HG 230.75-230.85 Thin Section

Coarse grained sediment with fine grained domains, clay material, rotation structures and lineations. Clasts range from sub-angular to sub-rounded. Mainly brown sediment with darker patches of brown throughout. Major amounts of grain crushing can be seen in the coarse grained material.

HG 257.55-257.75 Thin Section

Dark brown sediment with clasts that range from small to large. The clast shape ranges from sub-angular to sub-rounded. Lineations are abundant in this sample. Edge-to-edge grain crushing can also be seen. Darker organic rich domains are also present throughout the sample.

HG 316.65-316.80

Fine grained, dark brown sediment. Minor amounts of lineations can be seen. Faint water escape structures are also abundant.

HG 326.65-326.75

Dark brown sediment with clasts ranging from small to large. Grains are sub-angular in shape. Faint water escape structures are present.

HG 354.65-354.75

Grey sediment with clasts ranging from small to medium in size. Clasts are sub-angular to sub-rounded. Rotation structures can be seen throughout. Some clasts have multiple rotation structures surrounding them. Comet structures and lineations are also present.

HG 388.75-388.85

Dark brown sample with clasts that range from small to large. The clast shape ranges from angular to sub-rounded. Grain crushing is present in this sample along with some lineations. Faint water escape structures can also be seen.

HG 445.60-445.75

Coarse grained, light brown sample with clasts ranging from small to medium in size. The clast shape ranges from sub-angular to sub-rounded. Lineations were abundant throughout the sample. A few comet structures were also found.

HG 450.65-450.75

Mainly a coarse brown sediment with a few patches of a finer grained domain. The clasts range from small to large in size and angular to sub-rounded in clast shape. The coarser domain mainly contains grain crushing and stacking, with some rotation structures. The finer domain mainly contains lineations.

HG 3.75-3.85

Dark brown sediment with clasts ranging from small to large. The clasts range from angular to sub-rounded in shape. The sample mainly contains edge-to-edge grain crushing and rotation structures. Many grains are fractured and a few necking structures can also be seen.

HG 28.75-28.90

This sample contains clasts that range from small to large. A few fractured grains can be seen. The grain shape ranges from angular to rounded. Rotation structures can be seen throughout the sample along with some edge-to-edge grain crushing.

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 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 125.65-125.75

Brown sediment with clasts ranging from small to large in size. The clast shape ranges from angular to rounded. Rotation structures are abundant in this sample along with lineations. Comet structures and grain crushing is also present throughout this sample.

HG 129.65-129.75

Brown sediment with two main domains; a fine grained one rich in organic material and a coarse grained domain. The fine grained domain appears in several areas of the sample, and in one area alternates with the coarser domain. The coarse grained domain contains clasts ranging from small to medium in size, and angular to sub-rounded in shape. Grain crushing and lineations can commonly be seen in this domain.

HG 129.75-129.90

Brown sediment with clasts ranging from small to medium in size. Clast shape ranges from angular to sub-rounded. Rotation structures are abundant in this sample. Edge-to-edge grain crushing, comet structures, and lineations can also be seen in this sample.