scholarly journals ŚLADY WIERZEŃ POGAŃSKICH NA PRZYKŁADZIE ZNALEZISK Z OSTROWA LEDNICKIEGO

Author(s):  
DANUTA BANASZAK ◽  
ARKADIUSZ TABAKA

The article presents an analysis of finds and information attributed to the pre-Christian religion in Ostrów Lednicki and the ancillary facilities. To this end, a number of finds from the first half of the 10th to the early 12th centuries were described and interpreted. They include a piece of a gold amulet locket, a utensil made of clay with the swastika and an encircled cross, a buried horse, wooden horse figures, an ornamental element of a knife sheath ferrule, a round rattle and a wooden structure with cornerstone offerings. By means of comparative studies and analyses of the archaeological excavations in Ostrów Lednicki and its vicinity (Dziekanowice, Moraczewo), the authors conclude that in this area, a pagan cult centre could have existed in the late 9th and the early 10th centuries at the latest, related most probably to Svarog /Svarozic, god of the Sun, the home, and a divine blacksmith.

2010 ◽  
Vol 9 (1) ◽  
pp. 25-49 ◽  
Author(s):  
John Rose

Zodiac sun-gods on ancient synagogue mosaic floors have been discovered by archaeological excavations of sites in the Galilee and elsewhere in late antiquity Palestine. This was the period when the Roman Empire converted to Christianity – only to be followed by an attempt to restore pagan beliefs which the sun-god came to symbolise. One of these sites is located in the Roman Jewish city, Sepphoris. Its geographical and historical link to the Israeli-destroyed, Palestinian Galilee peasant village of Saffuriyya raises the further question of Arab historical claims on these ancient sites. Sun-god worship, its links to early Judaism, and its contribution to the evolution of the monotheistic religions of the Middle East will be examined.


2019 ◽  
Vol 3 (7) ◽  
pp. 95-114
Author(s):  
Rahim Velayati ◽  
Hamid Karamipour ◽  
Farzaneh Saadati Rad ◽  
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2021 ◽  
Vol 30 (1) ◽  
pp. 99-115
Author(s):  
Māra Pilmane

The Institute of Anatomy and Anthropology (AAI) of Riga Stradiņš University (RSU) displays a remarkable historical collection of educational and scientific materials on anatomy and embryology, 8381 items in total. The creation of the collection started in 2002, and nowadays it integrates 16 sub-collections: the main exhibits of P. Stradiņš’s collection; the collection of pathological exhibits from Gailezers Hospital with 542 items; the collection of the Children’s Clinical University Hospital with 21 exhibits; Anatomy Laboratory collection with 105 exhibits; Professor A. Amelin’s collection with 134 exhibits; the animal collection with 64 exhibits; the collection of embryological exhibits with 138 specimens together with 59 exhibits of the reproductive system; the bone collection from archaeological excavations in Riga with 986 exhibits; the collection of bone preparations and skulls, 4714 exhibits; V. Derums’ bone collection of 94 items. A separate collection contains 67 exhibits from the first Latvian anatomical excavations conducted under the guidance of Professor J. Prīmanis and Polish archaeological excavations of the Order of the Brothers of the Sword in St. George’s Church and the Convent yard, which includes 48 historical finds; the above is supplemented by 26 finds from anthropological material and a collection of bone specimens with 82 exhibits and a collection of skulls with 159 exhibits. A separate section at the AAI exhibition displays a collection of animal bones, which includes 58 exhibits and is used for comparative studies. Since 2003, the historical collection has been used to teach Latvians and foreigners who are interested to understand death, diseased tissues, to teach sympathy and how to protect oneself and others from diseases. The historical material is used for regular student training as well as for students’ research needs. Finally, digitization of unique exhibits, description in Latvian and English, and placing in the RSU repository has started, and, so far, 240 exhibits have been processed.


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.


1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1997 ◽  
Vol 161 ◽  
pp. 761-776 ◽  
Author(s):  
Claudio Maccone

AbstractSETI from space is currently envisaged in three ways: i) by large space antennas orbiting the Earth that could be used for both VLBI and SETI (VSOP and RadioAstron missions), ii) by a radiotelescope inside the Saha far side Moon crater and an Earth-link antenna on the Mare Smythii near side plain. Such SETIMOON mission would require no astronaut work since a Tether, deployed in Moon orbit until the two antennas landed softly, would also be the cable connecting them. Alternatively, a data relay satellite orbiting the Earth-Moon Lagrangian pointL2would avoid the Earthlink antenna, iii) by a large space antenna put at the foci of the Sun gravitational lens: 1) for electromagnetic waves, the minimal focal distance is 550 Astronomical Units (AU) or 14 times beyond Pluto. One could use the huge radio magnifications of sources aligned to the Sun and spacecraft; 2) for gravitational waves and neutrinos, the focus lies between 22.45 and 29.59 AU (Uranus and Neptune orbits), with a flight time of less than 30 years. Two new space missions, of SETI interest if ET’s use neutrinos for communications, are proposed.


1997 ◽  
Vol 161 ◽  
pp. 707-709 ◽  
Author(s):  
Jun Jugaku ◽  
Shiro Nishimura

AbstractWe continued our search for partial (incomplete) Dyson spheres associated with 50 solar-type stars (spectral classes F, G, and K) within 25 pc of the Sun. No candidate objects were found.


2000 ◽  
Vol 179 ◽  
pp. 263-264
Author(s):  
K. Sundara Raman ◽  
K. B. Ramesh ◽  
R. Selvendran ◽  
P. S. M. Aleem ◽  
K. M. Hiremath

Extended AbstractWe have examined the morphological properties of a sigmoid associated with an SXR (soft X-ray) flare. The sigmoid is cospatial with the EUV (extreme ultra violet) images and in the optical part lies along an S-shaped Hαfilament. The photoheliogram shows flux emergence within an existingδtype sunspot which has caused the rotation of the umbrae giving rise to the sigmoidal brightening.It is now widely accepted that flares derive their energy from the magnetic fields of the active regions and coronal levels are considered to be the flare sites. But still a satisfactory understanding of the flare processes has not been achieved because of the difficulties encountered to predict and estimate the probability of flare eruptions. The convection flows and vortices below the photosphere transport and concentrate magnetic field, which subsequently appear as active regions in the photosphere (Rust & Kumar 1994 and the references therein). Successive emergence of magnetic flux, twist the field, creating flare productive magnetic shear and has been studied by many authors (Sundara Ramanet al.1998 and the references therein). Hence, it is considered that the flare is powered by the energy stored in the twisted magnetic flux tubes (Kurokawa 1996 and the references therein). Rust & Kumar (1996) named the S-shaped bright coronal loops that appear in soft X-rays as ‘Sigmoids’ and concluded that this S-shaped distortion is due to the twist developed in the magnetic field lines. These transient sigmoidal features tell a great deal about unstable coronal magnetic fields, as these regions are more likely to be eruptive (Canfieldet al.1999). As the magnetic fields of the active regions are deep rooted in the Sun, the twist developed in the subphotospheric flux tube penetrates the photosphere and extends in to the corona. Thus, it is essentially favourable for the subphotospheric twist to unwind the twist and transmit it through the photosphere to the corona. Therefore, it becomes essential to make complete observational descriptions of a flare from the magnetic field changes that are taking place in different atmospheric levels of the Sun, to pin down the energy storage and conversion process that trigger the flare phenomena.


2000 ◽  
Vol 179 ◽  
pp. 193-196
Author(s):  
V. I. Makarov ◽  
A. G. Tlatov

AbstractA possible scenario of polar magnetic field reversal of the Sun during the Maunder Minimum (1645–1715) is discussed using data of magnetic field reversals of the Sun for 1880–1991 and the14Ccontent variations in the bi-annual rings of the pine-trees in 1600–1730 yrs.


2000 ◽  
Vol 179 ◽  
pp. 177-183
Author(s):  
D. M. Rust

AbstractSolar filaments are discussed in terms of two contrasting paradigms. The standard paradigm is that filaments are formed by condensation of coronal plasma into magnetic fields that are twisted or dimpled as a consequence of motions of the fields’ sources in the photosphere. According to a new paradigm, filaments form in rising, twisted flux ropes and are a necessary intermediate stage in the transfer to interplanetary space of dynamo-generated magnetic flux. It is argued that the accumulation of magnetic helicity in filaments and their coronal surroundings leads to filament eruptions and coronal mass ejections. These ejections relieve the Sun of the flux generated by the dynamo and make way for the flux of the next cycle.


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