Tempestite

Tempestites had been identified in the rock record for a long time, however the exact sequence of sedimentary structures that are commonly seen in the rock record, known as the idealized sequence, wasn't described until 1979 by Dott and Bourgeois. This idealized sequence follows the order of a hummocky cross stratified layer (H) often with sole markings on the base, followed by a planar laminated layer (F) synonymous to the lower place bed, followed by a cross laminated layer (X) preserved as ripple marks in plan view, and finally topped with a muddy layer (M) which is generally interpreted to be caused by suspensions settling of finer material during the waning period of the storm. Each one of these sedimentary structures can be affected by bioturbation, when organisms living in the sediment at the time burrow through it. Bioturbation, can be a great indicator of the depth of the water column the tempestite was deposited in, in a given study area, through the use if ichnology, as certain organisms will only persist at certain depths and will generate unique markings within the sedimentary structures that can be identified. However too much bioturbation can wipe out the preservation of the sedimentary structures and essentially making the bed massive, making the confident interpretation of a tempestite much more difficult for geologists.[2] Tempestites can also amalgamate due to their erosive bases and this will cause for portions of the idealized H-F-X-M sequence to repeat, as each storm event has eroded down into the sediment that was deposited by the last, and incorporating that sediment into its own deposit.[3]

Tempestite deposits are very useful for aiding in paleoecological and paleogeographical interpretations. As storms that generate tempestite deposits can only form in between 5 degrees and 20 degrees north and south latitude (with even the largest 1000 year storm only being preserved upwards of 35 degrees latitude), accurate recognition of a tempestite deposit within the rock record allows for confident interpretation of a range of latitudes. Since hummocky cross stratification forms during the combined flow and waning oscillatory flow current regimes, the preserved amplitudes of their hummocks and swales are reflective of the storm intensity. Once it is understood where the deposit in question was deposited relative to the paleo-shoreline, which can usually be done using the ichnological data preserved in the same location, the hummock amplitudes/wavelengths, grainsize (decreases with increase in paleo water depth), and bedding thickness (decreases with increase in paleo water depth) can be used to estimate the storm intensity/energy. An understanding of the intensity of past storms has large implications for our understanding of how storm intensity might change with climate change occurring today. During the Cretaceous, CO₂ levels were much higher and the global temperature was much higher. With an understanding of how storm intensity changed throughout this time period towards today, we can begin to understand how it will change with our changing climate.[4]

Tempestite deposits are also highly sought after petroleum reservoirs, as they are large laterally continuous sheet like deposits that have the potential to hold high volumes of petroleum with good permeability and porosity.