King of the Set

2019 ◽  
pp. 144-166
Author(s):  
Harlow Robinson
Keyword(s):  
Psychological Aspects ◽  
Political Activity ◽  
The Sun ◽  
Family Secrets

The chapter surveys films of the mid-1940s: The Purple Heart (a melodrama about American airmen held captive in Japan), A Walk in the Sun (an acclaimed documentary-style feature exploring the psychological aspects of an American platoon’s attack on an enemy-held farmhouse in Italy, with innovative musical treatment) and The Strange Love of Martha Ivers (an underrated film noir starring Barbara Stanwyck, Kirk Douglas and Judith Anderson dealing with corruption and family secrets in a small Pennsylvania city). Also discussed: Milestone’s work with actors Dana Andrews and Norman Lloyd; screenwriter Robert Rossen; Milestone’s involvement in political activity in Hollywood during studio strikes of 1945-46.

The Influence of Modern Party System on the Development of Parliamentarism in Russia: Institutional, Political and Psychological Aspects

2018 ◽  
Vol 42 ◽  
pp. 266-273
Author(s):  
Ivan S. Palitai
Keyword(s):  
Public Opinion ◽  
Party System ◽  
Psychological Aspects ◽  
Political Activity ◽  
The Public ◽  
Political Processes ◽  
The People ◽  
Voting System ◽  
New Ideas ◽  
Opinion Polls

The article is devoted to the modern Russian party system. In the first part of the article, the author shows the historical features of the parties formation in Russia and analyzes the reasons for the low turnout in the elections to the State Duma in 2016. According to the author the institutional reasons consist in the fact that the majority of modern political parties show less and less ability to produce new ideas, and the search for meanings is conducted on the basis of the existing, previously proposed sets of options. Parties reduce the topic of self-identification in party rhetoric, narrowing it down to “branded” ideas or focusing on the image of the leader. In addition, the author shows the decrease in the overall political activity of citizens after the 2011 elections, and points out that the legislation amendments led to the reduction of the election campaigns duration and changes in the voting system itself. The second part of the article is devoted to the study of the psychological aspects of the party system. The author presents the results of the investigation of images of the parties as well as the results of the population opinion polls, held by the centers of public opinion study. On the basis of this data, the author concludes that according to the public opinion the modern party system is ineffective, and the parties don’t have real political weight, which leads to the decrease of the interest in their activities and confidence in them. The author supposes that all this may be the consequence of the people’s fatigue from the same persons in politics, but at the same time the electorate’s desire to see new participants in political processes is formulated rather vaguely, since, according to the people, this might not bring any positive changes.

Research: An Analysis of Sun-Spot Destination Resort Market Segments: All-Inclusive Package Versus Independent Travel Arrangements

1997 ◽  
Vol 21 (1) ◽  
pp. 141-159 ◽  
Author(s):  
Jihwan Yoon ◽  
Elwood L. Shafer
Keyword(s):  
Length Of Stay ◽  
Employment Status ◽  
Telephone Interview ◽  
Demographic Characteristics ◽  
Psychological Aspects ◽  
The Sun ◽  
Market Segments ◽  
Independent Travel ◽  
Interview Survey

The sun-spot-destination resort market is one of the most important and growing segments of the contemporary tourism market. The objective of this study was to determine, through a telephone interview survey of 702 American travel parties, if there were significant differences between travel parties who preferred an all-inclusive travel package and those who preferred independent travel arrangements. The variables of interest in these comparisons were: socio-demographic characteristics, travel-related characteristics, determinant attributes and lifestyle characteristics. Results indicate that there are significant differences in terms of age distributions, employment status, preferred destinations, length of stay, several lifestyle characteristics and preferences for physical and psychological aspects (determinant attributes) of the resort.

Chromospheric activity as a function of age in main-sequence stars

1966 ◽  
Vol 24 ◽  
pp. 40-43
Author(s):  
O. C. Wilson ◽  
A. Skumanich
Keyword(s):  
Main Sequence ◽  
The Sun ◽  
Main Sequence Stars ◽  
Tentative Conclusion ◽  
Chromospheric Activity ◽  
General Field ◽  
Large Clusters

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.

Galactic orbits of stars

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley
Keyword(s):  
Globular Cluster ◽  
Potential Field ◽  
High Velocity ◽  
Velocity Vector ◽  
Variable Stars ◽  
The Sun ◽  
Proper Motions ◽  
Rr Lyrae ◽  
The Galaxy

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.

Seti Space Missions

1997 ◽  
Vol 161 ◽  
pp. 761-776 ◽  
Author(s):  
Claudio Maccone
Keyword(s):  
Electromagnetic Waves ◽  
Space Missions ◽  
Gravitational Lens ◽  
The Sun ◽  
Space Antenna ◽  
Focal Distance ◽  
Large Space ◽  
The Earth ◽  
Space Antennas ◽  
New Space

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.

A Search for Dyson Spheres around Late-Type Stars in the Solar Neighborhood II

1997 ◽  
Vol 161 ◽  
pp. 707-709 ◽  
Author(s):  
Jun Jugaku ◽  
Shiro Nishimura
Keyword(s):  
Solar Neighborhood ◽  
The Sun ◽  
Late Type ◽  
Solar Type

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.

Emergence of Twisted Magnetic Flux Related Sigmoidal Brightening

2000 ◽  
Vol 179 ◽  
pp. 263-264
Author(s):  
K. Sundara Raman ◽  
K. B. Ramesh ◽  
R. Selvendran ◽  
P. S. M. Aleem ◽  
K. M. Hiremath
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Magnetic Flux ◽  
Ultra Violet ◽  
Active Regions ◽  
Morphological Properties ◽  
Energy Storage And Conversion ◽  
The Sun ◽  
X Rays ◽  
The Magnetic Field

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.

Polar Magnetic Field Reversals of the Sun in Maunder Minimum

2000 ◽  
Vol 179 ◽  
pp. 193-196
Author(s):  
V. I. Makarov ◽  
A. G. Tlatov
Keyword(s):  
Magnetic Field ◽  
Maunder Minimum ◽  
The Sun ◽  
Annual Rings ◽  
Field Reversal ◽  
Polar Magnetic Field ◽  
Pine Trees ◽  
Using Data ◽  
Magnetic Field Reversal

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.

Solar Filaments as Tracers of Subsurface Processes

2000 ◽  
Vol 179 ◽  
pp. 177-183
Author(s):  
D. M. Rust
Keyword(s):  
Magnetic Fields ◽  
Magnetic Flux ◽  
Coronal Mass Ejections ◽  
Interplanetary Space ◽  
Intermediate Stage ◽  
Coronal Plasma ◽  
Magnetic Helicity ◽  
The Sun ◽  
New Paradigm ◽  
Solar Filaments

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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