scholarly journals Reading runes with the sun. A geosemiotic analysis of the Rök runestone

2021 ◽  
pp. 263497952110591
Author(s):  
Per Holmberg

In the field of runestone research, the importance of multimodal understanding has been downplayed although it is obvious that several semiotic resources interact when it comes to carving a stone and erecting it in the landscape. This study examines if it is possible to deal with the methodological challenges of a historical material and make a multimodal approach deepen our understanding of the Rök runestone, one of the most famous and enigmatic Viking Age runestones. The study applies Scollon and Scollon’s geosemiotic framework (2003). Through an investigation of how the visual semiotics interacts with place semiotics and interaction order, it turns out that the marked reading direction of the lines of the inscription symbolizes the movement of the sun, and that the change of font size in two lines probably mimics the change of solar brightness at sunrise and sunset. Further, it is suggested that the big crosses of cipher runes and the small crosses between some information units may represent the sun and stars, respectively. The conclusion is that the monument was risen for the enactment of a counsel of the gods with the aim of securing the rhythm of celestial light. Finally, implications for multimodal research are discussed.

Author(s):  
Daniel J. Chapman ◽  
Diego A. Arias

Solar brightness profiles were used to model the optical performance of a parabolic linear solar concentrator. A sensitivity analysis of the sun size on collector performance was completed using analytical methods. Ray traces were created for solar brightness profiles having circumsolar ratios from 0–40%, slope errors of the optical surface from 2–5 mrads, and angles of incidence varying from 0–60 degrees. Using typical meteorological data for two locations, the optical performance was calculated and averaged over a year. Intercept factors of these simulations were compared to simpler analytical models that cast the sun shape as a Gaussian function. Results showed that collector performance is relatively insensitive to solar profile, and that using a representative Gaussian solar profile will tend to underestimate collector performance compared to using exact weighted solar profiles by about 1%. This difference is within the uncertainty propagation of the intercept factor calculated with analytical methods.


Author(s):  
Julio Renato SÁEZ GALLARDO

El objetivo de este trabajo es proponer un Modelo holístico multimodal para una lectura crítica del racismo en la prensa escrita. Para ello, desde el Análisis Crítico del Discurso Multimodal (ACDM), usaremos como estrategia teórico-metodológica integradora las aportaciones de Teresa Velázquez (2011) y su modelo semiótico-discursivo; el modelo sociocognitivo de van Dijk (1990, 1997, 2003a, 2003b); el modelo de la semiótica visual de Kress y van Leeuwen (1996) y el modelo intersemiótico de Nikolajeva y Scott (2001). Se validarán las matrices de análisis aplicándolas al llamado conflicto mapuche en Chile para extraer resultados y conclusiones valederas en torno a la representación periodística de las minorías étnicas. Abstract: This work aims to propose a holistic multimodal approach for making critical reading about racism in the written press. In order to achieve this, and taking account the Multimodal Critical Discourse Analysis, we use as theoretical and methodological integrative strategies the contributions of Teresa Velázquez and her discursive-semiotic approach (2011), van Dijk’s sociocognitive approach (1990, 1997a, 2003a, 2003b), Kress and van Leeuwen’s visual semiotics approach (1996), and Nikolakeva and Scott’s intersemiotic approach (2001). The analysis matrices are validated using the so-called mapuche conflict in Chile in order to be able to draw conclusive results and conclusions about media representations of ethnic minorities.


Author(s):  
Gísli Sigurðsson

The eddas and sagas are literary works written in Iceland in the 13th and 14th centuries but incorporating memories preserved orally from preliterate times of (a) Norse myths, in prose and verse form, (b) heroic lays with common Germanic roots, (c) raiding and trading voyages of the Viking Age (800–1030 CE), and (d) the settlement of Iceland from Norway, Britain, and Ireland starting from the 870s and of life in the new country up to and beyond the conversion to Christianity in the year 1000. In their writing, these works show the influence of the learning and literature introduced to Iceland from the 11th century on through the educational system of the medieval Church. During these centuries, the Icelanders translated the lives of the principal saints, produced saga biographies of their own bishops, and recorded accounts of events and conflicts contemporary with their authors. They also produced conventional chronicles on European models of the kings of Norway and Denmark and large quantities of works, both translated and original, in the spirit of medieval chivalry. The eddas and sagas, however, reflect a unique and original departure that has no direct analogue in mainland Europe—the creation of new works and genres rooted in the secular tradition of oral learning and storytelling. This tradition encompassed the Icelanders’ worldview in the 12th, 13th and 14th centuries and their understanding of events, people, and chronology going back to the 9th century, and their experience of an environment that extended over the parts of the world known to the Norsemen of the Viking Age, both on earth and in heaven. The infrastructure that underlay this system of learning was a knowledge of the regnal years of kings who employed court poets to memorialize their lives, and stories that were told in connection with what people observed in the heavens and on earth, near and far, by linking the stories with individual journeys, dwellings, and the genealogies of the leading protagonists. In this world, people here on earth envisaged the gods as having their halls and dwellings in the sky among the stars and the sun, while beyond the ocean and beneath the furthest horizon lay the world of the giants. In Viking times, this furthest horizon shifted little by little westwards, from the seas around Norway and Britain to the Faroes, Iceland, Greenland, and eventually still farther south and west to previously unknown lands that people in Iceland retained memories of the ancestors having discovered and explored around the year 1000—Helluland, Markland, and Vínland—where they came into contact with the native inhabitants of the continent known as North America.


2020 ◽  
Vol 636 ◽  
pp. A43 ◽  
Author(s):  
N.-E. Nèmec ◽  
A. I. Shapiro ◽  
N. A. Krivova ◽  
S. K. Solanki ◽  
R. V. Tagirov ◽  
...  

Context. Magnetic features on the surfaces of cool stars lead to variations in their brightness. Such variations on the surface of the Sun have been studied extensively. Recent planet-hunting space telescopes have made it possible to measure brightness variations in hundred thousands of other stars. The new data may undermine the validity of setting the sun as a typical example of a variable star. Putting solar variability into the stellar context suffers, however, from a bias resulting from solar observations being carried out from its near-equatorial plane, whereas stars are generally observed at all possible inclinations. Aims. We model solar brightness variations at timescales from days to years as they would be observed at different inclinations. In particular, we consider the effect of the inclination on the power spectrum of solar brightness variations. The variations are calculated in several passbands that are routinely used for stellar measurements. Methods. We employ the surface flux transport model to simulate the time-dependent spatial distribution of magnetic features on both the near and far sides of the Sun. This distribution is then used to calculate solar brightness variations following the Spectral And Total Irradiance REconstruction approach. Results. We have quantified the effect of the inclination on solar brightness variability at timescales down to a single day. Thus, our results allow for solar brightness records to be made directly comparable to those obtained by planet-hunting space telescopes. Furthermore, we decompose solar brightness variations into components originating from the solar rotation and from the evolution of magnetic features.


1955 ◽  
Vol 8 (4) ◽  
pp. 487 ◽  
Author(s):  
G Swarup ◽  
R Parthasarathy

A multiple-element interferometer has been employed to determine one-dimensional distributions of radio brightness over the quiet Sun at a wavelength of 60 cm for scanning directions varying from 90� to 60� with respect to the central meridian of the Sun. These observations have been compared with measurements by other workers at the same, or nearly the same, wavelength. The present observations are reasonably consistent with the two-dimensional brightness distribution derived recently by O'Brien and Tandberg-Hanssen with a two-aerial interferometer, but do not agree with the earlier results of Stanier at the same wavelength. The disagreement, largely the absence of the theoretically predicted limb-brightening in Stanier's results, may reflect actual changes in the Sun over the solar cycle. However, the possibility of localized disturbed regions affecting Stanier's results for the quiet Sun cannot be eliminated.


1958 ◽  
Vol 11 (3) ◽  
pp. 338 ◽  
Author(s):  
G Swarup ◽  
R Parthasarathy

The localized radio bright regions on the Sun which give rise to a slowly varying component of the solar radiation were studied at a wavelength of 60 cm, using a 32-aerial interferometer with a beamwidth of 8�7 min of arc. The observations were undertaken during July 1954 to March 1955 and were limited in number due to this being a minimum period of the solar cycle. The low activity, however, provided the advantage of simple interpretation as often only one region was present on the solar disk.


2011 ◽  
Vol 11 (2) ◽  
pp. 141-163 ◽  
Author(s):  
Karen E. Wohlwend ◽  
Sarah Vander Zanden ◽  
Nicholas E. Husbye ◽  
Candace R. Kuby

Geosemiotics (Scollon and Scollon, 2003) frames this analysis of play, multimodal collaboration, and peer mediation as players navigate barriers to online connectivity in a children’s social network and gaming site. A geosemiotic perspective enables examination of children’s web play as discourses in place: fluidly converging and diverging interactions among four factors: (1) social actors, (2) interaction order, (3) visual semiotics, and (4) place semiotics. The video data are excerpted from an ethnographic study of a computer club for primary school-aged children in an afterschool program serving working-class and middle-class families in a US Midwest university community. Discourses of schooling in the computer room and Webkinz complicated children’s goal of coordinated game play and mutual participation in online games. Barriers to online connection produced ruptures that foregrounded childrens’ collaborative management of time and space. This foregrounding makes typically backgrounded practices, modes, and discourses visible and available for deconstruction and critique.


2000 ◽  
Vol 3 (1) ◽  
pp. 57-67
Author(s):  
Emília Pásztor ◽  
Curt Roslund ◽  
Britt-Mari Näsström ◽  
Heather Robertson

A well-built roadway from the early Viking Age at the Rösaring archaeological site in central Sweden is assumed by archaeologists to have been used for processions. The road is here examined in relation to its environment, the sun and the moon, the Milky Way and the rainbow. The aim was to extend landscape archaeology to include natural phenomena and their impact on prehistoric monuments as an aid to conventional archaeology. The play of sunlight over the road at noon was found to be particularly spectacular at midwinter and well-suited for enhancing the performance of rites which could have taken place at a large mound at the south end of the road, possibly in connection with the cult of the Norse fertility god Freyr.


1966 ◽  
Vol 24 ◽  
pp. 40-43
Author(s):  
O. C. Wilson ◽  
A. Skumanich

Evidence previously presented by one of the authors (1) suggests strongly that chromospheric activity decreases with age in main sequence stars. This tentative conclusion rests principally upon a comparison of the members of large clusters (Hyades, Praesepe, Pleiades) with non-cluster objects in the general field, including the Sun. It is at least conceivable, however, that cluster and non-cluster stars might differ in some fundamental fashion which could influence the degree of chromospheric activity, and that the observed differences in chromospheric activity would then be attributable to the circumstances of stellar origin rather than to age.


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