An inquiry into the lunar interior: A nonlinear inversion of the Apollo lunar seismic data
This study discusses in detail the inversion of the Apollo lunar seismic data and the question of how to analyze the results. The well-known problem of estimating structural parameters (seismic velocities) and other parameters crucial to an understanding of a planetary body from a set of arrival...
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| Format: | Article |
| Language: | English |
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American Geophysical Union.
2002
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| Online Access: | http://ir.unimas.my/id/eprint/9774/ http://ir.unimas.my/id/eprint/9774/1/An%20inquiry%20into%20the%20lunar%20interior%20A%20nonlinear%20inversion%20of%20the%20Apollo%20lunar%20seismic%20data%20%28abstract%29.pdf |
| _version_ | 1848836635572043776 |
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| author | Adnan, Shahid Khan Klaus, Mosegaard |
| author_facet | Adnan, Shahid Khan Klaus, Mosegaard |
| author_sort | Adnan, Shahid Khan |
| building | UNIMAS Institutional Repository |
| collection | Online Access |
| description | This study discusses in detail the inversion of the Apollo lunar seismic data and the
question of how to analyze the results. The well-known problem of estimating structural
parameters (seismic velocities) and other parameters crucial to an understanding of a
planetary body from a set of arrival times is strongly nonlinear. Here we consider this
problem from the point of view of Bayesian statistics using a Markov chain Monte Carlo
method. Generally, the results seem to indicate a somewhat thinner crust with a thickness
around 45 km as well as a more detailed lunar velocity structure, especially in the middle
mantle, than obtained in earlier studies. Concerning the moonquake locations, the shallow
moonquakes are found in the depth range 50–220 km, and the majority of deep
moonquakes are concentrated in the depth range 850–1000 km, with what seems to be an
apparently rather sharp lower boundary. In wanting to further analyze the outcome of the
inversion for specific features in a statistical fashion, we have used credible intervals, twodimensional
marginals, and Bayesian hypothesis testing. Using this form of hypothesis
testing, we are able to decide between the relative importance of any two hypotheses given
data, prior information, and the physical laws that govern the relationship between model
and data, such as having to decide between a thin crust of 45 km and a thick crust as
implied by the generally assumed value of 60 km. We obtain a Bayes factor of 4.2,
implying that a thinner crust is strongly favored. |
| first_indexed | 2025-11-15T06:26:54Z |
| format | Article |
| id | unimas-9774 |
| institution | Universiti Malaysia Sarawak |
| institution_category | Local University |
| language | English |
| last_indexed | 2025-11-15T06:26:54Z |
| publishDate | 2002 |
| publisher | American Geophysical Union. |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | unimas-97742015-11-18T08:14:59Z http://ir.unimas.my/id/eprint/9774/ An inquiry into the lunar interior: A nonlinear inversion of the Apollo lunar seismic data Adnan, Shahid Khan Klaus, Mosegaard G Geography (General) This study discusses in detail the inversion of the Apollo lunar seismic data and the question of how to analyze the results. The well-known problem of estimating structural parameters (seismic velocities) and other parameters crucial to an understanding of a planetary body from a set of arrival times is strongly nonlinear. Here we consider this problem from the point of view of Bayesian statistics using a Markov chain Monte Carlo method. Generally, the results seem to indicate a somewhat thinner crust with a thickness around 45 km as well as a more detailed lunar velocity structure, especially in the middle mantle, than obtained in earlier studies. Concerning the moonquake locations, the shallow moonquakes are found in the depth range 50–220 km, and the majority of deep moonquakes are concentrated in the depth range 850–1000 km, with what seems to be an apparently rather sharp lower boundary. In wanting to further analyze the outcome of the inversion for specific features in a statistical fashion, we have used credible intervals, twodimensional marginals, and Bayesian hypothesis testing. Using this form of hypothesis testing, we are able to decide between the relative importance of any two hypotheses given data, prior information, and the physical laws that govern the relationship between model and data, such as having to decide between a thin crust of 45 km and a thick crust as implied by the generally assumed value of 60 km. We obtain a Bayes factor of 4.2, implying that a thinner crust is strongly favored. American Geophysical Union. 2002 Article NonPeerReviewed text en http://ir.unimas.my/id/eprint/9774/1/An%20inquiry%20into%20the%20lunar%20interior%20A%20nonlinear%20inversion%20of%20the%20Apollo%20lunar%20seismic%20data%20%28abstract%29.pdf Adnan, Shahid Khan and Klaus, Mosegaard (2002) An inquiry into the lunar interior: A nonlinear inversion of the Apollo lunar seismic data. Journal Of Geophysical Research, 107 (E6). ISSN 0148-0227 DOI: 10.1029/2001JE001658 |
| spellingShingle | G Geography (General) Adnan, Shahid Khan Klaus, Mosegaard An inquiry into the lunar interior: A nonlinear inversion of the Apollo lunar seismic data |
| title | An inquiry into the lunar interior: A nonlinear inversion
of the Apollo lunar seismic data |
| title_full | An inquiry into the lunar interior: A nonlinear inversion
of the Apollo lunar seismic data |
| title_fullStr | An inquiry into the lunar interior: A nonlinear inversion
of the Apollo lunar seismic data |
| title_full_unstemmed | An inquiry into the lunar interior: A nonlinear inversion
of the Apollo lunar seismic data |
| title_short | An inquiry into the lunar interior: A nonlinear inversion
of the Apollo lunar seismic data |
| title_sort | inquiry into the lunar interior: a nonlinear inversion
of the apollo lunar seismic data |
| topic | G Geography (General) |
| url | http://ir.unimas.my/id/eprint/9774/ http://ir.unimas.my/id/eprint/9774/ http://ir.unimas.my/id/eprint/9774/1/An%20inquiry%20into%20the%20lunar%20interior%20A%20nonlinear%20inversion%20of%20the%20Apollo%20lunar%20seismic%20data%20%28abstract%29.pdf |