Standard Wireline Data Processing

 

 

Science operator: Texas A&M University

Hole: U1467C

Expedition: 359

Location: Maldives (Central Equatorial N Indian Ocean)

Latitude: 4° 51.0362' N

Longitude: 73°17.0198' E

Logging date: November 3, 2015

Sea floor depth (driller's): 498.2 m DRF

Sea floor depth (logger's):498.2 m WRF (downlog)

Total penetration: 1212.2 m DRF (714 m DSF)

Total core recovered: 266.15 m (80.1 % of cored section)

Oldest sediment recovered: Miocene

Lithology: Unlithified/partially lithified and lithified planktonic foraminfera-rich wackestone to packstone

 

 

Data

 

The logging data was recorded by Schlumberger in DLIS format. Data were processed at the Borehole Research Group of the Lamont-Doherty Earth Observatory in November 2015.

 

Logging Runs

Tool string
Run
Top depth (m WMSF) Bottom depth (m WMSF) Pipe depth (m WMSF) Notes
1. MSS/HRLA/APS/HLDS/EDTC-B/HNGS
Downlog
0
676
101

Closed caliper. Invalid HLDS and APS data.

Repeat
0
713
open hole
APS nuclear source off. Invalid APS data.
Main
0
713
101

 

 

Hole conditions were reported to be good, therefore the first tool string, consisting of the MSS/HRLA/APS/HLDS/EDTC-B/HNGS tools, was rigged up with nuclear sources. The hole remained filled with sea water, as there had been no sticking during drilling. The downlog proceeded without any incident to a depth of 1211 m WRF.

A repeat pass was carried out from total depth to 1085 m WRF, with an open caliper on the HLDS tool but with the APS nuclear cource shut off, to avoid activating the formation before the main pass. During the repeat pass it was noticed that the HLDS caliper was indicating a very large hole. Initially a problem with the caliper was suspected, however there was no indication of any failure or damage. Furthermore, a lack of significant variation in the tension valeus seemed to indicate that the tool was not making contact with the borehole wall. A main pass was conducted from total depth to 485 m WRF. As in the case of the repeat pass, the caliper remained fully open for most of the open hole interval, reading lesser values down to 14" only over a small portion of the hole. Since the caliper tool did not seem to be malfunctioning and indicated an enlarged hole it was decided to cancel any further logging operations and instead use the time to drill a dedicated loggiong hole. Upon retrieval of the tool string it was found that the caliper was indeed intact and functional.

 

The sea state was calm, therefore no Wireline Heave Compensator (WHC) was used.

The depths in the table are for the processed logs (after depth shift to the sea floor and depth matching between passes). Generally, discrepancies may exist between the sea floor depths determined from the downhole logs and those determined by the drillers from the pipe length. Typical reasons for depth discrepancies are ship heave, wireline and pipe stretch, tides, and the difficulty of getting an accurate sea floor from a 'bottom felt' depth in soft sediment.

 

Processing

 

Depth shift to sea floor and depth match. The original logs were first shifted to the sea floor (- 498.2 m). The sea floor depth was determined by the step in gamma ray values at 498.2 m WRF on the MSS/HRLA/APS/HLDS/EDTC-B/HNGS downlog. This corresponds to the sea floor depth given by the drillers (see above). The depth-shifted logs have then been depth-matched to the gamma ray log from the downlog of theMSS/HRLA/APS/HLDS/EDTC-B/HNGS tool string.

 

Depth matching is typically done in the following way. One log is chosen as reference (base) log (usually the total gamma ray log from the run with the greatest vertical extent and no sudden changes in cable speed), and then the features in the equivalent logs from the other runs are matched to it in turn. This matching is performed manually. The depth adjustments that were required to bring the match log in line with the base log are then applied to all the other logs from the same tool string.

 

Environmental corrections. The HNGS and HRLA data were corrected for hole size during the recording. The APS and HLDS data were corrected for standoff and hole size respectively during the recording.

 

High-resolution data. Bulk density (HLDS) and neutron porosity (APS) data were recorded sampling rates of 2.54 and 5.08 cm, respectively, in addition to the standard sampling rate of 15.24 cm. The enhanced bulk density curve is the result of Schlumberger enhanced processing technique performed on the MAXIS system onboard. While in normal processing short-spacing data is smoothed to match the long-spacing one, in enhanced processing this is reversed. In a situation where there is good contact between the HLDS pad and the borehole wall (low-density correction) the results are improved, because the short spacing has better vertical resolution. Gamma Ray data from the EDTC-B tool were recorded at sampling rates of 5.08 and 15.24 cm.

 

Quality Control

 

The quality of the data is assessed by checking against reasonable values for the logged lithologies, by repeatability between different passes of the same tool, and by correspondence between logs affected by the same formation property (e.g. the resistivity log should show similar features to the sonic velocity log). In Hole U1467C repeatability among the tree passes was excellent.

 

The gamma ray logs recorded through bottom hole assembly (BHA) and drill pipe should be used only qualitatively, because of the attenuation of the incoming signal. The thick-walled BHA attenuates the signal more than the thinner-walled drill pipe.

 

Hole diameter was recorded by the caliper on the HLDS tool (LCAL). As described in detail in the Logging Runs section above, the caliper provided very high readings in most of the hole, with the exception of a short interval from 370 to 450 m WMSF.

 

A null value of -999.25 may replace invalid log values.

 

Additional information about the drilling and logging operations can be found in the Operations and Downhole Measurements sections of the expedition report, Proceedings of the International Ocean Discovery Program, Expedition 359. For further questions about the logs, if the hole is still under moratorium please contact the staff scientist of the expedition.


After the moratorium period you may direct your questions to:

 

Cristina Broglia

Phone: 845-365-8343

Fax: 845-365-3182

E-mail: Cristina Broglia

 

Tanzhuo Liu

Phone: 845-365-8630

Fax: 845-365-3182

E-mail: Tanzhuo Liu