Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.naic.edu/~tghosh/thesis-jf/chap_4/Table4.2.pdf Дата изменения: Wed May 3 03:32:39 2000 Дата индексирования: Mon Apr 11 10:18:08 2016 Кодировка: Поисковые слова: cosmic rays

Table 4.2
SC MK 4.31 BR 6.44 OV 6.80 KP 7.67 PT 8.11 LA 8.33 FD 8.96 NL 10.19 HN 13.02 SC ...

Resolution (HPBW) in mas for each VLBA Baseline at ,18 cm
HN NL 6.03 16.15 15.95 17.89 22.32 25.91 22.44 ... 23.05 10.19 FD LA PT KP 8.31 19.40 43.95 ... 89.05 56.95 49.91 17.89 10.25 7.67 OV 9.25 30.59 ... 43.95 38.16 34.13 24.62 15.95 9.56 6.80 BR 8.44 ... 30.59 19.40 20.56 21.13 15.83 16.15 10.15 6.44 MK ... 8.44 9.25 8.31 7.74 7.47 7.23 6.03 4.95 4.31

4.95 10.15 9.56 10.25 11.51 12.35 11.96 23.05 ... 13.02

7.23 7.47 7.74 15.83 21.13 20.56 24.62 34.13 38.16 49.91 56.95 89.05 65.72 156.68 ... 60.98 ... 156.68 ... 60.98 65.72 22.44 25.91 22.32 11.96 12.35 11.51 8.96 8.33 8.11

Note.--Resolutions (Half-power beamwidth; HPBW) in milliarcse maximum V LBA baselines in Table 2.1 and computed using HPBW receiver wavelength in cm. A uniformly weighted image made from synthesized beam with a slightly narrower minor axis FWHM. For ranges from about 20 to 0.2 mas as the wavelength runs from 90 cm VLBA sites a re defined in Figure 2.1.

conds (mas) corresponding to the ~ 2063 ,/Bmax mas, where , is the a long u-v plane track will have a the longest VLBA baseline, HPBW to 7 mm. Two-letter codes for the