Geoscience Reference
In-Depth Information
Ta b l e 2
Selected WWSSN stations for the USGS/ICSU scanning project
Number
Code
Latitude
Longitude
Location
Digital station
−
16.46
−
71.49
0011
ARE
Arequipa,
Peru NNA
−
0038
ESK
55.32
3.21
Eskdalemuir,
Scotland ESK
0078
NNA
−
11.99
−
76.84
Nana,
Peru NNA
0001
AAE
9.03
38.77
Addis Ababa,
Ethiopia FURI
0005
AFI
−
13.91
−
171.78
Apia,
Western Samoa AFI
0112
ANP
25.18
121.52
Anpu,
Taiwan TATO
0009
ANT
−
23.70
−
70.42
Antofagasta,
Chile LVC
0021
BOG
4.62
−
74.07
Bogota,
Columbia BOCO
0026
CHG
18.79
98.98
Chiengmai,
Thailand CHTO
0028
COL
64.90
−
147.79
College,
Alaska COL,COLA
0030
COR
44.59
−
123.30
Corvallis,
Oregon CSR
0031
CTA
−
20.09
146.25
Charters Towers,
Australia CTAO
0033
DAV
7.09
125.57
Davao,
Philippines DAV
0042
GIE
−
0.73
−
90.30
Galapagos
Islands,
Ecuador PAYS
0044
GUA
13.54
144.91
Guam,
Marianas Islands GUMO
0048
HNR
−
9.43
159.95
Honiara,
Solomon Islands HNR
0070
KBS
78.92
11.92
Kingsbay,
Spitsbergen KBS
0052
KEV
67.76
27.01
Kevo,
Finland KEV
0053
KIP
21.42
158.02
Kipapa,
Hawaii KIP
0055
KON
59.65
9.63
Kongsberg,
Norway KONO
0064
MAT
36.54
138.21
Matsushiro,
Japan MAJO
0072
MUN
−
31.98
116.21
Mundaring,
W. Australia NWAO (142 km)
0074
NAI
−
1.27
36.80
Nairobi,
Kenya NAI, KMBO
0073
NAT
−
5.12
−
35.03
Natal,
Brazil RCBR (40 km)
0086
PMG
−
9.41
147.15
Port Moresby,
New Guinea PMG
0093
QUI
−
0.20
−
78.50
Quito,
Ecuador OTAV (49 km)
−
−
0095
RAR
21.22
159.77
Rarotonga,
Cook Islands RAR
−
0099
SBA
77.85
166.76
Scott Base,
Antarctica SBA
0102
SE0
37.57
126.97
Seoul,
Korea INCN (31 km)
0106
SJG
18.11
−
66.15
San Juan,
Puerto Rico SJG
0108
SPA
−
90.00
0.00
South Pole,
Antarctica SPA, QSPA
0113
TAU
−
42.91
147.32
Hobart,
Tasmania TAU
0119
TUC
32.31
−
110.78
Tucson,
Arizona TUC
0122
WEL
−
41.29
174.77
Wellington,
New Zealand SNZO (6 km)
0123
WES
42.38
−
71.32
Weston,
Massachusetts HRV (24 km)
0124
WIN
−
22.57
17.10
Windhoek,
Namibia TSUM (375 km)
0096
RCD
44.08
103.21
Rapid City,
S. Dakota RSSD (67 km)
0101
SCP
40.80
−
77.87
State College,
Pennsylvania SSPA (18 km)
25 years. It also includes the large temporary network archive of the IRIS PASS-
CAL Program data (http://www.iris.edu/about/PASSCAL/). It is responsible for the
long-term (perpetual) archive and distribution of all IRIS generated data, and is the
primary archive for the FDSN (http://www.fdsn.org/). The funding for IRIS comes
from the National Science Foundation (through its Division of Earth Sciences), and
acts in a leadership role to create a perpetually viable, openly accessible archive
for seismic data. The DMC is the core component of the IRIS Data Management
System (for more information, refer to http://www.iris.edu/).
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