Automatic grain measurements

For the measurements a Hitachi KP 161 CCD camera, a PC with built-in frame grabber and the software package IPPLUS, version 4 were used. Before each measurement series the system has to be calibrated.

The sediment sample was homogenised, sieved over a 2000µm sieve and split. Next, grains from the resulting sample were loosely scattered on a petri dish in such a way that grains are isolated as much as possible. With camera and frame grabber a picture of about 50 grains was produced on the monitor. Next there is a visual screening for grains that are lying against or one top of each other and that could be interpreted by the software as one grain. If so, these grains were separated. 

The picture of about 50 grains was analysed by IPPLUS in such a way that marginal grains were not considered. In this way 10 pictures were studied. The resulting 500 values for the grain surface were put in a spread-sheet. From the surfaces, the volumes of the grains were calculated following Komar & Cui (diameter = 2.sqrt(surface/p); volume = diameter3 ). These volumes are used for the cumulative values. The volume percentages below a certain diameter were calculated by interpolation, for which a straight line in between two relevant points was used as a basis. This implies that when grain size differences in between two consecutive points are larger, errors will also be larger. In practice this is an issue by the coarser phi-values.
 
 
MPS Sieve IPPLUS
72GS14-1  D20 261 207
                  D50 357 319
                  D80 509 442
72GS14-2  D20 274 236
                  D50 376 332
                  D80 534 449
72GS14-3  D20 242 199 330
                  D50 332 313 446
                  D80 468 434 728
72GS14-4  D20 393 307 451
                 D50  553 469 665
                  D80 777 768 950
72GS14-5 D20 365 294
                  D50 517 430
                  D80 739 721
00DW25-4 D20 238 190 298
D50 387 322 526

                 D80 651 639 947
00DW25-4 D20 238 190 298
                 D50 387 322 526
                 D80 618 493 787
72GS15-1 D20 305 211 372
                  D50 390 320 528
                  D80 502 437 867
72GS15-2  D20 297 271 312
                  D50 406 354 437
                  D80 569 464 730
72GS15-3 D20  271 239 398
                  D50 362 327 557
                  D80 490 433 889
72GS15-4 D20 301 231 414
                  D50 457 361 669
                  D80 659 585 1173
72GS15-5 D20 260 213
                 D50 418 344
                 D80 606 517
00DW24-3 D20 203 161 210
D50 304 257 285
D80 454 403 366
00DW24-4 D20 292 244 268
D50 457 379 572
D80 685 653 805

Table 1. D20,  D50 and D80 values of grain size distributions using laser counter (MPS), sieve and grain shape (IPPLUS) methods. Samples originate from counterflush borings (GS) and  vibrocores (DW). 

Results

The results obtained from this short study are twofold: a comparison between sampling techniques i.e. between coring and counterflush drilling and the comparison between various analytical methods.

As regards the sampling techniques: the expectation was that the grain size results based on counterflush samples would show coarser values compared to the core samples because of the spill-over of fines out of the sampling basins. Indeed, from the 2 one-metre intervals studied, both intervals showed coarser values for the counterflush sample. Besides, the core samples do show a somewhat higher (although still low) percentage mud than the counterflush samples. Seabed dynamics with time might have caused an appreciable grain size variability.

A comparison of the three analytical methods showed that the laser counter results were systematically coarser than the sieving results i.e. with a factor of 1.13. In earlier, more precise, comparisons using a set of sieves a half-phi 

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