An ultra-laminar tetrode gun for high duty cycle applications

Author(s):  
R. True
Keyword(s):  
Author(s):  
J. Šulc ◽  
H. Jelínková ◽  
M. E. Doroshenko ◽  
T. T. Basiev ◽  
V. V. Osiko ◽  
...  

Author(s):  
M. Hübner ◽  
M. Wilkens ◽  
B. Eppich ◽  
A. Maaßdorf ◽  
D. Martin ◽  
...  

2010 ◽  
Vol 56 (4) ◽  
pp. 454-468 ◽  
Author(s):  
M. Brock Fenton

Abstract Twenty-five characters or suites of characters from bats are considered in light of changes in bat classification. The characters include some associated with flower-visiting (two), echolocation (12), roosting (six), reproduction (two) and three are of unknown adaptive function. In both the 1998 and 2006 classifications of bats into suborders (Megachiroptera and Microchiroptera versus Yinpterochiroptera and Yangochiroptera, respectively), some convergences between suborders are the same (e.g., foliage roosting, tent building), but others associated with echolocation differ substantially. In the 1998 phylogeny convergences associated with echolocation (high duty cycle echolocation, nasal emission of echolocation calls) occurred among the Microchiroptera. In the 2006 phylogeny, they occur between Yinpterochiroptera and Yangochiroptera. While some traits apparently arose independently in two suborders (e.g., foliage-roosting, tent building, low intensity echolocation calls, noseleafs, nasal emission of echolocation calls, high duty cycle echolocation behaviour), others appear to have been ancestral (roosting in narrow spaces, laryngeal echolocation, stylohyal-tympanic contact, oral emission of echolocation calls, and small litter size). A narrow profile through the chest is typical of bats reflecting the thoracic skeleton. This feature suggests that the ancestors of bats spent the day in small crevices. Features associated with laryngeal echolocation appear to be ancestral, suggesting that echolocation evolved early in bats but was subsequently lost in one yinpterochiropteran lineage.


2013 ◽  
Vol 13 (1) ◽  
pp. 26 ◽  
Author(s):  
Elizabeth L Clare ◽  
Amanda M Adams ◽  
Aline Z Maya-Simões ◽  
Judith L Eger ◽  
Paul DN Hebert ◽  
...  

2004 ◽  
Vol 213 ◽  
pp. 409-414 ◽  
Author(s):  
Seth Shostak ◽  
Ray Villard

In optical SETI (OSETI) experiments, it is generally assumed that signals will be deliberate, narrowly targeted beacons sent by extraterrestrial societies to large numbers of candidate star systems. If this is so, then it may be unrealistic to expect a high duty cycle for the received signal. Ergo, an advantage accrues to any OSETI scheme that realistically suggests where and when to search. In this paper, we elaborate a proposal (Castellano, Doyle, & McIntosh 2000) for selecting regions of sky for intensive optical SETI monitoring based on characteristics of our solar system that would be visible at great distance. This can enormously lessen the amount of sky that needs to be searched. In addition, this is an attractive approach for the transmitting society because it both increases the chances of reception and provides a large reduction in energy required. with good astrometric information, the transmitter need be no more powerful than an automobile tail light.


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