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Uzay ajans\u0131 NASA<\/a>, G\u00fcne\u015f<\/a> Sistemi\u2019ni \u00e7evreleyen dev koruyucu balon helyosferin s\u0131n\u0131rlar\u0131n\u0131 haritalamak \u00fczere yeni bir uzay g\u00f6revi ba\u015flatt\u0131\u011f\u0131n\u0131 a\u00e7\u0131klad\u0131.<\/p>\n \u00a0<\/p>\n SINIRLAR \u0130LK KEZ AYRINTILI \u0130NCELENECEK<\/strong><\/p>\n \u00a0<\/p>\n NASA\u2019n\u0131n<\/a> Interstellar Mapping and Acceleration Probe (IMAP) adl\u0131 uzay arac\u0131, G\u00fcne\u015f\u2019in olu\u015fturdu\u011fu ve G\u00fcne\u015f Sistemi\u2019ni galaktik radyasyondan koruyan helyosferin yap\u0131s\u0131n\u0131 inceleyecek.\u00a0<\/p>\n \u00a0<\/p>\n G\u00f6revin iki y\u0131l s\u00fcrmesi ve bu s\u00fcre\u00e7te helyosferin s\u0131n\u0131rlar\u0131n\u0131n ve i\u00e7 dinamiklerinin ayr\u0131nt\u0131l\u0131 bi\u00e7imde haritalanmas\u0131 hedefleniyor.<\/p>\n \u00a0<\/p>\n G\u00dcNE\u015e’TEN GELEN Y\u00dcKSEK ENERJ\u0130L\u0130 PAR\u00c7ACIKLAR<\/strong><\/p>\n \u00a0<\/p>\n IMAP g\u00f6revi kapsam\u0131nda, G\u00fcne\u015f y\u00fczeyinden f\u0131rlayan y\u00fcksek enerjili par\u00e7ac\u0131klar, gezegenler aras\u0131 bo\u015flukta olu\u015fan manyetik alanlar ve galaksinin daha uzak b\u00f6lgelerinde \u00e7\u00f6ken y\u0131ld\u0131zlardan geriye kalan kozmik toz incelenecek.<\/p>\n \u00a0<\/p>\n NASA\u2019dan yap\u0131lan a\u00e7\u0131klamada, \u201cUzay arac\u0131, G\u00fcne\u015f\u2019in etkinli\u011fini ve helyosferin s\u0131n\u0131rlar\u0131n\u0131n, y\u0131ld\u0131zlar aras\u0131 uzayla nas\u0131l etkile\u015fime girdi\u011fini ara\u015ft\u0131r\u0131yor\u201d ifadeleri kullan\u0131ld\u0131.<\/p>\n \u00a0<\/p>\n