Patterns in the variations of copepod spring and summer abundance in the northeastern Norwegian Sea and the Barents Sea in cold and warm years during the 1980s and 1990s   总被引：4，自引：1，他引：4  

Tande  K. S.; Nilssen  E. M.; Edvardsen  A.; Drobysheva  S.; Nesterova  V.; Tereschenko  V. 《ICES Journal of Marine Science》2000,57(6):1581-1591

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Electromagnetic sounding of the Kola Peninsula with a powerful extremely low frequency source   总被引：1，自引：0，他引：1  

Velikhov  E. P.  Grigoriev  V. F.  Zhdanov  M. S.  Korotayev  S. M.  Kruglyakov  M. S.  Orekhova  D. A.  Popova  I. V.  Tereschenko  E. D.  Schors  Y. G. 《Doklady Earth Sciences》2011,438(1):711-716

Experiment on electromagnetic sounding of the Kola Peninsula using unique mobile measuring complex of the low-frequency sounding was conducted, allowing to investigate a geoelectric section with a depth of several kilometers on distances up to 100 km from the stationary transmitting aerial. Excess on the order of amplitudes of the vertical component above the horizontal at all frequencies of sounding was registered in a number of points of measurements. This feature managed to be explained quantitatively by circulation of current on regional faults with the closure of current through the sea—before unknown galvanic coastal effect. Interpretation of the results of modeling and neural network solving of inverse problem essentially specifies the fault tectonics of the central part of the Kola Peninsula. Anomaly remote from the observation profile was found out—local pinch of a crustal conductive layer consisting of graphitized rocks and associated with the zone of overthrust.  相似文献   

Asteroid observations at low phase angles: III. Brightness behavior of dark asteroids     

Vasilij G. Shevchenko  Vasilij G. Chiorny  Yury N. Krugly  Igor A. Tereschenko 《Icarus》2008,196(2):601-611

The results of photometric observations of eight main-belt asteroids with low surface albedo are presented. The magnitude-phase dependences including low phase angles (<1 deg) have been obtained for Asteroids 76 Freia (down to phase angle 0.1 deg, P-type), 190 Ismene (0.3 deg, P-type), 303 Josephina (0.2 deg, C-type), 309 Fraternitas (0.1 deg, C-type), 313 Chaldaea (0.1 deg, C-type), 444 Gyptis (0.8 deg, P-type), 615 Roswitha (0.1 deg, C-type), and 954 Li (0.03 deg, FCX-type). The behavior of brightness in the range of opposition effect is found to be practically linear for 190 Ismene with amplitude of opposition effect only 0.03 mag. Amplitudes of the opposition effect for other asteroids are close to a mean for this type. The obtained data allowed us also to determine the rotation periods of asteroids: 303 Josephina (12.497±0.001 h), 309 Fraternitas (11.205±0.005 h), 615 Roswitha (4.422±0.001 h) and 954 Li (7.207±0.002 h). The color indexes B-V, V-R and R-I have been determined for some asteroids.  相似文献