Region Spherical Harmonic Magnetic Modeling from Near-Surface and Satellite-Altitude Anomlaies

The compiled near-surface data and satellite crustal magnetic measured data are modeled with a regionally concentrated spherical harmonic presentation technique over Australia and Antarctica. Global crustal magnetic anomaly studies have used a spherical harmonic analysis to represent the Earth'...

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Main Authors: von Frese, Ralph R. B., Kim, Hyung Rae, Taylor, Patrick T.
Format: Other/Unknown Material
Language:unknown
Published: 2013
Subjects:
Online Access:http://hdl.handle.net/2060/20140013360
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:20140013360 2023-05-15T13:59:55+02:00 Region Spherical Harmonic Magnetic Modeling from Near-Surface and Satellite-Altitude Anomlaies von Frese, Ralph R. B. Kim, Hyung Rae Taylor, Patrick T. Unclassified, Unlimited, Publicly available September 9, 2013 application/pdf http://hdl.handle.net/2060/20140013360 unknown Document ID: 20140013360 http://hdl.handle.net/2060/20140013360 Copyright, Distribution as joint owner in the copyright CASI Geosciences (General) GSFC-E-DAA-TN11100 ESA Living Planet Symposium 9-13 Sept. 2013; Edinburgh; United Kingdom 2013 ftnasantrs 2019-07-21T06:13:10Z The compiled near-surface data and satellite crustal magnetic measured data are modeled with a regionally concentrated spherical harmonic presentation technique over Australia and Antarctica. Global crustal magnetic anomaly studies have used a spherical harmonic analysis to represent the Earth's magnetic crustal field. This global approach, however is best applied where the data are uniformly distributed over the entire Earth. Satellite observations generally meet this requirement, but unequally distributed data cannot be easily adapted in global modeling. Even for the satellite observations, due to the errors spread over the globe, data smoothing is inevitable in the global spherical harmonic presentations. In addition, global high-resolution modeling requires a great number of global spherical harmonic coefficients for the regional presentation of crustal magnetic anomalies, whereas a lesser number of localized spherical coefficients will satisfy. We compared methods in both global and regional approaches and for a case where the errors were propagated outside the region of interest. For observations from the upcoming Swarm constellation, the regional modeling will allow the production a lesser number of spherical coefficients that are relevant to the region of interest Other/Unknown Material Antarc* Antarctica NASA Technical Reports Server (NTRS)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic Geosciences (General)
spellingShingle Geosciences (General)
von Frese, Ralph R. B.
Kim, Hyung Rae
Taylor, Patrick T.
Region Spherical Harmonic Magnetic Modeling from Near-Surface and Satellite-Altitude Anomlaies
topic_facet Geosciences (General)
description The compiled near-surface data and satellite crustal magnetic measured data are modeled with a regionally concentrated spherical harmonic presentation technique over Australia and Antarctica. Global crustal magnetic anomaly studies have used a spherical harmonic analysis to represent the Earth's magnetic crustal field. This global approach, however is best applied where the data are uniformly distributed over the entire Earth. Satellite observations generally meet this requirement, but unequally distributed data cannot be easily adapted in global modeling. Even for the satellite observations, due to the errors spread over the globe, data smoothing is inevitable in the global spherical harmonic presentations. In addition, global high-resolution modeling requires a great number of global spherical harmonic coefficients for the regional presentation of crustal magnetic anomalies, whereas a lesser number of localized spherical coefficients will satisfy. We compared methods in both global and regional approaches and for a case where the errors were propagated outside the region of interest. For observations from the upcoming Swarm constellation, the regional modeling will allow the production a lesser number of spherical coefficients that are relevant to the region of interest
format Other/Unknown Material
author von Frese, Ralph R. B.
Kim, Hyung Rae
Taylor, Patrick T.
author_facet von Frese, Ralph R. B.
Kim, Hyung Rae
Taylor, Patrick T.
author_sort von Frese, Ralph R. B.
title Region Spherical Harmonic Magnetic Modeling from Near-Surface and Satellite-Altitude Anomlaies
title_short Region Spherical Harmonic Magnetic Modeling from Near-Surface and Satellite-Altitude Anomlaies
title_full Region Spherical Harmonic Magnetic Modeling from Near-Surface and Satellite-Altitude Anomlaies
title_fullStr Region Spherical Harmonic Magnetic Modeling from Near-Surface and Satellite-Altitude Anomlaies
title_full_unstemmed Region Spherical Harmonic Magnetic Modeling from Near-Surface and Satellite-Altitude Anomlaies
title_sort region spherical harmonic magnetic modeling from near-surface and satellite-altitude anomlaies
publishDate 2013
url http://hdl.handle.net/2060/20140013360
op_coverage Unclassified, Unlimited, Publicly available
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source CASI
op_relation Document ID: 20140013360
http://hdl.handle.net/2060/20140013360
op_rights Copyright, Distribution as joint owner in the copyright
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