalogue by Gutenberg is the one determined by medium-period instruments.