Tectonic types of marginal and inner seas; their place in the development of the crust

Inner and marginal deep seas are of considerable interest not only for their genesis but also as “micromodels” of oceans. In the latter case it must be noted that some of them essentially differ from oceans in several parameters. They have a shorter period of development, thicker sedimentary cover, less distinct linear magnetic anomalies or an absence of them, high heat-flow values and seismic activity over their whole area. Consequently, the analogy with the oceans has certain limitations as the deep structure of such seas is not homogeneous and they probably vary in genesis.

Only a few marginal seas are cut off from the principal areas of the oceans by island arcs formed, most probably, along transform faults. The origin of this type is more or less reliably demonstrated for the Bering Sea. Other types of marginal seas are more numerous. Some of them (such as the Gulf of Aden and the Gulf of California) are embryonic apophyses connected with the oceans. Others are atrophied (the Tasman and the Labrador seas) small oceans. The group of marginal and inner seas which lie in the inside zone of mature or young island arcs is even more numerous. Only a few basins of this group resulted from linear spreading imprinted in the system of magnetic anomalies (the Shikoku-Parese-Vela basin), the rest are supposed to have been formed in the process of diffusal or polyaxial spreading of recent time as in Afar.

The majority of inner and marginal seas are younger than recent oceans. They are formed by rifting, oriented crosswise to continental margins of the Atlantic type or along the strike of margins of Andean type. More ancient basins of marginal and inner seas have been involved in Phanerozoic orogens or more rarely became parts of platforms (Ciscaspian syneclise).