Show simple item record

dc.contributor.authorUgalde, H.
dc.contributor.authorMorris, W. A.
dc.contributor.authorClark, C.
dc.contributor.authorMiles, B.
dc.contributor.authorMilkereit, B.
dc.date.accessioned2021-02-12T22:54:25Z
dc.date.available2021-02-12T22:54:25Z
dc.date.issued2007-01-01
dc.identifier.citationUgalde, H., Morris, W. A., Clark, C., Miles, B., & Milkereit, B. (2007). The Lake Bosumtwi meteorite impact structure, Ghana—A magnetic image from a third observational level. Meteoritics & Planetary Science, 42(4‐5), 793-800.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2007.tb01075.x
dc.identifier.urihttp://hdl.handle.net/10150/656706
dc.description.abstractThe Bosumtwi impact structure in Ghana is the youngest and best-preserved medium-sized impact structure on Earth, and because of the vast amount of prior geophysical and geological data gathered in the area, it constitutes a great natural laboratory to try to develop new geophysical interpretation and modeling techniques. During the 2004 International Continental Scientific Drilling Program (ICDP) drilling campaign at Lake Bosumtwi, we made magnetic field observations at 162 stations around the lake. This study differs from all previous magnetic surveys at Bosumtwi, which only measured the scalar portion of the Earth’s magnetic field, in that we measured the full magnetic vector at each station. Acquisition of the full magnetic vector was made possible by innovative use of a borehole deviation probe, which uses a magnetic sensor for absolute orientation reference. Estimates of the magnetic vector orientation and magnitude at each observation station were derived from a series of measurements collected at 50 cm spacing over a depth range of 25 m. In this study, we report a comparison between the scalar total field intensity derived from this new survey approach with the other two previously acquired marine and airborne magnetic data sets. The scalar total magnetic intensity (TMI) computed from the vector data set compares in close agreement with the other two data sets. Some discrepancies between the data sets can be explained by differences in the distances between the sensor and the magnetic sources for the various surveys. The highlight of this study is that we demonstrate that is possible to acquire at least partial vector data with readily available instrumentation.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectgeophysical signature
dc.subjectMagnetism
dc.subjectBosumtwi Ghana impact crater
dc.titleThe Lake Bosumtwi meteorite impact structure, Ghana—A magnetic image from a third observational level
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume42
dc.source.issue4-5
dc.source.beginpage793
dc.source.endpage800
refterms.dateFOA2021-02-12T22:54:25Z


Files in this item

Thumbnail
Name:
azu_meteoritics_v42_n4-5_793_8 ...
Size:
3.986Mb
Format:
PDF

This item appears in the following Collection(s)

Show simple item record