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Structure and evolution of the Carlsberg Ridge : Evidence for non-stationary spreading on old and modern spreading centres. / Merkouriev, S. A.; Sotchevanova, N. A.

In: Current Science, Vol. 85, No. 3, 10.08.2003, p. 334-338.

Research output: Contribution to journal › Article › peer-review

Harvard

Merkouriev, SA & Sotchevanova, NA 2003, 'Structure and evolution of the Carlsberg Ridge: Evidence for non-stationary spreading on old and modern spreading centres', Current Science, vol. 85, no. 3, pp. 334-338.

APA

Merkouriev, S. A., & Sotchevanova, N. A. (2003). Structure and evolution of the Carlsberg Ridge: Evidence for non-stationary spreading on old and modern spreading centres. Current Science, 85(3), 334-338.

Vancouver

Merkouriev SA, Sotchevanova NA. Structure and evolution of the Carlsberg Ridge: Evidence for non-stationary spreading on old and modern spreading centres. Current Science. 2003 Aug 10;85(3):334-338.

Author

Merkouriev, S. A. ; Sotchevanova, N. A. / Structure and evolution of the Carlsberg Ridge : Evidence for non-stationary spreading on old and modern spreading centres. In: Current Science. 2003 ; Vol. 85, No. 3. pp. 334-338.

BibTeX

@article{36dea619741b49a8bc3699249d81c89a,
title = "Structure and evolution of the Carlsberg Ridge: Evidence for non-stationary spreading on old and modern spreading centres",
abstract = "We present the results of magnetic and bathymetric data collected on board Russian vessels during the last decade. Our analysis shows that since late Cretaceous the proto-Carlsberg Ridge (CR) was spreading at a faster rate, prior to India's collision with Eurasia. Since Eocene, the present CR is characterized by slow spreading. Our results depict two discordant systems of linear magnetic anomalies. One corresponds with fast spreading with respect to latitude axis of the proto-ridge and the other with slow spreading with respect to modern axis of the CR, suggesting that the two spreading systems are asymmetric both relative to each other and relative to axial anomaly. We infer that during both these periods the structure and spreading on the CR was non-stationary.",
author = "Merkouriev, {S. A.} and Sotchevanova, {N. A.}",
year = "2003",
month = aug,
day = "10",
language = "English",
volume = "85",
pages = "334--338",
journal = "Current Science",
issn = "0011-3891",
publisher = "Indian Academy of Sciences",
number = "3",

}

RIS

TY - JOUR

T1 - Structure and evolution of the Carlsberg Ridge

T2 - Evidence for non-stationary spreading on old and modern spreading centres

AU - Merkouriev, S. A.

AU - Sotchevanova, N. A.

PY - 2003/8/10

Y1 - 2003/8/10

N2 - We present the results of magnetic and bathymetric data collected on board Russian vessels during the last decade. Our analysis shows that since late Cretaceous the proto-Carlsberg Ridge (CR) was spreading at a faster rate, prior to India's collision with Eurasia. Since Eocene, the present CR is characterized by slow spreading. Our results depict two discordant systems of linear magnetic anomalies. One corresponds with fast spreading with respect to latitude axis of the proto-ridge and the other with slow spreading with respect to modern axis of the CR, suggesting that the two spreading systems are asymmetric both relative to each other and relative to axial anomaly. We infer that during both these periods the structure and spreading on the CR was non-stationary.

AB - We present the results of magnetic and bathymetric data collected on board Russian vessels during the last decade. Our analysis shows that since late Cretaceous the proto-Carlsberg Ridge (CR) was spreading at a faster rate, prior to India's collision with Eurasia. Since Eocene, the present CR is characterized by slow spreading. Our results depict two discordant systems of linear magnetic anomalies. One corresponds with fast spreading with respect to latitude axis of the proto-ridge and the other with slow spreading with respect to modern axis of the CR, suggesting that the two spreading systems are asymmetric both relative to each other and relative to axial anomaly. We infer that during both these periods the structure and spreading on the CR was non-stationary.

UR - http://www.scopus.com/inward/record.url?scp=4444373074&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:4444373074

VL - 85

SP - 334

EP - 338

JO - Current Science

JF - Current Science

SN - 0011-3891

IS - 3

ER -

ID: 51324424