On the problem of frequency calibration of induction variometers with large air-core loops     

Josef Bochníček  Jaroslav Šubrt  Reviewer M. Hvoždara  Reviewer J. Podlešák 《Studia Geophysica et Geodaetica》1971,15(1):76-85

Zusammenfassung Es wird eine Methode für experimentelle Untersuchung der Frequenzkennlinien von Induktionsvariometern mit Aufnahmeschleifen nichttraditioneller Ausmasse beschrieben. Die Grundlage des beschriebenen Verfahrens bildet eine genaue Bestimmung jenes Teils des magnetischen Kraftflusses, der durch die Aufnahmeschleife durchgeht.  相似文献   

Überschreitung einer breiten Gebirgsbarriere durch Rossby-Wellen     

Josef Egger 《Meteorology and Atmospheric Physics》1971,20(4):289-300

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Messung des Ultrarot-Pleochroismus von Mineralen VIII. Der Pleochroismus der OH-Streckfrequenz in Andalusit     

A. Beran  J. Zemann 《Mineralogy and Petrology》1969,13(3-4):285-292

Zusammenfassung Mikroskopisch Einschluß-freie Andalusite aus Brasilien zeigen im UR-Absorptionsspektrum ein Doppelmaximum bei zirka 2,9 und ein deutlich schwächeres einfaches Maximum bei 3,04 , die OH-Valenzschwingungen zugeordnet werden. Diese Maxima verschwinden nach mehrtägigem Glühen bei 1000° C. In Platten parallel (110) zeigt das Doppelmaximum bei zirka 2,9 einen extrem starken Pleochroismus, wobei die Bande praktisch völlig verschwindet, wenn der elektrische Vektor parallel [001] schwingt. Damit müssen zumindest die OH-Gruppen, die für diese Bande verantwortlich sind, in die Struktur eingebaut sein. Für beide Arten von OH-Gruppen werden die plausiblen Anordnungen diskutiert.

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Measurement of the infrared-pleochroism in minerals. VIII. The pleochroism of the OH-stretching frequency in andalusite

Summary Inclusion-free andalusites from Brazil show in the IR absorption spectrum a double maximum at ca. 2.9 and a much weaker single maximum at 3.04 which are interpreted as belonging to OH-stretching frequencies. The maxima disappear after annealing the specimen at 1000°C for several days. Plates parallel to (110) show a very strong pleochroism for the 2.9 -band, the peak being practically of zero height if the electric vector vibrates parallel [001]. This proves that at least the OH-groups which are responsible for this absorption band are constituents of the crystal structure. For both kinds of OH-groups the probable distributions are discussed.

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Mit 3 Abbildungen  相似文献   

Transit of an electromagnetic low-frequency disturbance through the lower ionosphere     

Josef Bochníček 《Studia Geophysica et Geodaetica》1968,12(1):91-99

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Dynamic manifestations of the geomagnetic field in the Quaternary continental sediments of Czechoslovakia     

Václav Bucha  Josef Horáček  Reviewer A. Janáčková 《Studia Geophysica et Geodaetica》1973,17(4):321-336

Summary The paper brings a brief geological asessment of the sedimentational cycles, analyses the methods of collection and investigation of samples and the representativeness of the results obtained. Problems of magnetic cleaning and the types of demagnetization curves investigated are discussed. The continuous nature of the variations of the magnetic declination, inclination and remanent magnetization, determined by palaeomagnetic investigation of Quaternary sediments, is also discussed. The conclusion contains the principal facts about the dynamics of the geomagnetic field in the Quaternary and points out the possibility of applying them to the theory of the geomagnetic field, as well as to geological correlations.  相似文献   

The Effect of Geomagnetic and Solar Activity on the Distribution of Controlling Pressure Formations in the Northern Hemisphere in Winter     

Bochníček  Josef  Hejda  Pavel  Pýcha  Josef 《Studia Geophysica et Geodaetica》1999,43(4):390-398

The distribution of controlling pressure formations, occurring in the Northern Hemisphere during the winters (January and February) of the years 1952 – 1996, has been analysed. It was found that the deepening of the Icelandic and Aleutian pressure lows is connected not only with a particular QBO phase and level of geomagnetic activity (Bochníek et al., 1999) but also with a particular level of solar activity.  相似文献   

Seeing Conditions at Sutherland. Results of the 1992/93 seeing campaign     

Josef Gochermann  Walter F. Wargau  Claus Tappert  Theodor Schmidt-Kaler  Robert S. Stobie  Fred Marang  Greg Roberts  Francois G. van Wyk  Peter Rucks 《Experimental Astronomy》1999,9(1):1-15

In order to decide whether the seeing conditions at SAAO/Sutherland justify the erection of a 3.5 m telescope and also to compare Sutherland with the Gamsberg/Namibia site, a seeing campaign covering 15 months has been carried out. For direct comparison with the results of the seeing campaign at Gamsberg twenty years before the same QUESTAR telescope was employed. The seeing is determined by the scattering of the star-trail exposed on a film in the focal plane of the telescope. The campaign commenced in February 1992. Up to May 1993, data for 204 nights, that is 47.3% of the total number of nights, were collected. Due to wind speeds above 30 km h^-1, 25 out of the 204 nights were not considered in the final reduction. The useful 179 nights are evenly distributed over the campaign period. The median seeing value for the whole period is = 0.52. There are differences during the year: the best season gives = 0.42, the worst = 0.67. Each night was divided into three intervals, although data for each of the three intervals were not always available. Generally, there is an improvement in the seeing during the course of a night. The results are compared to the seeing values of Gamsberg/Namibia and ESO/La Silla.  相似文献   

Buchbesprechungen     

J. Zemann 《Mineralogy and Petrology》1970,14(3):232-234

Ohne Zusammenfassung  相似文献   

Buchbesprechungen     

H. Wieseneder  E. Schroll  J. Zemann 《Mineralogy and Petrology》1970,14(2):168-169

Ohne Zusammenfassung  相似文献   

The period of rotation and the photoelectric lightcurve of the minor planet 79 eurynome     

Hans Josef Schober 《Icarus》1976,28(3):415-420

The minor planet 79 Eurynome was observed during the 1974 opposition for four nights in November, using a photoelectric photometer attached to the 60 cm telescope at the Observatoire de Haute Provence, France. A synodic period of P_syn = 5^h 58^m46^s ± 6^s m.e. was derived. The total amplitude of the lightcurve is only 0.05 mag. The lightcurve shows a double maximum and double minimum. Both minima appear to be at the same level. Observations were carried out in an instrumental filter system (UBV)' Results are shown only for V′, but U′ and B′ measurements supplement the conclusions concerning the rotation. The phase angle α, covered by the observations, ranges from 3 to 5°. The present results for 79 Eurynome rule out the longer period of 0^d.49830 derived by F. Scaltriti and V. Zappalà in favor of their possible period of 0^d.24915.  相似文献