国产精品无码免费专区午夜_精品无码国产一区二区三区51安_AV无码久久久久不卡蜜桃_在线观看片免费人成视频无码

SUMMARY OF THE ISC BULLETIN OF EVENTS OF 2001

D.A.STORCHAK

dmitry@isc.ac.uk

Presented at the EGU meeting, Nice, April 2004
  1. ABSTRACT
  2. AGENCIES CONTRIBUTING DATA TO THE ISC
  3. SEISMIC STATIONS REPORTING TO THE ISC
  4. DISTRIBUTION OF THE ISC LOCATIONS WITH THE NUMBER OF CONTRIBUTING NETWORKS
  5. THRESHOLDS FOR MANUAL REVIEW
  6. CONTRIBUTORS TO THE ISC mb AND MS
  7. OVERALL mb COMPLETENESS
  8. HOW CONSISTENT ARE THE ISC, IDC, NEIC mb AND MS ?
  9. RELATIVE NUMBER OF VARIOUS SEISMIC PHASE REPORTS
  10. USING S-ARRIVAL TIMES FOR LOCATION
  11. COMPARISON OF ISC, NEIC, IDC DATA SETS
  12. ISC EVENTS BASED ON UNASSOCIATED STATION REPORTS
  13. EVENTS OF SPECIAL INTEREST
  14. ON-LINE ISC BULLETIN
  15. CONCLUSIONS

ABSTRACT


    The ISC Bulletin for year 2001 is now available on the Internet and the ISC CD Volume 12.  In our presentation, we will give an overview of the data published in the Bulletin. We describe the major sources of data contributed to the ISC, including arrival times and amplitude readings and compare the data sets from other major data centres with that of the ISC. We discuss the magnitude threshold policy, which was applied to select events for manual review at the ISC and show the difference between the Reviewed and Comprehensive ISC bulletins. We evaluate the importance of re-analysis on a global scale from the distribution of events for which the ISC associates independently reported phase readings or hypocentres. We also give a summary of "new" events discovered by the ISC from previously unassociated phase readings, and other events of special interest in the Bulletin. We discuss the overall and regional completeness of the Bulletin as well as reasons for the differences between mb values computed by the ISC and other major data centres.  We conclude with analysis of later phases reported to the ISC and a summary of how they were used to improve ISC hypocentres.

AGENCIES CONTRIBUTING DATA TO THE ISC


agency

    As many as 100 agencies contributed to the 2001 ISC Bulletin. The ISC generally accepts seismic data in the form of a bulletin (a collection of hypocentres and associated station readings), a catalogue of hypocentres, unassociated station readings, station readings associated to already known hypocentres and moment tensor solutions. Where possible the ISC prefers a "bulletin" as opposed to "catalogue plus unassociated readings". This allows us to produce the ISC Bulletin more efficiently and also guarantees the accuracy of associations. These maps show a large number of yellow on red circles which indicate room for improvement. A number of contributions (grey circles) have been stopped or interrupted. This is either due the closure of operations at some places, or due to failure to obtain the data in time. The ISC continues searching for new possible sources of data. A number of new or previously interrupted contributions are indicated by blue circles.

SEISMIC STATIONS REPORTING TO THE ISC


station

   The value of the ISC Bulletin is totally dependent on the network of stations around the world reporting their data to the ISC in time for analysis. The above map represents the stations which have contributed at least one reading which was actually associated to an event in the ISC Bulletin. As usual, the total number of such stations in year 2001 was large: 3085. The turnover of the reporting stations is also large. 12% of the total number have not reported during the previous year (green circles). 10% of the stations reported in year 2000 have not reported in 2001 (red circles). This is due to various reasons such as: some station were closed or moved far enough to warrant another station code or the contact with a network was lost and the data had not been contributed.

DISTRIBUTION OF THE ISC LOCATIONS WITH THE NUMBER OF CONTRIBUTING NETWORKS


netw_num

   Generally the ISC locations are more reliable if phase readings of at least two different networks are used. The ISC hypocentre will almost always be less accurate than a local one if station readings from only one network are used. This is due to the ISC using Jeffreys - Bullen travel times as opposed to the more appropriate local travel times used by local agencies.
   The figure to the left shows a distribution of ISC events with the number of distinct networks which reported it. The grey coloured part of the pie chart represents events based on station readings from just one network and therefore generally least accurately located by the ISC. Light and dark blue colour represent more accurately located events. 
   Generally, the greater the magnitude, the bigger proportion of events reported by several networks.
   Overall 79% of ISC events with a magnitude above the ISC completeness threshold of 3.8 mb were reported by at least 3 networks.

THRESHOLDS FOR MANUAL REVIEW

man_rev

   There has been no collection threshold applied at the ISC for the data year 2001. All reported events, regardless of size, have been parsed to the ISC database, processed automatically and made available to the ISC users. When it came to a manual review of the automatic bulletin, the ISC had to apply certain magnitude threshold as it could not afford to review every event. This year we concentrated on events with magnitude 3.5 and above. Apart from these, we also reviewed events with station readings reported at distances of more than 10 degrees, as well as events with reports from at least two different networks.
   The ISC only attempts relocating events from the reviewed part of the bulletin. 15% of the total number of reviewed events could not have been relocated by the ISC due to the lack of required number of station reports of P- and/or S-arrivals or poor azimuthal coverage of those reports. One of the problems is that some of the agencies still report us hypocentres but not station readings on which those hypocentres were based.

CONTRIBUTORS TO THE ISC mb AND MS

amp
  The majority of station reports eligible for ISC mb come from only a few sources. By far the largest are IDC(CTBTO),38% and NEIC,34%. Nearly every station report from IDC, DMN (Nepal) and LDG (France) comes with an amplitude for mb. More than a half of reports from NEIC, MOS (Russia), AUST (Australia) and BJI (China) contain an amplitude reading for mb.   Out of all station reports, eligible for ISC MS, only 18% contain amplitude readings. This is largely due to a limited frequency band of majority of seismic stations. As much as 97% of all amplitude reports eligible for ISC MS came from just five sources: NEIC, IDC, MOS (Russia), BJI (China) and LDG (France).

OVERALL mb COMPLETENESS


complet

   We tried to establish a completeness of three most comprehensive global bulletins: IDC, NEIC and ISC. To compare thresholds of completeness like for like we did not simply use original IDC and NEIC values of depth and magnitude. Instead, for each event from any of three bulletins, we used the best available depth and magnitude estimate available to the ISC. So the same physical event reported by all three agencies is represented by the same magnitude and depth. We only considered hypocentral solutions at depth less than 33km with available mb estimate.
   The ISC bulletin is the most complete for mb by default, as almost all IDC and NEIC events become part of the ISC bulletin. The IDC bulletin, however, is almost as complete as the ISC’s. The magnitude threshold is around 3.8 mb. NEIC bulletin is much less complete with a threshold of 4.4 mb. The reason for such difference is that the IDC forms an event if at least three station/array data are available. The accuracy of these locations is low. Such locations with rare exceptions get adopted by the ISC as the best available estimates. NEIC does not routinely include such events in it's bulletin.
   Here we only use events with available mb estimate. One has to remember that if magnitudes of smaller events were taken into consideration, than ISC bulletin would be profoundly more comprehensive source of data than any of IDC or NEIC.
   One should expect large regional variations of completeness due to predominently continental position of seismic networks.

HOW CONSISTENT ARE THE ISC, IDC, NEIC mb AND MS ?

mb_ms
   Values of the ISC network mb and MS are heavily and, in almost equal shares, dominated by contributions of amplitudes by IDC and NEIC. It is important to know how consistent the ISC mb and MS values with those of IDC and NEIC.
   Below we only considered shallow events common to ISC and IDC (NEIC), where both ISC and IDC(NEIC) mb and MS estimates are available. Such estimates were only considered reliable if based on more than 5 station measurements.
   It is clear that the IDC mb and MS values are generally smaller than those of ISC. This is possibly caused by certain deviation from standard procedures at IDC. In particular:
  •  non-standard digital filtering of waveforms prior to taking measurements;
  •  non-standard measurement procedures;
  •  constant use of arrays;
  •  predominantly low noise station positioning.
   NEIC mb and MS are generally consistent with those of the ISC.

RELATIVE NUMBER OF VARIOUS SEISMIC PHASE REPORTS

sec_pha_1
  The ISC Bulletin contains a large variety of seismic phases, but until data year 2001 only P arrivals were used by the ISC for location. The graph above shows that nearly all mb>=5 events in the bulletin have an azimuthal gap < 180 degrees, if only P arrivals are taken into account. For certain smaller events the azimuthal gap may be too large to guarantee a confident location. For instance, only 63% of mb 4.0 events have an acceptable gap. In such cases, use of arrivals other than P can assist in computing more constrained  hypocentres, even if the P gap stays insufficient.
sec_pha_2
   The above graph shows a relative number of reports for each of P, S, PcP and PKP for those poorly constrained events with azimuthal gap in excess of 180 degrees.
    For almost all mb at least 30% of all reports are phases other than P.  These additional phases could be used for event location. In fact, starting with year 2001, the ISC has been successfully using both crustal and teleseismic S arrivals for location. As far as PKP tables are concerned, PKPbc branch of Jeffreys-Bullen tables, the most often reported at distances 144-157 degrees,  is known to be incorrect. So using PKP would involve either correcting J-B or using different travel time tables.

USING S-ARRIVAL TIMES FOR LOCATION


s_1

    For the first time in it's history the ISC used local and teleseismic S-arrival times for location. The advantage is mostly visible for small events, where previously the number and azimuthal coverage of reporting stations were sometimes not sufficient to achieve a free (neither origin time, no latitutude, longitude or depth are fixed)  or fixed depth ISC location. As it appears from the upper graph, the number of events with free ISC solution as well as the overall number of solutions have increased in 2001 as compared to 2000. Overall as many as 85% of all reviewed events for 2001 were relocated by the ISC, based on all collected station reports of P and S.

s_2

   As expected, S-arrivals provided a better constraint on the event depths. In particular, the ISC free depth determinations in 2001 became slightly more consistent with ISC depths based on the pP-P reports as compared to 2000.

COMPARISON OF ISC, NEIC, IDC DATA SETS

/docs/papers/download/2004p01/azim_gap
  The ISC bulletin includes both NEIC & IDC data, so there would be at least as many station readings in each ISC event as with NEIC & IDC. However, the total number of readings is not as important for an accurate location as azimuthal gap. Above we have compared the azimuthal gaps of data sets, used by three agencies for location of common events. We have taken into account, that neither ISC nor NEIC use PKP arrivals for location, although IDC does. Therefore azimuthal gap of defining stations for some IDC events could be smaller at times. Both ISC/NEIC & ISC/IDC comparisons show that much fewer ISC events have a gap exceeding 90 and 180 degrees. As we have explained above, the superiority in azimuthal coverage of the ISC data set over the IDC one would be even bigger, had the ISC used PKP arrivals for location.

ISC EVENTS BASED ON UNASSOCIATED STATION REPORTS


new_ev

    Since 1974 the ISC has searched its unassociated phase readings to find events not reported by other agencies ("search” events). These would be events in remote areas, events in border regions and also small events, often ignored by the ISC in the past to avoid constraints on the data management and analysis system. Since 1999 the ISC has entirely removed all data collection thresholds and the number of search events dropped as a result. We now believe that the majority of the ISC search events are genuinely new. The areas include border regions in the Balkans, Turkey, Hindu Kush, Burma and the Pacific rim.
A small number of events were found this year on the mid-oceanic ridges. These events are usually reported by the IDC. In 2001 the IDC has not produced it's bulletin for 12 days due to technical reasons, which allowed the ISC to find a number of additional genuinely new events.

EVENTS OF SPECIAL INTEREST


spec_ev

    Above we have reproduced those events which were either caused by human activities or felt by people or caused damage. The distribution of the felt events generally matches the areas where both the level of seismicity and population are high. The distribution of explosions and rockbursts generally matches the areas of industrial activities. One could, for instance, observe a large number of explosions/rockbursts in Scandinavia, Northwest Russia, Germany, Poland, Slovenia, France and the United States. Unfortunately there are no reports from other areas with comparatively high level of industrial activities. In fact, some agencies prefer to exclude artificial events from their catalogues as opposed to marking them as artificial. This is not always the best approach. Such events are likely to be reported by neighbouring agencies or even by international data centres, who generally will not have precise information on the nature of the event. Having appreciated the sensitive nature of this issue, the ISC asks where possible to report artificial events along with natural ones.

ON-LINE ISC BULLETIN

    The ISC Bulletin is available on-line. A search tool allows users to select required data from the Bulletin. It is important to select an appropriate bulletin type in order to receive a desired outcome. The table below provides some guidance on the contents of each type of the ISC bulletin, it's variabilty, availability, typical total number of events along with drawbacks to be aware of when requesting data on-line.

Type

Collected

Published

Comprehensive

Contents

  • All events as reported to the ISC by other agencies
  • One physical event often reported by several agencies; these are not grouped
  • Only station readings, associated to an event in the original report
  • All events have been reviewed by the ISC seismologists
  • 84% relocated by the ISC, based on available station reports
  • Reviewed events
  • Not reviewed (small), not relocated by the ISC
  • Events reported late
  • Events corrected after review was complete

Variability

Changes with every new report; provisional agency reports get swapped for final reports

Stays exactly the same after the end of manual review

Changes with every new report or correction

Availability

Soon after an event reported

20 - 22 months after an event occurs

Soon after an event reported

Total, events

277,527

41,705

191,016

Warnings

  • Events are often duplicated as every physical seismic event is represented by as many events as reported by various agencies;
  • Events are presented exactly as they were interpreted by the automatic system;
  • None of the events have been reviewed by the ISC seismologists

16% of all events have not been relocated by the ISC due to the lack of necessary station reports. In this case one of the reported solutions is chosen as prime

  • 79% of events have not been reviewed by the ISC seismologists;
  • Non-reviewed events are not relocated by the ISC;
  • Event splits are common, especially with the data, reported to the ISC after the submission deadline


CONCLUSIONS

  • The 2001 ISC Bulletin remains the most comprehensive global source of seismic parametric data.
  • The overall completeness threshold for shallow events is found to be close to 3.8 mb. This threshold is nevertheless subject to a large regional variation.
  • As much as 79% of the ISC events with magnitude above the completeness threshold are located based on station readings from a minimum of 3 networks.
  • The ISC Bulletin events generally have smaller station azimuthal gap than those of NEIC and IDC (CTBTO).
  • The use of S-arrivals has improved the convergence statistics for small events and helped to better constrain the ISC depths. The use of other phases like PcP and PKP would be beneficial.
  • The ISC mb values are dominated by the body wave amplitudes from IDC (38% of the total number) and NEIC (34%). As much as 99% of surface wave amplitudes for ISC MS are contributed by only 5 sources: NEIC, IDC, MOS (Russia), BJI (China) and LDG (France). The ISC Bulletin would benefit from other agencies contributing amplitudes.
  • ISC mb / MS are generally consistent with those of NEIC. IDC mb / MS are generally smaller than ISC.
  • The number of new events discovered by the ISC, based on unassociated station reports, declines as more comprehensive local reports are received.
  • The ISC Bulletin would benefit from station reports contributed as associated to known hypocentres.
国产精品无码免费专区午夜_精品无码国产一区二区三区51安_AV无码久久久久不卡蜜桃_在线观看片免费人成视频无码

      黑人巨大国产9丨视频| 久久精品99国产| 免费看黄色一级大片| 色哟哟免费网站| 99草草国产熟女视频在线| 第九区2中文字幕| 亚洲老女人av| 欧美在线观看www| 日本在线视频www色| 亚洲国产高清av| 久久久久免费看黄a片app| 日韩精品视频网址| 中文字幕国产传媒| 黄色免费视频大全| 久草视频这里只有精品| 污网站在线免费| 99re在线视频免费观看| 国产黄色激情视频| 91在线第一页| 69久久久久久| 精品久久久久av| 黄色国产一级视频| 国产av熟女一区二区三区| 男女视频在线观看网站| 天天视频天天爽| 国产精品宾馆在线精品酒店| www.在线观看av| 超碰91在线播放| 天堂网在线免费观看| 无码人妻丰满熟妇区五十路百度| a天堂资源在线观看| 路边理发店露脸熟妇泻火| 日韩av加勒比| 中文字幕资源在线观看| 美女在线视频一区二区| 99热手机在线| 91视频免费版污| 国产精品涩涩涩视频网站| 亚洲国产精品久久久久爰色欲| 999一区二区三区| a级片一区二区| 91传媒免费视频| 无码人妻精品一区二区三区99v| 亚洲第一精品区| 日日噜噜噜夜夜爽爽| 色网站在线视频| 五月六月丁香婷婷| 992kp免费看片| 日本成人xxx| 欧美aaa在线观看| 久久久国产精华液999999 | 男人舔女人下面高潮视频| 成人综合视频在线| 欧美日韩一区二区在线免费观看| 97国产在线播放| 日本www在线视频| 99精品在线免费视频| 欧美日韩在线中文| 日韩一级片播放| 亚洲精品午夜在线观看| 天堂av在线8| 三上悠亚免费在线观看| 久久人人爽人人片| 三级黄色片免费看| 成人一区二区av| 男人用嘴添女人下身免费视频| 精品人妻一区二区三区四区在线 | 日韩黄色片在线| 男人的天堂狠狠干| 无码人妻丰满熟妇区毛片18| 黄色国产精品视频| 黄色国产小视频| 激情成人在线观看| 欧美高清中文字幕| 欧美丰满熟妇xxxxx| 手机在线国产视频| 五月天在线免费视频| 人妻夜夜添夜夜无码av| 99免费视频观看| www.亚洲自拍| 黄色片网址在线观看| 久草福利视频在线| 一本二本三本亚洲码| 成年人午夜免费视频| 欧美婷婷精品激情| 日本美女爱爱视频| 日韩中文字幕二区| 一级片免费在线观看视频| 69sex久久精品国产麻豆| 日日摸天天爽天天爽视频| 国产精品久久久久久久99| 黄色大片在线免费看| 久久久久久蜜桃一区二区| 国产精品无码电影在线观看| www日韩视频| 久久av喷吹av高潮av| 成年人免费在线播放| 日韩av影视大全| 国产乱子夫妻xx黑人xyx真爽 | 亚洲国产精品成人天堂| 熟女人妇 成熟妇女系列视频| 黄色www在线观看| 成人综合视频在线| 26uuu成人| 黑森林福利视频导航| 最近免费观看高清韩国日本大全| 国产成人无码一二三区视频| 日本丰满少妇黄大片在线观看| 成人小视频在线看| 国产亚洲精品久久久久久久| 麻豆三级在线观看| 乱妇乱女熟妇熟女网站| 天天干天天操天天干天天操| 女性隐私黄www网站视频| 精品视频在线观看一区二区| 日本肉体xxxx裸体xxx免费| aa视频在线播放| 色黄视频免费看| 一路向西2在线观看| 黄色免费视频大全| www.一区二区.com| 亚洲国产午夜精品| 亚洲激情在线观看视频| 99视频在线免费播放| 精品免费久久久久久久| 欧美激情国内自拍| 天天操天天爽天天射| 免费av观看网址| 国产精品三级一区二区| 手机在线视频一区| 国产 porn| 欧美一级片中文字幕| 黄色大片中文字幕| 91免费国产精品| 成人短视频在线看| 亚洲精品mv在线观看| 成人午夜激情av| 午夜精品久久久内射近拍高清| 777av视频| 日本一本中文字幕| 国产在线无码精品| 精品91一区二区三区| 91性高潮久久久久久久| 手机av在线网| 国产精品久久a| 91极品尤物在线播放国产| 日本老熟妇毛茸茸| 午夜免费精品视频| av无码精品一区二区三区| 激情综合网婷婷| 青青青在线播放| 一本久道综合色婷婷五月| 国产精品亚洲αv天堂无码| 亚洲中文字幕无码不卡电影| 精品人妻一区二区三区四区在线 | 毛片毛片毛片毛| 国产欧美一区二| 欧美一级xxxx| 中文字幕在线视频一区二区三区 | 精品无码国产一区二区三区av| 亚洲天堂第一区| 99热这里只有精品免费| 天天做天天躁天天躁| 屁屁影院ccyy国产第一页| 亚洲精品久久久久久久蜜桃臀| 日韩精品视频在线观看视频| 免费视频爱爱太爽了| 国产精品无码一区二区在线| 久久久久久久久久久视频| www.xxx亚洲| 九九热精品在线播放| 国产又大又长又粗又黄| 欧美亚洲色图视频| 乱妇乱女熟妇熟女网站| 99视频在线免费| 在线播放av中文字幕| 青青草免费在线视频观看| 可以看毛片的网址| 红桃av在线播放| 亚洲成人天堂网| 麻豆视频传媒入口| 日韩精品 欧美| 毛葺葺老太做受视频| 久久精品国产露脸对白| 国产女主播av| 精品国产一区三区| 搡女人真爽免费午夜网站| 性鲍视频在线观看| 成人av在线不卡| 国产天堂在线播放| 樱空桃在线播放| 男女激情无遮挡| 97超碰成人在线| 久久久久久av无码免费网站下载| 欧美成人免费在线观看视频| 亚洲最大综合网| 色哺乳xxxxhd奶水米仓惠香| 青青草原成人网| 91视频福利网| 日韩a在线播放|