Relative paleointensity record during the last 800 ka from the equatorial Indian Ocean: Implication for relationship between inclination and intensity variations

Paleomagnetic and rock magnetic investigations were carried out on three sediment cores taken from the Ninetyeast Ridge, the eastern equatorial Indian Ocean. The cores are 4.1–10.2 m long and cover the last 270–790 ka with average sedimentation rates of 1.3–1.9 cm/ka. Generally stable demagnetization behaviors and relatively uniform rock magnetic characteristics allowed us to reconstruct relative paleointensity records (NRM 30mT /IRM 30mT ) for each core. The relative paleointensity records showed a beneficial agreement with each other except for the uppermost parts of the cores, and patterns similar to the Sint‐800 paleointensity stack and other relative paleointensity records. Spectral analyses of the relative paleointensity records revealed a dominant periodicity at about 100 ka, but not for the normalizer and other rock magnetic proxies. These results suggested that the 100 ka periodicity in the paleointensity records during the Brunhes Chron would not be caused by sedimentological effects. The mean inclination values of the three cores were close to the expected hypothetical geocentric axial dipole (GAD) direction, which implies that ∼5–10° of negative inclination anomaly (Δ I ) is centered at the western equatorial Pacific Ocean, and not extended to the eastern equatorial Indian Ocean. A comparison between the relative paleointensity variation and Δ I amplitude between the eastern equatorial Indian Ocean and the western equatorial Pacific Ocean suggests that changes of the GAD intensity control the relative contribution of the persistent nondipole components and produces the inclination variation.