Why is the Remanent Magnetic Intensity of Cretaceous MORB so Much Higher Than That of Mid- to Late Cenozoic MORB?

    flowchart
    W[2005AGUFMGP33B..05W]
    LA["Linked Authors (0)"]
    LI["Linked Institutions (1)"]
    W== author ==>LA
    W== affil ==>LI
    click LA "#linked-authors"
    click LI "#linked-institutions"
Graph neighborhood for 'Why is the Remanent Magnetic Intensity of Cretaceous MORB so Much Higher Than That of Mid- to Late Cenozoic MORB?'. Click aggregate nodes to navigate.
ADS bibcode
2005AGUFMGP33B..05W
year
2005
Listed Authors
Wang, D.
van der Voo, R.
Peacor, D. R.
Listed Institutions
University of Michigan, Department of Geological Sciences, Ann Arbor, MI 48109-1005 United States
University of Michigan, Department of Geological Sciences, Ann Arbor, MI 48109-1005 United States
University of Michigan, Department of Geological Sciences, Ann Arbor, MI 48109-1005 United States

Linked Authors [?]

Linked Institutions