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A modified R(1)circle times R(1) method for helioseismic rotation inversions
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1996 (English)In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, Vol. 279, no 2, 498-510 p.Article in journal (Refereed) Published
Abstract [en]

We present an efficient method for two-dimensional (2D) inversions for the solar rotation rate using the Subtractive Optimally Localized Averages (SOLA) method and a modification of the R(1) x R(1) technique proposed by Sekii. The SOLA method is based on

Place, publisher, year, edition, pages
BLACKWELL SCIENCE LTD , 1996. Vol. 279, no 2, 498-510 p.
Keyword [en]
methods; numerical; Sun; interior; Sun; oscillations; Sun; rotation; STRATEGY
URN: urn:nbn:se:uu:diva-85376OAI: oai:DiVA.org:uu-85376DiVA: diva2:113284
Addresses: ASTRON OBSERV, S-75120 UPPSALA, SWEDEN. UNIV LONDON QUEEN MARY & WESTFIELD COLL, ASTRON UNIT, LONDON E1 4NS, ENGLAND.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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