FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1490560422> ?p ?o ?g. }

• W1490560422 abstract "[1] Building on Robert Morris's (1990) research on hexachordal ZC-relations, Stephen Soderberg (1998) identifies a constellation of ten hexachords that embed either one diminished seventh chord or two diminished triads. Soderberg divides the constellation, called MORRIS (or T-HEX), into four overlapping eight-hexachord sub-constellations based on tetrachordal subset content. The first of these sub-constellations, TRISTAN, includes the hexachords that embed two instances of set class 4-27[0258], the set class of the major-minor and half-diminished seventh chords. Similarly, constellations ZAUBER, AGITATION, and BROODING include the hexachords that embed two instances of set classes 4-18[0147], 4-13[0136], and 4-12[0236], respectively. Soderberg characterizes each of these tetrachordal set types as a of the diminished seventh chord. When the w, is 1, the result is set class 4-27-that is, moving any pc of a diminished seventh chord by interval class (ic) 1 creates a member of set class 4-27. Similarly, setting w = 2, 4, and 5 creates set classes 4-18, 4-13, and 4-12, respectively. The article goes on to point out a general property of voice leading: in each hexachord the pair of tetrachords can be connected by holding two pitch classes in common and by moving two others by ±w. The cases involving 4-27 and ic 1 voice leading (TRISTAN) are familiar-ii-V7,the Tristan chord with resolution, A7-B7at the beginning of Debussy's Faune, and others-and have been addressed in the theoretic literature by several authors.(1) Example 1 presents the MORRIS constellation and its four overlapping sub-constellations, henceforth called MORRIS1,MORRIS2,MORRIS4,and MORRIS5,with each subscript indicating the warp index, w.Example 1. The MORRIS Constellation (after Soderberg 1998)[2] Taking Soderberg's MORRIS constellation as a starting point, this study explores a wide variety of voice-leading transformations involving set types 4-27, 4-18, 4-13, and 4-12. It starts with the tetrachordal voice-leading transformations that produce the MORRISwhexachords-the nine ways that a tetrachord may be connected to another in the same set class by holding two pitch classes in common and by moving two others by ±w. (For each value of w there are nine transformations but only eight hexachord types because two of the transformations yield the same hexachord type.) The article then greatly expands the scope of inquiry, not only by allowing a given tetrachord to connect to any member of the same set class, but also by considering all twenty-four ways to voice-lead each of these twenty-four tetrachordal connections. As a result, each of these much larger voice-leading spaces-MORRIS+1,MORRIS+2,MORRIS+4,and MORRIS+5-contains 576 (= 24 × 24) voice-leading transformations. Each MORRISwis a subset of its corresponding MORRIS+w.[3] The paper provides an organized view of the entire MORRISw/MORRIS+wsystem, but it also develops other voice-leading spaces within MORRISw/MORRIS+w,each of which involves only a few of the MORRISw/MORRIS+wvoice-leading transformations. The additional voice-leading spaces usually also include rules for requiring, preferring, allowing, or forbidding one transformation to follow another. Although the number of potential voice-leading spaces is infinite,(2) my reasons for creating the ones I do are simple-to exercise melodic control over intervallic characteristics of the voices and to exercise harmonic control, not only of the individual tetrachords, but over the total pc content of sets of adjacent tetrachords. For example, in one space defined below a set of six MORRIS5voice-leading transformations can be concatenated in any order but remain within a single octatonic collection, in another space four MORRIS+4transformations are strung together so that one voice descends chromatically while the other voices also move stepwise, and in a third example ten MORRIS+2transformations are arranged so that each voice is saturated with a different interval class. …" @default.
• W1490560422 created "2016-06-24" @default.
• W1490560422 creator A5048634662 @default.
• W1490560422 date "2011-12-01" @default.
• W1490560422 modified "2023-09-23" @default.
• W1490560422 title "Exploring Tetrachordal Voice-Leading Spaces Within and Around the MORRIS Constellation" @default.
• W1490560422 cites W1585059742 @default.
• W1490560422 cites W1971488087 @default.
• W1490560422 cites W1974094366 @default.
• W1490560422 cites W1983389294 @default.
• W1490560422 cites W1987789864 @default.
• W1490560422 cites W1990014647 @default.
• W1490560422 cites W1990244325 @default.
• W1490560422 cites W1998790503 @default.
• W1490560422 cites W1999258801 @default.
• W1490560422 cites W2004886102 @default.
• W1490560422 cites W2008354687 @default.
• W1490560422 cites W2015528565 @default.
• W1490560422 cites W2025455396 @default.
• W1490560422 cites W2025518365 @default.
• W1490560422 cites W2028352550 @default.
• W1490560422 cites W2030499578 @default.
• W1490560422 cites W2034596905 @default.
• W1490560422 cites W2036576183 @default.
• W1490560422 cites W2043453567 @default.
• W1490560422 cites W2044225040 @default.
• W1490560422 cites W2070520568 @default.
• W1490560422 cites W2075435139 @default.
• W1490560422 cites W2100459483 @default.
• W1490560422 cites W2129405468 @default.
• W1490560422 cites W2150117890 @default.
• W1490560422 cites W2277819535 @default.
• W1490560422 cites W2295517378 @default.
• W1490560422 cites W2335421503 @default.
• W1490560422 cites W2338250689 @default.
• W1490560422 cites W2549330885 @default.
• W1490560422 cites W2560389497 @default.
• W1490560422 cites W4247679155 @default.
• W1490560422 cites W4252464960 @default.
• W1490560422 cites W4323765029 @default.
• W1490560422 doi "https://doi.org/10.30535/mto.17.4.2" @default.
• W1490560422 hasPublicationYear "2011" @default.
• W1490560422 type Work @default.
• W1490560422 sameAs 1490560422 @default.
• W1490560422 citedByCount "1" @default.
• W1490560422 countsByYear W14905604222018 @default.
• W1490560422 crossrefType "journal-article" @default.
• W1490560422 hasAuthorship W1490560422A5048634662 @default.
• W1490560422 hasBestOaLocation W14905604221 @default.
• W1490560422 hasConcept C121332964 @default.
• W1490560422 hasConcept C1276947 @default.
• W1490560422 hasConcept C142362112 @default.
• W1490560422 hasConcept C15744967 @default.
• W1490560422 hasConcept C46312422 @default.
• W1490560422 hasConcept C70352696 @default.
• W1490560422 hasConceptScore W1490560422C121332964 @default.
• W1490560422 hasConceptScore W1490560422C1276947 @default.
• W1490560422 hasConceptScore W1490560422C142362112 @default.
• W1490560422 hasConceptScore W1490560422C15744967 @default.
• W1490560422 hasConceptScore W1490560422C46312422 @default.
• W1490560422 hasConceptScore W1490560422C70352696 @default.
• W1490560422 hasIssue "4" @default.
• W1490560422 hasLocation W14905604221 @default.
• W1490560422 hasOpenAccess W1490560422 @default.
• W1490560422 hasPrimaryLocation W14905604221 @default.
• W1490560422 hasRelatedWork W2077616253 @default.
• W1490560422 hasRelatedWork W2758277628 @default.
• W1490560422 hasRelatedWork W2899084033 @default.
• W1490560422 hasRelatedWork W2912350827 @default.
• W1490560422 hasRelatedWork W2935909890 @default.
• W1490560422 hasRelatedWork W2948807893 @default.
• W1490560422 hasRelatedWork W3173606202 @default.
• W1490560422 hasRelatedWork W3183948672 @default.
• W1490560422 hasRelatedWork W2778153218 @default.
• W1490560422 hasRelatedWork W3110381201 @default.
• W1490560422 hasVolume "17" @default.
• W1490560422 isParatext "false" @default.
• W1490560422 isRetracted "false" @default.
• W1490560422 magId "1490560422" @default.
• W1490560422 workType "article" @default.