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Parameter |
Description |
Validation |
Data Type |
||
WCODE (primary key) |
primary key of the waveform record archived in the
waveform-database and associated with the records of the databank |
cannot be missing |
I6 |
||
WEPIK |
distance from the epicentre to the recording station in km |
cannot be missing |
I3 |
||
WFTD |
distance from the recording station to the closest point
on the surface projection of the rupture, in km |
missing value is -99 |
I3 |
||
WAZI |
azimuth between the epicentre and the station in degrees
east of north |
0 £ wazi
< 359 cannot be missing |
I3 |
||
Local intensity Is Idef |
Is WINT |
local intensity |
I £ Is
£ XII missing value is blank |
A5 |
|
|
Idef WIDF |
acronym of the intensity scale on which the epicentral
intensity has been determined |
missing value is blank, cannot be missing, if Io is given |
A7 |
|
WSTG |
time lag in s between the P-wave arrival time or trigger
time and the S-wave arrival time |
missing value is 9.9 |
F4.1 |
||
WNCH |
total number of channels stored on this record |
1 £ wnch £ 3 cannot be missing |
I1 |
||
Corrected peak acceleration Ac_max Ac_t |
Ac_max WCAMAX WCAMAY WCAMAZ |
array with 3 elements indicating the peak acceleration
derived from corrected acceleration time histories, in m/s2 |
cannot be missing, default value: -999.999 |
3×F8.3 |
|
|
Ac_t WCATMAX WCATMAY WCATMAZ |
array with 3 elements indicating the time, in s, after the
beginning of the component records, at which the peak acceleration occurred |
cannot be missing, default value: -999.999 |
3×F8.3 |
|
Corrected peak velocity Vmax Vt |
Vmax WCVMAX WCVMAY WCVMAZ |
array with 3 elements indicating the peak velocity derived
from velocity time histories, in cm/s |
cannot be missing, default value: -999.999 |
3×F8.3 |
|
|
Vt WCVTMAX WCVTMAY WCVTMAZ |
array with 3 elements indicating the time, in s, after the
beginning of the component records, at which the peak velocity occurred |
cannot be missing, default value: -999.999 |
3×F8.3 |
|
Filenames of uncorrected time histories (primary keys) |
WRAWX WRAWY WRAWZ |
array with 3 elements, indicating the filenames of the
uncorrected time histories archived in the databank |
cannot be missing |
3×A15 |
|
Filenames of corrected time histories (primary keys) |
WCORX WCORY WCORZ |
array with 3 elements, indicating the filenames of the
corrected time histories archived in the databank |
cannot be missing |
3×A15 |
|
Filenames of Response spectra (primary keys) |
WSPCX WSPCY WSPCZ |
array with 3 elements, indicating the filenames of the
response spectra archived in the databank |
cannot be missing |
3×A15 |
|
WECODE (primary key) |
primary key of the associated earthquake record archived
in the earthquake-database |
cannot be missing |
I6 |
||
WSCODE (primary key) |
primary key of the associated station record archived in
the station-database |
cannot be missing |
I6 |
||
WREF |
source of the strong-motion record |
cannot be missing |
A250 |
Notes on parameters of waveform-database:
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Fault Distance
The distance or source-path has a significant influence on the near source behaviour of ground motion models, particularly for small events for which location and depth errors can be many times the source dimension. The assessment of source distance requires accurate focal and rupture locations as well as reliable station positions and knowledge of the source mechanism. For small magnitude crustal events the source distance is close to the epicentral distance. We took the source distance to be the closest distance to the surface projection of the fault rupture as proposed by Joyner and Boore (1981). Generally there is little difference between epicentral distance and fault distance for small magnitude crustal earthquake due to its small source dimension. |
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Local Intensity, Is
The two character fields give the local intensity and its scale has been defined, despite of a number of problems associated with the assessment of intensity. The intensity-values have been directly adopted from the literature or from bulletins without re-assessment. |
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