Saudi Arabian Broadband Array
Summary
- Network Code: XI
- Experiment duration: 1995-11 to 1997-02
- Number of events: 1929
- Prinicpal investigators: Frank Vernon, Jon Berger
- Download dataless SEED volume
Introduction
From November 1995 to March 1997 a total of nine broadband temporary stations were deployed across the Saudi Arabian shield. These stations consisted of STS-2 seismometers recorded continuously at 40 sps on REFTEK dataloggers. All installations were at bedrock sites. The results from our field deployment of nine portable broadband stations suggest that sites in the Arabian shield are extremely quiet. Using data sections selected randomly during the deployment, noise studies showed that most stations were exceptionally quiet with noise levels near the USGS Peterson (1993) low noise model for frequencies higher than 0.1 Hz. At lower frequencies, the horizontal components showed increased noise levels, possibly due to instrumental characteristics. High-frequency ( > 1 Hz) noise varied as much as 10 dB between day and night for some stations (RAYN, TAIF) while more isolated stations (HALM) were constant. Seasonal noise levels also varied, with April to June being the quietest months. Slight changes in peak microseism frequency also occurred seasonally. The quietest stations were HALM, RAYN, AFIF and UQSK, all of which were located in central Saudi Arabia and showed noise levels near the low noise model for frequencies between 0.1 and 4 HZ. The optimal site for a new station would be near HALM as it was both quiet and showed very little diurnal variation due to cultural noise.
The low noise at these stations also contributes to the very low detection threshold of events with mb = 3.5 at distances from 10 to 100 degrees. These stations appear to be among the best sites in the world for the properties of detection thresholds and ground noise levels. Seismograms from sources 10 degrees from the center of the network have unique characteristics which can be used to identify the source regions. Zagros events have a clear Pn and Sn arrivals with an observable Lg. Shallow events from the Arabian Sea have clear P, S, and surface waves but no discernible Lg phases. From the opposite direction, aftershocks from the Gulf of Aqaba have very weak P and S waves with very strong Lg phases.
Station List
| sta | ondate | offdate | lat | lon | elev | staname | statype | refsta | dnorth | deast |
|---|---|---|---|---|---|---|---|---|---|---|
| AFIF | 1995001 | – | 23.931 | 43.04 | 1.116 | Afif, Saudi Arabia | ss | HALM | 121.2775 | -129.8206 |
| BISH | 1995001 | 1996071 | 19.9228 | 42.6901 | 1.379 | Bisha, Saudi Arabia | ss | HALM | -324.0641 | -170.17 |
| HALM | 1995001 | – | 22.8454 | 44.3173 | 0.93 | Hadabat Al-Mahri, Saudi Arabia | ss | HALM | – | – |
| RANI | 1995001 | – | 21.3116 | 42.7761 | 1.001 | Raniyah, Saudi Arabia | ss | HALM | -169.7276 | -159.6634 |
| RAYN | 1995001 | 1996160 | 23.522 | 45.5008 | 0.792 | Ar-Rayn, Saudi Arabia | ss | HALM | 75.7196 | 120.6603 |
| RAYN | 1996161 | – | 23.5225 | 45.5032 | 0.631 | Ar-Rayn, Saudi Arabia | ss | HALM | 75.7772 | 120.9045 |
| RIYD | 1996069 | – | 24.722 | 46.643 | 0.717 | Riyadh, Saudi Arabia | ss | HALM | 210.5587 | 234.9251 |
| SODA | 1995001 | – | 18.2921 | 42.3769 | 2.876 | Al-Soda, Saudi Arabia | ss | HALM | -505.0186 | -205.0602 |
| TAIF | 1996150 | – | 21.281 | 40.349 | 2.05 | Taif, Saudi Arabia | ss | HALM | -168.5365 | -411.1522 |
| UQSK | 1996161 | – | 25.789 | 42.36 | 0.95 | Uqlat Squoor, Saudi Arabia | ss | HALM | 328.6509 | -196.0379 |
Total: 10
Channel List
| sta | chan | ondate | chanid | offdate | ctype | edepth | hang | vang | descrip |
|---|---|---|---|---|---|---|---|---|---|
| AFIF | BHE | 1995001 | 2082 | – | n | -0 | 90 | 90 | – |
| AFIF | BHN | 1995001 | 2083 | – | n | -0 | 0 | 90 | – |
| AFIF | BHZ | 1995001 | 2084 | – | n | -0 | 0 | 0 | – |
| BISH | BHE | 1995001 | 2085 | 1996071 | n | -0 | 90 | 90 | – |
| BISH | BHN | 1995001 | 2086 | 1996071 | n | -0 | 0 | 90 | – |
| BISH | BHZ | 1995001 | 2087 | 1996071 | n | -0 | 0 | 0 | – |
| HALM | BHE | 1995001 | 2088 | – | n | -0 | 90 | 90 | – |
| HALM | BHN | 1995001 | 2089 | – | n | -0 | 0 | 90 | – |
| HALM | BHZ | 1995001 | 2090 | – | n | -0 | 0 | 0 | – |
| RANI | BHE | 1995001 | 2091 | – | n | -0 | 90 | 90 | – |
| RANI | BHN | 1995001 | 2092 | – | n | -0 | 0 | 90 | – |
| RANI | BHZ | 1995001 | 2093 | – | n | -0 | 0 | 0 | – |
| RAYN | BHE | 1995001 | 2094 | 1996160 | n | -0 | 90 | 90 | – |
| RAYN | BHE | 1996161 | 2095 | 1997032 | n | 0 | 90 | 90 | – |
| RAYN | BHN | 1995001 | 2096 | 1996160 | n | -0 | 0 | 90 | – |
| RAYN | BHN | 1996161 | 2097 | 1997032 | n | 0 | 0 | 90 | – |
| RAYN | BHZ | 1995001 | 2098 | 1996160 | n | -0 | 0 | 0 | – |
| RAYN | BHZ | 1996161 | 2099 | 1997032 | n | 0 | 0 | 0 | – |
| RIYD | BHE | 1996069 | 2100 | – | n | -0 | 90 | 90 | – |
| RIYD | BHN | 1996069 | 2101 | – | n | -0 | 0 | 90 | – |
| RIYD | BHZ | 1996069 | 2102 | – | n | -0 | 0 | 0 | – |
| SODA | BHE | 1995001 | 2103 | – | n | -0 | 90 | 90 | – |
| SODA | BHN | 1995001 | 2104 | – | n | -0 | 0 | 90 | – |
| SODA | BHZ | 1995001 | 2105 | – | n | -0 | 0 | 0 | – |
| TAIF | BHE | 1996150 | 2106 | – | n | -0 | 90 | 90 | – |
| TAIF | BHN | 1996150 | 2107 | – | n | -0 | 0 | 90 | – |
| TAIF | BHZ | 1996150 | 2108 | – | n | -0 | 0 | 0 | – |
| UQSK | BHE | 1996161 | 2109 | – | n | -0 | 90 | 90 | – |
| UQSK | BHN | 1996161 | 2110 | – | n | -0 | 0 | 90 | – |
| UQSK | BHZ | 1996161 | 2111 | – | n | -0 | 0 | 0 | – |
Total: 30
Selected References
- Frank Vernon and Jon Berger, 1998, Broadband Seismic Characterization of the Arabian Shield: Final Scientific and Technical Report, Department of Energy, Issued by Phillips Laboratory under Contract No F19628-95-K-0015
URL: http://eqinfo.ucsd.edu/deployments/saudi_arabia.php [Last updated: 2006-10-26 (299) 22:47:09 UTC]