CĂRȚI ÎN ENGLEZĂ ÎN LEGĂTURĂ CU «ARCMIN»
Descoperă întrebuințarea
arcmin în următoarea selecție bibliografică. Cărți în legătură cu
arcmin și extrase din aceasta pentru a furniza contextul de întrebuințare al acestuia în literatura Engleză.
Collimation Tolerances Magnification Step Convergence Divergence ×7 2arcmin
6.5arcmin 3arcmin ×10 1.5arcmin 4.5arcmin 2arcmin ×15 1.0arcmin 3.0arcmin
1.5arcmin ×20 0.75arcmin 2.25arcmin 1.0arcmin ×30 0.5arcmin 1.5arcmin ...
2
Binocular Vision and Stereopsis
(Redrawn from Rogers and Graham 1985.) Table 12.1. Models of disparity
coding Two-channel organization Broadly tuned. -12 -8-40 4 8 12 Peak-to-trough
amplitude of test surface (arcmin) a) An ever-ascending staircase created by
illusory ...
Before modern isophotometry, its major axis was thought to have an extent of
only about 160 arcmin, although Hubble (1932) found evidence from faint stellar
clusters (now recognised as star clouds) that the disk might have a diameter of ...
4
Observational Constraints on Circumstellar Disk Evolution ...
displaying the density in 10% increments from 0-90% of the peak surface density
of 15 arcmin-2 in the center of h Per. This surface density is higher than the ~ 7-8
arcmin-2 peak found by BK05, who were restricted to sources with spectral ...
Thayne Michael Currie, 2008
5
Disparity Averaging Mechanisms in Stereopsis
Perceived depth data collected in Experiment 1 were to be used to predict the
outcome for Experiment 2, which tested whether disparity averaging occurs at
stereothreshold or increment threshold from 0 arcmin (the pedestal disparity).
6
Vision in 3D Environments
0 30 20 10 LK –80 –60 –40 –20 (a) 0 20 40 60 80 Mask lateral shift (arcmin) M
a s k i n g s e n s i t i v i t y M a s k i n g s e n s i t i v i t y –80 (b) –60 –40 –20 0 20
40 60 80 Mask lateral shift (arcmin) Figure 5.3 Masking sensitivity (thick line)
when ...
Laurence R. Harris, Michael R. M. Jenkin, 2011
7
Perceiving in Depth, Volume 1: Basic Mechanisms
−50 0 an amplitude of 65 arcmin. Responses away from the rest- ing position
were slower than those toward the resting posi- tion (Houtman and van der Pol
1982b). Perlmutter and Kertesz (1982) used the stimulus shown in Figure 10.44,
...
8
Perceiving in Depth, Volume 1: Basic Mechanisms
Stimulus used by Perlmutter and Kertesz (1982). an amplitude of 65 arcmin.
Responses away from the resting position were slower than those toward the
resting position (Houtman and van der Pol 1982b). Perlmutter and Kertesz (1982)
used ...
Ian P. Howard, Brian J. Rogers, 2012
9
Video Displays, Work, and Vision
... preferred 3:1 to 15:1; 6:1 to 10:1 preferred 3s 3:1; > 15:1 preferred 5:1 to 10:1 4:
1 3s 3:1; 8:1-10:1 optimum 3 3.5 mm 3= 18arcmin; 2.6 mm preferred 3s 18arcmin
15-21 arcmin 2s 16 arcmin; 20 arcmin preferred 15.2-20.6 arcmin 3s 20 arcmin ...
10
Fundamental Parameters in Cosmology
It is basically the Saskatoon experiment29 mounted on a balloon platform: a
chopping flat is mounted in front of an off-axis 1 m primary, feeding two Q-band (
39 arcmin FWHM, 8 GHz bandwidth), one K-band (54 arcmin FWHM, 8 GHz ...
ȘTIRI NOI CARE INCLUD TERMENUL «ARCMIN»
Află ce ziare naționale și internaționale au scris despre și cum este întrebuințat termenul
arcmin în contextul următoarelor știri.
Stony Brook deep-space hunter discovers ultra dark galaxies far, far …
This image was made from the Subaru Telescope at the National Astronomical Observatory of Japan. A small region of 6 x 6 arcmin is cut out ... «Newsday, Iun 15»
Monster Black Hole Wakes After 26 Years
The mission is dedicated to spectroscopy (E/∆E = 500) and imaging (angular resolution: 12 arcmin FWHM) of celestial gamma-ray sources in ... «eNews Park Forest, Iun 15»
Astronomers discover more than 800 dark galaxies in the famous …
A small region of 6 x 6 arcmin is cut out from large Coma Cluster images. Yellow circles show two of the 47 dark galaxies discovered last year, ... «Astronomy Magazine, Iun 15»
Scientists discover brightest early galaxy and likely first generation …
DEIMOS (the DEep Imaging and Multi-Object Spectrograph) boasts the largest field of view (16.7 arcmin by 5 arcmin) of any of the Keck ... «Phys.Org, Iun 15»
Exact Lens Positioning Is Key to High-Performance Optics Production
As the performance is operator independent and fully software controlled, there exists a centering accuracy of less than 2 µm and less than 0.2 arcmin, ... «Photonics.com, Iun 15»
Planetary performance increases accuracy - New gear range from …
... between just five and seven arcmin for single and double-stage ratios respectively, the HPN delivers exceptional accuracy and repeatability. «Industry Today, Mai 15»
Magnetar near Galactic Centre supermassive black hole delivers …
... that led to its discovery. The main Image is 8 arcmin across (about 61 light-years); Inset image is about 14 arcsec across (1.8 light-years). «Astronomy Now Online, Mai 15»
Unusual asteroid suspected of spinning to explosion
DEIMOS (the DEep Imaging and Multi-Object Spectrograph) boasts the largest field of view (16.7 arcmin by 5 arcmin) of any of the Keck ... «Phys.Org, Mar 15»
Thermonuclear supernova ejects our galaxy's fastest star (w/ video)
Joe Miller, ESI also has a low-resolution mode and can image in a 2 x 8 arcmin field of view. An upgrade provided an integral field unit that can ... «Phys.Org, Mar 15»
Best images! Asteroid 2004 BL86, as it swept near Earth
Taken from 20:28 to 20:44 UTC. Telescope Maksutov-Cassegrain 30cm f/5.6, CCD Sbig STL-6303, field of view 58×39 arcmin. Thank you ... «EarthSky, Ian 15»
