The future of terrestrial broadcasting. The short-wave super transmitter

IEE Review ◽  
1989 ◽  
Vol 35 (4) ◽  
pp. 131 ◽  
Author(s):  
James Wood
Keyword(s):  

Author(s):  
Simon Mundy ◽  
Esmée Schilte

At the end of the last century, a dictionary could confidently define broadcasting as the transmission of a signal for television or radio. Within a decade, every element of that definition had changed. Transmission had branched out from the cumbersome business of placing masts bearing receivers and transmitters at the highest vantage points across the countryside. A signal was no longer confined to the band waves that the air could carry — invisible streams snaking their way across the landscape: Ultra High Frequency (UHF) carrying television, as long as the hills weren’t in the way; Very High Frequency (VHF or FM)carrying wonderful quality sound, as long as the same hills were not joined by chimneys, bodies, the wrong sort of cloud or stonework; Long Wave, unstoppable by anything except distance, it seemed,carrying cricket and the shipping forecast across Europe and far out to sea; Medium Wave(AM), the carrier of choice for hosts of daytime local music stations and great for listening in the car, but hopeless when night fell and the waves went bouncing around the ionosphere bringing martial music from Albania where the football commentary should have been; and Short Wave — the touchiest of the wave bands, that made catching the words as hard as catching fish, but finally gave national broadcasters a global reach.



1966 ◽  
Vol 24 ◽  
pp. 51-52
Author(s):  
E. K. Kharadze ◽  
R. A. Bartaya

The unique 70-cm meniscus-type telescope of the Abastumani Astrophysical Observatory supplied with two objective prisms and the seeing conditions characteristic at Mount Kanobili (Abastumani) permit us to obtain stellar spectra of a high quality. No additional design to improve the “climate” immediately around the telescope itself is being applied. The dispersions and photographic magnitude limits are 160 and 660Å/mm, and 12–13, respectively. The short-wave end of spectra reaches 3500–3400Å.



1961 ◽  
Vol 13 ◽  
pp. 29-41
Author(s):  
Wm. Markowitz
Keyword(s):  

A symposium on the future of the International Latitude Service (I. L. S.) is to be held in Helsinki in July 1960. My report for the symposium consists of two parts. Part I, denoded (Mk I) was published [1] earlier in 1960 under the title “Latitude and Longitude, and the Secular Motion of the Pole”. Part II is the present paper, denoded (Mk II).



1978 ◽  
Vol 48 ◽  
pp. 387-388
Author(s):  
A. R. Klemola
Keyword(s):  

Second-epoch photographs have now been obtained for nearly 850 of the 1246 fields of the proper motion program with centers at declination -20° and northwards. For the sky at 0° and northward only 130 fields remain to be taken in the next year or two. The 270 southern fields with centers at -5° to -20° remain for the future.



Author(s):  
Godfrey C. Hoskins ◽  
Betty B. Hoskins

Metaphase chromosomes from human and mouse cells in vitro are isolated by micrurgy, fixed, and placed on grids for electron microscopy. Interpretations of electron micrographs by current methods indicate the following structural features.Chromosomal spindle fibrils about 200Å thick form fascicles about 600Å thick, wrapped by dense spiraling fibrils (DSF) less than 100Å thick as they near the kinomere. Such a fascicle joins the future daughter kinomere of each metaphase chromatid with those of adjacent non-homologous chromatids to either side. Thus, four fascicles (SF, 1-4) attach to each metaphase kinomere (K). It is thought that fascicles extend from the kinomere poleward, fray out to let chromosomal fibrils act as traction fibrils against polar fibrils, then regroup to join the adjacent kinomere.



Author(s):  
Nicholas J Severs

In his pioneering demonstration of the potential of freeze-etching in biological systems, Russell Steere assessed the future promise and limitations of the technique with remarkable foresight. Item 2 in his list of inherent difficulties as they then stood stated “The chemical nature of the objects seen in the replica cannot be determined”. This defined a major goal for practitioners of freeze-fracture which, for more than a decade, seemed unattainable. It was not until the introduction of the label-fracture-etch technique in the early 1970s that the mould was broken, and not until the following decade that the full scope of modern freeze-fracture cytochemistry took shape. The culmination of these developments in the 1990s now equips the researcher with a set of effective techniques for routine application in cell and membrane biology.Freeze-fracture cytochemical techniques are all designed to provide information on the chemical nature of structural components revealed by freeze-fracture, but differ in how this is achieved, in precisely what type of information is obtained, and in which types of specimen can be studied.



Author(s):  
B. C. Hutchens
Keyword(s):  


Author(s):  
Maria Hodges
Keyword(s):  


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