Magnetic fields in the solar nebula may have played a key role in the radial transport of
angular momentum and mass during the early accretional phase of the solar system …

Magnetic fields in the solar nebula may have played a central role in mass and angular
momentum transport in the protosolar disk and facilitated the accretion of the first …

The textures of chondritic meteorites demonstrate that they are not the products of planetary
melting processes. This has long been interpreted as evidence that chondrite parent bodies …

Paleomagnetic studies of chondritic meteorites in recent years have revealed strong
magnetic fields in the protoplanetary disk, suggesting amplification through …

Chondritic meteorites have been traditionally thought to be samples of undifferentiated
bodies that never experienced large-scale melting. This view has been challenged by the …

The magnetic properties of eleven ordinary chondrites (eight LL-chondrites and three L-
chondrites) have been analysed. The samples were repeatedly fragmented and oriented to …

Introduction: Thermal and aqueous alteration are common occurrences in the lifetime of
carbonaceous chondrites. These alteration processes must be well understood in order to …

Several chondritic meteorites contain magnetizations that have been attributed to either
solar nebula fields or to core dynamos that may have operated within partially differentiated …

The study of the paleomagnetism of carbonaceous chondrites can lead to an estimate of the
magnetic fields present in the early solar system. CM chondrites contain abundant magnetite …

The origin of magnetization in Allende may have significant implications for our
understanding of core formation/differentiation/dynamo processes in chondrite parent …