Perevod: Vol'nova A.A.
Poyasnenie:
Vid nochnogo neba s 5-kilometrovoi vysoty
plato Chahnantor, raspolozhennogo v chiliiskih Andah, zastavlyaet zatait' dyhanie.
Davlenie razrezhennoi atmosfery v etom temnom meste sostavlyaet 50% ot normal'nogo, pri etom vozduh zdes'
neveroyatno suhoi.
Eto ideal'noe mesto dlya Bol'shogo Millimetrovogo/submillimetrovogo Massiva Atakamy
(Atacama Large
Millimeter/submillimeter Array, ALMA), kotoryi skonstruirovan dlya izucheniya Vselennoi na dlinah voln,
v 1000 raz bol'shih, chem vidimyi svet.
V centre etoi panoramy raspolozhilis'
7- i 12-metrovaya antenny massiva AL'MA, osveshennye svetom molodoi Luny, gnezdyasheisya v arke Mlechnogo Puti.
Konfiguraciya antenn AL'MY, rabotayushih v rezhime
interferometra, pozvolit poluchit' razreshenie, sravnimoe s kosmicheskimi
teleskopami.
Chudesnyi nochnoi vid ukrashayut sled ot meteora i sputnik Mlechnogo Puti — galaktiki Bol'shoe (snizu) i
Maloe Magellanovy Oblaka.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Publikacii s klyuchevymi slovami:
radiotelescope - interferometry - Radiointerferometr - Radioteleskop
Publikacii so slovami: radiotelescope - interferometry - Radiointerferometr - Radioteleskop | |
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