HG 493.80-493.90

Coarse brown sediment, with clasts ranging from small to large in size. Clast shape ranges from sub-angular to rounded. Lineations and grain crushing are common throughout the sample. It also contains comet structures and a few rotation structures. Many of the larger clasts are also fractured.

HG 498.20-498.35

Coarse grained sample with clasts ranging from small to medium in size. Clast shape ranges from angular to sub-rounded. Lineations and rotation structures are common in this sample. Grain crushing and comet structures are also present in minor amounts.

HG 2.60-2.70

Brown sediment clasts ranging from small to large in size. Clasts range from sub-angular to sub-rounded in shape. Comet structures and grain crushing are commonly seen in this sample. Lineations and a few rotation structures can also be seen.

HG 35.0-35.10

Brown sediment with clasts that range from small to medium in size. The grain shape ranges from angular to sub-rounded. Lineations and rotation structures were the most common throughout the sample. Grain crushing/stacking and a few comet structures were also present. Clay material was also dispersed throughout the sample.

HG 70.40-70.50

Dark brown sediment with clasts ranging from small to large in size. Clast shape ranges from angular to sub-rounded. Lineations and comet structures can commonly be seen throughout the sample. Some rotation structures and grain crushing can also be seen in varying amounts.

HG 75.45-75.60

Dark brown sediment with clasts ranging from small to medium in size. The clast shape ranges from angular to sub-rounded. Lineations are commonly seen throughout the sample. Grain crushing/stacking can also be seen along with varying amounts of rotation structures and comet structures.

HG 77.35-77.45

Brown sediment with clasts ranging from small to medium in size. The clast shape ranges from angular to sub-rounded. Lineations are the most abundant in this sample, along with grain crushing. A few comet structures and rotation structures can also be seen throughout the sample.

HG 80.75-80.85

Dark brown sediment with clasts ranging from small to large in size. Clast shape ranges from angular to rounded. Lineations and comet structures are the most common in this sample. Some rotation structures can also be seen.

HG 87.30-87.35

Dark brown sediment with clasts ranging from small to medium in size. Clast shape ranges from angular to sub-rounded. Rotation structures and lineations are common throughout the sample. Comet structures and grain stacking/crushing can also be seen in minor amounts.

HG 109.60-109.70

Dark brown sediment with clasts ranging from small to medium in size. Clast shape ranges from angular to sub-rounded. Lineations and comet structures are abundant. Some grain crushing and rotation structures can also be seen.

HG 111.70-111.80

Brown sediment with clasts ranging from small to large in size. Clast shape ranges from sub-angular to rounded. Lineations are abundant in this sample. Some rotation structures and comet structures can also be seen in varying amounts. Some organic matter can also be seen.

HG 114.40-114.50

Brown sediment with clasts ranging from small to medium in size. Clast shape ranges from angular to sub-rounded. Lineations are the most abundant microstructure, but this sample also includes some comet and rotation structures as well.

HG 114.60-114.70

Brown sediment with clasts ranging from small to medium in size. Clast shape ranges from angular to sub-rounded. Lineations and rotation structures are common throughout this sample. Some comet structures and grain crushing can also be seen throughout in minor amounts.

HG 116.45-116.55

Light brown sediment with clasts ranging from small to large. The clast shape ranges from angular to rounded. Rotation structures are abundant in this sample. Some necking structures and comet structures can also be seen, along with a few lineations.

HG 120.0-120.10

Brown sediment with clasts ranging from small to medium in size. Clast shape ranges from sub-angular to sub-rounded. Lineations are common throughout this sample, along with some comet structures. Minor amounts of rotation structures can also be seen.