The Other Psalm Singing: Biblical Training in the Catholic Petites Écoles during the Late Renaissance

Keyword(s):  
Author(s):  
B.O. Stetsiuk

This article systemizes the types of musical improvisation according to various approaches to this phenomenon. It uses as the basis the classification by Ernst Ferand, which presently needs to be supplemented and clarified. It was stressed that the most general approach to the phenomenon of musical improvisation is its classification based on the layer principle (folklore, academic music, “third” layer). Within these layers, there are various forms of musical improvisation whose systemization is based on different principles, including: performer composition (collective or solo improvisation), process technology (full or partial improvisation), thematic orientation (improvisation theme in a broad and narrow context), etc. It was emphasized that classification of musical improvisation by types is manifested the most vividly when exemplified by jazz, which sums up the development of its principles and forms that shaped up in the previous eras in various regions of the world and have synthetized in the jazz language, which today reflects the interaction between such fundamental origins of musical thought as improvisation and composition. It was stated that the basic principles for classification of the types of musical improvisation include: 1) means of improvisation (voices; keyboard, string, wind and percussion instruments); 2) performer composition (solo or collective improvisation); 3) textural coordinates (vertical, horizontal, and melodic or harmonic improvisation, respectively); 4) performance technique (melodic ornaments, coloring, diminutiving, joining voices in the form of descant, organum, counterpoint); 5) scale of improvisation (absolute, relative; total, partial); 6) forms of improvisation: free, related; ornamental improvisation, variation, ostinato, improvisation on cantus firmus or another preset material (Ernst Ferand). It was stressed that as of today, the Ferand classification proposed back in 1938 needs to be supplemented by a number of new points, including: 1) improvisation of a mixed morphological type (music combined with dance and verbal text in two versions: a) invariable text and dance rhythm, b) a text and dance moves that are also improvised); 2) “pure” musical improvisation: vocal, instrumental, mixed (S. Maltsev). The collective form was the genetically initial form of improvisation, which included all components of syncretic action and functioned within the framework of cult ritual. Only later did the musical component per se grow separated (autonomous), becoming self-sufficient but retaining the key principle of dialogue that helps reproduce the “question-answer” system in any types of improvisation – a system that serves as the basis for creation of forms in the process of improvisation. Two more types of improvisation occur on this basis, differing from each other by communication type (Y. Lotman): 1) improvisation “for oneself” (internal type, characterized by reclusiveness and certain limitedness of information); 2) improvisation “for others” (external type, characterized by informational openness and variegation). It was emphasized that solo improvisation represents a special variety of musical improvisation, which beginning from the Late Renaissance era becomes dominating in the academic layer, distinguishable in the initial phase of its development for an improvising writing dualism (M. Saponov). The classification criterion of “composition” attains a new meaning in the system of professional music playing, to which improvisation also belongs. Its interpretation becomes dual and applies to the performance and textural components of improvisation, respectively. With regard to the former, two types occur in the collective form of improvisation: 1) improvisation by all participants (simultaneous or consecutive); 2)improvisation by a soloist against the background of invariable fixed accompaniment in other layers of music performance. The following types of improvisation occur in connection with the other – textural – interpretation of the term “composition”, which means inner logical principle of organization of musical fabric (T. Bershadska): 1) monodic, or monophonic (all cases of solo improvisation by voice or on melodic wind instruments); 2) heterophonic (collective improvisation based on interval duplications and variations of the main melody); 3) polyphonic (different-picture melodies in party voices of collective improvisation); 4) homophonic-harmonic (a combination of melodic and harmonic improvisations, typical for the playing on many-voiced harmonic instruments). It was emphasized that in the theory of musical improvisation, there is a special view at texture: on the one hand, it (like in a composition) “configures” (E. Nazaikinskyi) the musical fabric, and on the other hand, it is not a final representation thereof, i.e., it does not reach the value of Latin facio (“what has been done”). A work of improvisation is not an amorphous musical fabric; on the contrary, it contains its own textural organization, which, unlike a written composition, is distinguishable for the mobility and variability of possible textural solutions. The article’s concluding remarks state that classification of the types of musical improvisation in the aspect of its content and form must accommodate the following criteria: 1) performance type (voices, instruments, performance method, composition of participants, performance location); 2) texture type (real acoustic organization of musical space in terms of vertical, horizontal and depth parameters); 3) thematic (in the broad and narrow meanings of this notion: from improvisation on “idea theme” or “image theme” to variation improvisations on “text theme”, which could be represented by various acoustic structures: modes, ostinato figures of various types, melody themes like jazz evergreens, harmonic sequences, etc.).


2019 ◽  
Vol 16 (4) ◽  
pp. 41-77
Author(s):  
Petr Pavlas ◽  

The article picks up the threads of especially Martin Muslow’s 1990s research and describes the distinctiveness of the “relational metaphysics of resemblance” in the middle of the seventeenth century. The late Renaissance metaphysical outlines, carried out in the Comenius circle, are characteristic for their relationality, accent on universal resemblance, providentialism, pansensism, sensualism, triadism – and also for their effort to define metaphysical terms properly. While Comenians share the last – and only the last – feature with Cartesians, they differ in the other features. Therefore, Cartesians and Comenians cannot come to terms in the issue of the proper definitions either. Quite on the contrary, they oppose each other on this issue. By means of Johann Clauberg’s criticism of Georg Ritschel and René Descartes’s only supposedly “mysterious” and “solipsist” second meditation, the article turns a Cartesian mirror to the Comenian metaphysical project. In its light, the definitions of Georg Ritschel, Johann Heinrich Bisterfeld and Jan Amos Comenius turn out to be unacceptable for Cartesians (and also for Thomists and, in part, for Baconians). Despite their superficially Aristotelian-scholastic appearance, their content is notably Paracelsian-Campanellian (with a Timplerian foundation). Even though Comenian definitions of metaphysical terms had been refused and refuted by Cartesians, they experienced a second lifespan in their robust influence on Leibniz and Newton.


Author(s):  
Alexander B. Haskell

This book resituates the beginnings of English colonization in America in a Renaissance and post-Reformation context in which providential thought and conceptualizations of sovereignty were complexly entwined. Fearful that God resented the timidity with which English monarchs brandished their divinely granted power, colonizers encouraged a bold reimagining of royal duties as extending across the vast Atlantic. At the same time, they theorized colonization as a calling to which all resolute Christians were lawfully bound, thus setting into motion a Virginian colonizing enterprise in which planters, even more than monarchs themselves, determined the contours of licit conduct on the other side of the ocean. In reconstructing the evolution of the Virginia venture from the era of Elizabethan captains to the Jacobean Virginia Company to the seventeenth-century politics of forging an English commonwealth in the New World, the book recovers especially the extent to which American colonization emerged from the same late Renaissance search for an enduring basis for civil polity that would also spur Thomas Hobbes to formulate his revolutionary idea of the sovereign state. Yet, Hobbes's notion of state sovereignty was a distinctly late arrival in the history of English colonization in America. As a result, Virginia's commonwealth set a precedent for colonies that treated their own civil integrity as comparable to that of the kingdom from which they had sprung.


Author(s):  
Laurence Simmons

This essay brings together two paintings that on the surface seem to have very little in common: one dates from 1528–29 (The Visitation by the Italian late Renaissance painter Jacopo Carucci, better known as Pontormo after his birthplace), the other from 1968 (Visible Mysteries no. 8 by Colin McCahon). They are brought together here because they share the same subject matter: the central Catholic doctrine of the Incarnation, the mystery of God’s word becoming flesh, and the belief that divine and human natures are united. These two paintings can, in both similar and different ways, teach us something about the visible mystery that is painting.


1988 ◽  
Vol 62 (03) ◽  
pp. 411-419 ◽  
Author(s):  
Colin W. Stearn

Stromatoporoids are the principal framebuilding organisms in the patch reef that is part of the reservoir of the Normandville field. The reef is 10 m thick and 1.5 km2in area and demonstrates that stromatoporoids retained their ability to build reefal edifices into Famennian time despite the biotic crisis at the close of Frasnian time. The fauna is dominated by labechiids but includes three non-labechiid species. The most abundant species isStylostroma sinense(Dong) butLabechia palliseriStearn is also common. Both these species are highly variable and are described in terms of multiple phases that occur in a single skeleton. The other species described areClathrostromacf.C. jukkenseYavorsky,Gerronostromasp. (a columnar species), andStromatoporasp. The fauna belongs in Famennian/Strunian assemblage 2 as defined by Stearn et al. (1988).


1967 ◽  
Vol 28 ◽  
pp. 207-244
Author(s):  
R. P. Kraft

(Ed. note:Encouraged by the success of the more informal approach in Christy's presentation, we tried an even more extreme experiment in this session, I-D. In essence, Kraft held the floor continuously all morning, and for the hour and a half afternoon session, serving as a combined Summary-Introductory speaker and a marathon-moderator of a running discussion on the line spectrum of cepheids. There was almost continuous interruption of his presentation; and most points raised from the floor were followed through in detail, no matter how digressive to the main presentation. This approach turned out to be much too extreme. It is wearing on the speaker, and the other members of the symposium feel more like an audience and less like participants in a dissective discussion. Because Kraft presented a compendious collection of empirical information, and, based on it, an exceedingly novel series of suggestions on the cepheid problem, these defects were probably aggravated by the first and alleviated by the second. I am much indebted to Kraft for working with me on a preliminary editing, to try to delete the side-excursions and to retain coherence about the main points. As usual, however, all responsibility for defects in final editing is wholly my own.)


1967 ◽  
Vol 28 ◽  
pp. 177-206
Author(s):  
J. B. Oke ◽  
C. A. Whitney

Pecker:The topic to be considered today is the continuous spectrum of certain stars, whose variability we attribute to a pulsation of some part of their structure. Obviously, this continuous spectrum provides a test of the pulsation theory to the extent that the continuum is completely and accurately observed and that we can analyse it to infer the structure of the star producing it. The continuum is one of the two possible spectral observations; the other is the line spectrum. It is obvious that from studies of the continuum alone, we obtain no direct information on the velocity fields in the star. We obtain information only on the thermodynamic structure of the photospheric layers of these stars–the photospheric layers being defined as those from which the observed continuum directly arises. So the problems arising in a study of the continuum are of two general kinds: completeness of observation, and adequacy of diagnostic interpretation. I will make a few comments on these, then turn the meeting over to Oke and Whitney.


1966 ◽  
Vol 24 ◽  
pp. 337
Author(s):  
W. Iwanowska

A new 24-inch/36-inch//3 Schmidt telescope, made by C. Zeiss, Jena, has been installed since 30 August 1962, at the N. Copernicus University Observatory in Toruń. It is equipped with two objective prisms, used separately, one of crown the other of flint glass, each of 5° refracting angle, giving dispersions of 560Å/mm and 250Å/ mm respectively.


2020 ◽  
Vol 43 ◽  
Author(s):  
Philip Pettit

Abstract Michael Tomasello explains the human sense of obligation by the role it plays in negotiating practices of acting jointly and the commitments they underwrite. He draws in his work on two models of joint action, one from Michael Bratman, the other from Margaret Gilbert. But Bratman's makes the explanation too difficult to succeed, and Gilbert's makes it too easy.


1999 ◽  
Vol 173 ◽  
pp. 249-254
Author(s):  
A.M. Silva ◽  
R.D. Miró

AbstractWe have developed a model for theH2OandOHevolution in a comet outburst, assuming that together with the gas, a distribution of icy grains is ejected. With an initial mass of icy grains of 108kg released, theH2OandOHproductions are increased up to a factor two, and the growth curves change drastically in the first two days. The model is applied to eruptions detected in theOHradio monitorings and fits well with the slow variations in the flux. On the other hand, several events of short duration appear, consisting of a sudden rise ofOHflux, followed by a sudden decay on the second day. These apparent short bursts are frequently found as precursors of a more durable eruption. We suggest that both of them are part of a unique eruption, and that the sudden decay is due to collisions that de-excite theOHmaser, when it reaches the Cometopause region located at 1.35 × 105kmfrom the nucleus.


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