Faculty Opinions recommendation of Great apes' understanding of other individuals' line of sight.

Author(s):  
Kent Berridge
Keyword(s):  
2007 ◽  
Vol 18 (5) ◽  
pp. 462-468 ◽  
Author(s):  
Sanae Okamoto-Barth ◽  
Josep Call ◽  
Michael Tomasello
Keyword(s):  

1967 ◽  
Vol 31 ◽  
pp. 171-172
Author(s):  
Th. Schmidt-Kaler

The integralNHof neutral-hydrogen density along the line of sight is determined from the Kootwijk and Sydney surveys. The run ofNHwith galactic longitude agrees well with that of thermal continuous radiation and that of the optical surface brightness of the Milky Way.


1994 ◽  
Vol 144 ◽  
pp. 421-426
Author(s):  
N. F. Tyagun

AbstractThe interrelationship of half-widths and intensities for the red, green and yellow lines is considered. This is a direct relationship for the green and yellow line and an inverse one for the red line. The difference in the relationships of half-widths and intensities for different lines appears to be due to substantially dissimilar structuring and to a set of line-of-sight motions in ”hot“ and ”cold“ corona regions.When diagnosing the coronal plasma, one cannot neglect the filling factor - each line has such a factor of its own.


1968 ◽  
Author(s):  
ANDREW J. ECKLES ◽  
THOMAS A. GARRY ◽  
WILLIAM C. MULLEN

2016 ◽  
Vol E99.B (6) ◽  
pp. 1362-1370 ◽  
Author(s):  
Maki ARAI ◽  
Tomohiro SEKI ◽  
Ken HIRAGA ◽  
Kazumitsu SAKAMOTO ◽  
Tadao NAKAGAWA
Keyword(s):  

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