Geophysical Institute of the ASCR

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How to get to the Geophysical Institute ♦ When arriving by car... direction Brno, take Exit Spořilov and immediately another Exit Spořilov. Coming from Brno, take Exit Spořilov. ♦ When arriving by train… Most probably you will arrive at the Main railway station or railway station Holešovice. Take Subway, Line C, direction Háje. Go until station Roztyly. When you get to the surface, you can see the new building of the T-MOBILE Company. The Geophysical Institute is beyond this building and beyond the highway. You can recognize it by the great white parabolic antenna with the label NEXTEL. The final walk will take about 10 minutes. ♦ When arriving by plane… Take bus No.119 to the bus terminal Dejvická. Take Subway Line A (green color) to station Museum. Change to line C (red color), direction Háje. Get off at station Roztyly. You can see the building of the institute beyond the new building of T-MOBILE Company and beyond the highway. You can recognize it by the great white parabolic antenna with the label NEXTEL. 73
Art exhibitons at the Geophysical Institute In 2004 - 2005, eight exhibitions of the following artists took place at the Geophysical Institute: Miroslav Koval (Sobotín, N. Moravia; drawings and photographs), Karel Adamus (Třinec, Silesia; drawings), Pavla Francová (Prague; pastels and touch drawings), Václav Vokolek (Tursko, central Bohemia; drawings, paintings, texts), Ryosuke Cohen (Japan; mailart), Jan Wojnar (Třinec, Silesia; grid poesy), Pavel Mühlbauer (Prague; drawings, paintings, pastels) and Jindřich Růžička (Prague; drawings, linocuts). The drawing on the opposite page is a photograph by Jindřich Růžička. 74
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Academy of Sciences of the Czech Re
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Estimates of P-wave anisotropy from
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Scientific Divisions of the ASCR Ma
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Organization Units of the Geophysic
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Staff of the Geophysical Institute,
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Observatories of the Geophysical In
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The air-ground temperature monitori
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Geographic locations of the observa
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fourth logging. A passage of the fr
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Fig. 3. The borehole climate change
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Fig. 5. Monitoring results (1995-20
Page 25 and 26: Fig. 6. Residual gravity anomalies
Page 27 and 28: Fig. 9. Example showing measured P-
Page 29 and 30: Fig. 10. A simplified sketch showin
Page 31 and 32: Deep structure, seismotectonics and
Page 33 and 34: References Špičák A., Hanuš V.
Page 35 and 36: etrieved by inversion of surface wa
Page 37 and 38: References Babuška V., Plomerová
Page 39 and 40: References Brož M., Hrubcová P.,
Page 41 and 42: consecutive event pairs occurring s
Page 43 and 44: Amplitude ratios for complete momen
Page 45 and 46: References Vavryčuk V., 2005. Foca
Page 47 and 48: Fig. 28. Projections of the 3D ray
Page 49 and 50: Fig. 30 shows comparison of QI (red
Page 51 and 52: Electromagnetic depth soundings A c
Page 53 and 54: with the maximum/minimum resistivit
Page 55 and 56: spectral methods (Hejda and Reshetn
Page 57 and 58: vertical profiles of magnetic susce
Page 59 and 60: ) The rapidly varying geomagnetic f
Page 61 and 62: Let us try to answer the question w
Page 63 and 64: Drilling the Eger Rift in Central E
Page 65 and 66: provided by IAGA, was used to cover
Page 67 and 68: 2005 Fulbright Scholarship, Prof. G
Page 69 and 70: Structure of the budget of the Geop
Page 71 and 72: Project code Title Principal invest
Page 73 and 74: Selected publications Alcalá M.D.,
Page 75: Vavryčuk V., Hrubcová P., Brož M
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Geophysical Institute of the ASCR

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