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MAREES TERRESTRES BULLETIN D'INFORM
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BIM 146 December 15, 2010 New Chall
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1994), and TPXO.6 (Egbert et al., 1
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4. An attempt to improve the region
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From Fig. 2, we also see that, the
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GPS network called GEONET (GPS Eart
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References Bos, M. S., Baker, T. F.
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Planets Space, 59, 307-311. Sato, T
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Fig. 1. Locations of the observatio
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the dense seismic observation netwo
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difference of loading effects of oc
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is done with an optical lever using
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6. Application of laser interferome
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Figure 11. Strain seismograms of th
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Higashi, T., 1996, A study on chara
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2. Fundamentals and techniques At t
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100 low frequencies earth tide freq
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Tab. 4: Averages of noise levels at
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References Asch, G., Elstner, C., J
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The 1 / s part is also worth mentio
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As it was mentioned before the resu
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Fig. 9. Morlet Wavelet Spectrum, su
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9. CONCLUSIONS This investigation w
- Page 54 and 55: 2. Objectives of Aswan Tidal Gravit
- Page 56 and 57: 5. Recording of Data The data logge
- Page 58 and 59: Figure 5: Pre-processed hourly data
- Page 60 and 61: Figure 6: Residuals of gravity tide
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- Page 64 and 65: time. In addition, models for gravi
- Page 66 and 67: Fig. 3 (Zahran, 2005) shows gravity
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- Page 76 and 77: The instrumentation of the tidal st
- Page 78 and 79: 4. Tidal analysis The tidal analysi
- Page 80 and 81: References Banka, D., Crossley, D.
- Page 82 and 83: 1. Introduction The estimation of a
- Page 84 and 85: Figure 1 Air density distributions
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- Page 88 and 89: Figure 4 Attraction effect from the
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- Page 92 and 93: Figure 7 Atmospheric reductions for
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- Page 106 and 107: 4. Recording of Data The recorded d
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