COLUMELLA 10.101: TWO EMENDATIONS

2020 ◽  
pp. 1-5
Author(s):  
Boris Kayachev
Keyword(s):  
The Other ◽  
Relevant Point

Columella invites his readers to plant different flowers, including violets—which will be the main focus of the following discussion (10.94–102): uerum ubi iam puro discrimine pectita tellus deposito squalore nitens sua semina poscet,     95 pangite tunc uarios, terrestria sidera, flores: candida leucoia et flauentia lumina caltae, narcissique comas et hiantis saeua leonis ora feri, calathisque uirentia lilia canis, necnon uel niueos uel caeruleos hyacinthos.     100 tum quae pallet humi, quae frondes purpurat auro, ponatur uiola, et nimium rosa plena pudoris. 96 pangite Heinsius: pingite SAR || 99 nitentia Gesner || 101 frondes SA: frondens R | purpurat auro ϛ: purpura tabo SAR: purpura et auro Ursinus: purpurat albo Heinsius This is the text of Rodgers's recent OCT, but with a somewhat modified apparatus criticus. For the purposes of my argument, it will be useful also to quote from the outset a related catalogue of melliferous flowers from another book of Columella's treatise (9.4.4): mille praeterea semina uel crudo caespite uirentia uel subacto sulco flores amicissimos apibus creant, ut sunt in uirgineo solo […] gladiolus narcissi. at in hortensi lira consita nitent candida lilia nec his sordidiora leucoia, tum Punicae rosae luteolaeque et Sarranae uiolae, nec minus caelestis luminis hyacinthus. There are a number of more general similarities, but the relevant point is that the two catalogues list many of the same flowers and describe them in similar ways, which means that one catalogue can serve as an interpretative guide to the other. The first two items in the prose list of garden flowers (nitent candida lilia nec his sordidiora leucoia) correspond to candida leucoia and calathisque uirentia lilia canis, similarly listed in the first half of the verse catalogue; nitent (lilia) can thus support Gesner's emendation nitentia for uirentia (lilia), unduly neglected by recent editors. The metaphoric periphrasis gladiolus narcissi can be compared with narcissique comas. Both texts describe the hyacinth as sky-blue, which seems to be otherwise unparalleled (nec minus caelestis luminis hyacinthus and necnon […] caeruleos hyacinthos: note also that in both cases the reference is introduced by a litotes). Finally, just like the prose list (tum Punicae rosae luteolaeque et Sarranae uiolae), Columella's poem groups roses with two varieties of violet (note also that both passages are introduced with tum): tum quae pallet humi, quae frondes purpurat auro, ponatur uiola, et nimium rosa plena pudoris. The prose version makes it all but certain that the poem should likewise refer to a yellow and a purple varieties of violet. While Columella's verse description of the former variety is fairly unambiguous (if not very informative), that of the latter raises questions.

scholarly journals Proper name-marking via liaison in French

2019 ◽  
Vol 72 (4) ◽  
pp. 627-652
Author(s):  
Natascha Pomino ◽  
Elisabeth Stark
Keyword(s):  
Empirical Studies ◽  
Proper Names ◽  
Noun Phrases ◽  
The Other ◽  
Linguistic Change ◽  
The Poor ◽  
Other Hand ◽  
Relevant Point ◽  
Proper Name ◽  
The One

Abstract The liaison consonant [z] in French noun phrases has traditionally been assumed to function as a plural marker. The realization of “plural [z]” in N(oun)-A(djective)-combinations is becoming, however, very rare in naturalistic data – except for contexts which allow a proper-name reading. On the one hand, one might think that we are dealing with a recent phenomenon, the beginning of a potential linguistic change in French in the sense of exaptation, reuse of former morphophonological material such as plural markers to signal proper-namehood in the sense of ‘frozen morphology’. If this turns out correct, we expect the productivity of the new synchronic function to increase: New NA-combinations which function as proper names should be realized systematically with liaison, and proper name-marking via liaison should also become possible with other liaison consonants. On the other hand, we may be dealing with a (completed) diachronic process, in that only those NA-combinations which allowed liaison at the relevant point in time may have a liaison consonant in their univerbalized form. That is, new NA-combinations, even though they are used as proper names, do not display a liaison consonant, because liaison is no longer possible. The purpose of this paper was to investigate, based on empirical studies, whether liaison productively marks NA-combinations which function as proper names and distinguishes them from NA-combinations that count as common nouns, or whether we are dealing with a completed diachronic process. In view of the poor productivity observed, we argue that we are dealing with cases of univerbation.

Les « superstitions » à l’épreuve de la modernité : un retour en grâce ?

2016 ◽  
Vol 63 (4) ◽  
pp. 497-512
Author(s):  
Lionel Obadia
Keyword(s):  
Point Of View ◽  
History Of Ideas ◽  
The Other ◽  
Relevant Point ◽  
History Of ◽  
Point Of Departure ◽  
Better Than

Have we finished with superstition, from the point of view of history, of ideas and of psychology? Nothing is less certain. On the basis of some ancient or recent publications on this topic, this article attempts to pinpoint the fact that, owing to the empirical and theoretical topicality of superstition, it certainly deserves better than the ideological and intellectual disqualification it has been subjected to. Recent reflections, inspired by anthropological and psychological approaches, seem part of a new interest in beliefs and symbols previously mastered by dominant and exclusive systems of thoughts, be they religious or profane. But a close examination of the effective uses of the notion of ‘superstition’ demonstrates that the projective stigmatization of the ‘Other’ remains a relevant point of departure from which it can be rehabilitated, alongside the latest psychological approaches of belief.

Stromatoporoids from the Famennian (Devonian) Wabamun Formation, Normandville oilfield, north–central Alberta, Canada

1988 ◽  
Vol 62 (03) ◽  
pp. 411-419 ◽  
Author(s):  
Colin W. Stearn
Keyword(s):  
Patch Reef ◽  
Abundant Species ◽  
The Other ◽  
North Central ◽  
Biotic Crisis

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).

D. The Line Spectrum of Pulsating Variable Stars

1967 ◽  
Vol 28 ◽  
pp. 207-244
Author(s):  
R. P. Kraft
Keyword(s):  
Variable Stars ◽  
The Other ◽  
Line Spectrum ◽  
Afternoon Session ◽  
Empirical Information ◽  
Pulsating Variable Stars ◽  
Almost Continuous ◽  
Informal Approach

(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.)

C. The Continuous Spectrum of Pulsating Variable Stars

1967 ◽  
Vol 28 ◽  
pp. 177-206
Author(s):  
J. B. Oke ◽  
C. A. Whitney
Keyword(s):  
Continuous Spectrum ◽  
Variable Stars ◽  
Velocity Fields ◽  
The Other ◽  
Line Spectrum ◽  
Direct Information ◽  
Thermodynamic Structure ◽  
Diagnostic Interpretation ◽  
Pulsating Variable Stars ◽  
The Continuum

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.

Observing programme for the 24-inch/36-inch Schmidt telescope

1966 ◽  
Vol 24 ◽  
pp. 337
Author(s):  
W. Iwanowska
Keyword(s):  
The Other ◽  
Schmidt Telescope ◽  
Flint Glass

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.

A hard choice for Tomasello

2020 ◽  
Vol 43 ◽  
Author(s):  
Philip Pettit
Keyword(s):  
Joint Action ◽  
The Other ◽  
Hard Choice ◽  
Margaret Gilbert ◽  
Michael Bratman ◽  
Human Sense ◽  
Sense Of Obligation

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.

A study of cometary eruptions through OH radio-lines

1999 ◽  
Vol 173 ◽  
pp. 249-254
Author(s):  
A.M. Silva ◽  
R.D. Miró
Keyword(s):  
Short Duration ◽  
Growth Curves ◽  
The Other ◽  
Initial Mass ◽  
Radio Lines ◽  
Other Hand ◽  
Sudden Rise

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.

Note on Selection of Coordinate Systems for Geodynamics

1975 ◽  
Vol 26 ◽  
pp. 395-407
Author(s):  
S. Henriksen
Keyword(s):  
Sea Level ◽  
The Other ◽  
Coordinate Systems ◽  
Mean Sea Level ◽  
The Earth ◽  
The One ◽  
Static Systems ◽  
Selection Of

The first question to be answered, in seeking coordinate systems for geodynamics, is: what is geodynamics? The answer is, of course, that geodynamics is that part of geophysics which is concerned with movements of the Earth, as opposed to geostatics which is the physics of the stationary Earth. But as far as we know, there is no stationary Earth – epur sic monere. So geodynamics is actually coextensive with geophysics, and coordinate systems suitable for the one should be suitable for the other. At the present time, there are not many coordinate systems, if any, that can be identified with a static Earth. Certainly the only coordinate of aeronomic (atmospheric) interest is the height, and this is usually either as geodynamic height or as pressure. In oceanology, the most important coordinate is depth, and this, like heights in the atmosphere, is expressed as metric depth from mean sea level, as geodynamic depth, or as pressure. Only for the earth do we find “static” systems in use, ana even here there is real question as to whether the systems are dynamic or static. So it would seem that our answer to the question, of what kind, of coordinate systems are we seeking, must be that we are looking for the same systems as are used in geophysics, and these systems are dynamic in nature already – that is, their definition involvestime.

Discussion of the Oblique Rotator Model Cases Of 108 Aqr and x Serp.

1976 ◽  
Vol 32 ◽  
pp. 577-588
Author(s):  
C. Mégessier ◽  
V. Khokhlova ◽  
T. Ryabchikova
Keyword(s):  
Mathematical Formulation ◽  
The Other ◽  
Rotator Model ◽  
Oblique Rotator ◽  
First Results

My talk will be on the oblique rotator model which was first proposed by Stibbs (1950), and since received success and further developments. I shall present two different attempts at describing a star according to this model and the first results obtained in the framework of a Russian-French collaboration in order to test the precision of the two methods. The aim is to give the best possible representation of the element distributions on the Ap stellar surfaces. The first method is the mathematical formulation proposed by Deutsch (1958-1970) and applied by Deutsch (1958) to HD 125248, by Pyper (1969) to α2CVn and by Mégessier (1975) to 108 Aqr. The other one was proposed by Khokhlova (1974) and used by her group.

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