. . "Uma \u00F3rbita el\u00EDptica alta (HEO), em ingl\u00EAs Highly Elliptical Orbit, \u00E9 uma \u00F3rbita el\u00EDptica em que a menor altitude do sat\u00E9lite \u00E9 de cerca de 1 000 km, enquanto que sua maior altitude ultrapassa os 35 786 km. A visibilidade desses sat\u00E9lites pode ser superior a 12 horas quando est\u00E3o pr\u00F3ximos do apogeu."@pt . "Highly Elliptical Orbit"@de . . "Uma \u00F3rbita el\u00EDptica alta (HEO), em ingl\u00EAs Highly Elliptical Orbit, \u00E9 uma \u00F3rbita el\u00EDptica em que a menor altitude do sat\u00E9lite \u00E9 de cerca de 1 000 km, enquanto que sua maior altitude ultrapassa os 35 786 km. A visibilidade desses sat\u00E9lites pode ser superior a 12 horas quando est\u00E3o pr\u00F3ximos do apogeu."@pt . "\u0412\u044B\u0441\u043E\u043A\u0430\u044F \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u043E\u0440\u0431\u0438\u0442\u0430 (\u0442\u0430\u043A\u0436\u0435 \u0412\u044B\u0441\u043E\u043A\u043E\u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u043E\u0440\u0431\u0438\u0442\u0430, \u0412\u042D\u041E) \u2014 \u044D\u0442\u043E \u0442\u0438\u043F \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u043E\u0439 \u043E\u0440\u0431\u0438\u0442\u044B, \u0443 \u043A\u043E\u0442\u043E\u0440\u043E\u0439 \u0432\u044B\u0441\u043E\u0442\u0430 \u0432 \u0430\u043F\u043E\u0433\u0435\u0435 \u0432\u043E \u043C\u043D\u043E\u0433\u043E \u0440\u0430\u0437 \u043F\u0440\u0435\u0432\u044B\u0448\u0430\u0435\u0442 \u0432\u044B\u0441\u043E\u0442\u0443 \u0432 \u043F\u0435\u0440\u0438\u0433\u0435\u0435."@ru . . "Una \u00F3rbita altamente el\u00EDptica u \u00F3rbita muy el\u00EDptica (HEO, por las siglas del ingl\u00E9s Highly Elliptical Orbit) es una \u00F3rbita el\u00EDptica con una alta excentricidad y, normalmente, geoc\u00E9ntrica. Algunos conocidos ejemplos de \u00F3rbitas HEO inclinadas son las \u00F3rbitas M\u00F3lniya y las .\u200B"@es . . "Une orbite elliptique \u00E9lev\u00E9e[r\u00E9f. n\u00E9cessaire] est une orbite terrestre haute avec une p\u00E9riapside de basse altitude et une apoapside de haute altitude (plus de 35 786 kilom\u00E8tres). Contrairement \u00E0 la plupart de ceux situ\u00E9s sur une orbite g\u00E9ostationnaire, les v\u00E9hicules spatiaux situ\u00E9s sur une orbite elliptique \u00E9lev\u00E9e peuvent g\u00E9n\u00E9ralement voir les deux p\u00F4les de la Terre."@fr . . . "1067096526"^^ . . "\u0412\u044B\u0441\u043E\u043A\u0430\u044F \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u043E\u0440\u0431\u0438\u0442\u0430 (\u0442\u0430\u043A\u0436\u0435 \u0412\u044B\u0441\u043E\u043A\u043E\u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u043E\u0440\u0431\u0438\u0442\u0430, \u0412\u042D\u041E) \u2014 \u044D\u0442\u043E \u0442\u0438\u043F \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u043E\u0439 \u043E\u0440\u0431\u0438\u0442\u044B, \u0443 \u043A\u043E\u0442\u043E\u0440\u043E\u0439 \u0432\u044B\u0441\u043E\u0442\u0430 \u0432 \u0430\u043F\u043E\u0433\u0435\u0435 \u0432\u043E \u043C\u043D\u043E\u0433\u043E \u0440\u0430\u0437 \u043F\u0440\u0435\u0432\u044B\u0448\u0430\u0435\u0442 \u0432\u044B\u0441\u043E\u0442\u0443 \u0432 \u043F\u0435\u0440\u0438\u0433\u0435\u0435."@ru . "\u5927\u692D\u5706\u8F68\u9053\uFF08Highly Elliptical Orbit\uFF0C\u7F29\u5199\u4E3AHEO\uFF09\u5730\u7403\u8F68\u9053\u7684\u4E00\u79CD\uFF0C\u5E38\u4E3A\u822A\u5929\u5668\u6240\u4F7F\u7528\u3002 \u5927\u692D\u5706\u8F68\u9053\u662F\u4E00\u79CD\u5177\u6709\u8F83\u4F4E\u8FD1\u5730\u70B9\u548C\u6781\u9AD8\u8FDC\u5730\u70B9\u7684\u692D\u5706\u8F68\u9053\uFF0C\u5176\u8FDC\u5730\u70B9\u9AD8\u5EA6\u5927\u4E8E\u9759\u6B62\u536B\u661F\u7684\u9AD8\u5EA6\uFF0835786\u5343\u7C73\uFF09\u3002\u6839\u636E\u5F00\u666E\u52D2\u5B9A\u5F8B\uFF0C\u536B\u661F\u5728\u8FDC\u5730\u70B9\u9644\u8FD1\u533A\u57DF\u7684\u8FD0\u884C\u901F\u5EA6\u8F83\u6162\uFF0C\u56E0\u6B64\u8FD9\u79CD\u6781\u5EA6\u62C9\u957F\u7684\u8F68\u9053\u7684\u7279\u70B9\u662F\u536B\u661F\u5230\u8FBE\u548C\u79BB\u5F00\u8FDC\u5730\u70B9\u7684\u8FC7\u7A0B\u5F88\u957F\uFF0C\u800C\u7ECF\u8FC7\u8FD1\u5730\u70B9\u7684\u8FC7\u7A0B\u6781\u77ED\u3002\u8FD9\u4F7F\u5F97\u536B\u661F\u5BF9\u8FDC\u5730\u70B9\u4E0B\u65B9\u7684\u5730\u9762\u533A\u57DF\u7684\u8986\u76D6\u65F6\u95F4\u53EF\u4EE5\u8D85\u8FC712\u5C0F\u65F6\u3002\u8FD9\u79CD\u7279\u70B9\u80FD\u591F\u88AB\u901A\u4FE1\u536B\u661F\u6240\u5229\u7528\u3002 \u5177\u6709\u5927\u503E\u659C\u89D2\u5EA6\u7684\u9AD8\u692D\u5706\u8F68\u9053\u536B\u661F\u53EF\u4EE5\u8986\u76D6\u5730\u7403\u7684\u6781\u5730\u5730\u533A\uFF0C\u8FD9\u662F\u8FD0\u884C\u4E8E\u5730\u7403\u540C\u6B65\u8F68\u9053\u7684\u536B\u661F\u6240\u65E0\u6CD5\u505A\u5230\u7684\u3002\u7531\u4E8E\u82CF\u8054\uFF08\u4EE5\u53CA\u73B0\u5728\u7684\u4FC4\u7F57\u65AF\uFF09\u5927\u90E8\u5206\u56FD\u571F\u5904\u4E8E\u7EAC\u5EA6\u8F83\u9AD8\u7684\u5730\u533A\uFF0C\u53D1\u5C55\u5730\u7403\u540C\u6B65\u536B\u661F\u5BF9\u5176\u610F\u4E49\u4E0D\u5927\uFF0C\u6240\u4EE5\u82CF\u8054\u662F\u6700\u91CD\u89C6\u53D1\u5C55\u9AD8\u692D\u5706\u8F68\u9053\u536B\u661F\u7684\u56FD\u5BB6\u3002\u4E00\u79CD\u8457\u540D\u7684\u9AD8\u692D\u5706\u8F68\u9053\u7C7B\u578B\uFF0C\u5373\u95EA\u7535\u8F68\u9053\uFF08\u6216\u6709\u97F3\u8B6F\u70BA\u83AB\u5C3C\u4E9E\u8ECC\u9053\uFF0C\u503E\u89D2\u4E3A63.4\u00B0\uFF09\uFF0C\u662F\u4EE5\u82CF\u8054\u7684\u8FD0\u8F7D\u706B\u7BAD\u540D\u79F0\uFF08\u95EA\u7535\u53F7\uFF09\u547D\u540D\u7684\u3002"@zh . . . . . "\u0412\u0438\u0441\u043E\u043A\u0430 \u0435\u043B\u0456\u043F\u0442\u0438\u0447\u043D\u0430 \u043E\u0440\u0431\u0456\u0442\u0430"@uk . "\u9577\u6955\u5186\u8ECC\u9053\uFF08\u3061\u3087\u3046\u3060\u3048\u3093\u304D\u3069\u3046\u3000Highly elliptical orbit,HEO\uFF09\u306F\u3001\u4EBA\u5DE5\u885B\u661F\u306E\u8ECC\u9053\u306E\u5206\u985E\u306E\u4E00\u3002\u6955\u5186\u8ECC\u9053(elliptical orbit)\u306E\u4E00\u7A2E\u3067\u3082\u3042\u308B\u3002\u8ECC\u9053\u96E2\u5FC3\u7387\u304C\u5927\u304D\u306A\u8ECC\u9053\u3067\u3042\u308A\u3001\u30E2\u30EB\u30CB\u30E4\u8ECC\u9053\u3084\u30C4\u30F3\u30C9\u30E9\u8ECC\u9053\u3082\u3053\u308C\u306B\u5206\u985E\u3055\u308C\u308B\u3002 \u3053\u306E\u3088\u3046\u306A\u6975\u7AEF\u306A\u6955\u5186\u8ECC\u9053\u306B\u304A\u3051\u308B\u885B\u661F\u306F\u3001\u9060\u5730\u70B9\u4ED8\u8FD1\u306B\u304A\u3044\u3066\u306F\u3001\u5730\u4E0A\u304B\u3089\u306F\u3086\u3063\u304F\u308A\u3068\u79FB\u52D5\u3057\u3066\u3044\u308B\u3088\u3046\u306B\u898B\u3048\u3001\u89B3\u6E2C\u53EF\u80FD\u6642\u9593\u3082\u9577\u304F\u306A\u308B\u3002\u307E\u305F\u3001\u305D\u306E\u6027\u8CEA\u3092\u5FDC\u7528\u3057\u3001\u5730\u4E0A\u306E\u9AD8\u7DEF\u5EA6\u5730\u5E2F\u306B\u304A\u3044\u3066\u3082\u3001\u885B\u661F\u304C\u6BD4\u8F03\u7684\u9577\u6642\u9593\u3001\u9AD8\u3044\u4EF0\u89D2\u306E\u4F4D\u7F6E\u3092\u4FDD\u3064\u3053\u3068\u304C\u3067\u304D\u308B\u3002\u3053\u308C\u3089\u306E\u7279\u6027\u306F\u3001\u901A\u4FE1\u885B\u661F\u306B\u5411\u3044\u3066\u304A\u308A\u3001\u9759\u6B62\u8ECC\u9053\u4E0A\u306E\u901A\u4FE1\u885B\u661F\u304B\u3089\u3067\u306F\u3001\u9AD8\u7DEF\u5EA6\u5730\u5E2F\u306B\u304A\u3044\u3066\u4EF0\u89D2\u304C\u4F4E\u304F\u306A\u308A\u3059\u304E\u5229\u7528\u3067\u304D\u306A\u3044\u5834\u5408\u304C\u3042\u308B\u3068\u3044\u3046\u6B20\u70B9\u3092\u88DC\u3048\u308B\u3002"@ja . "\u0412\u0438\u0441\u043E\u043A\u0430 \u0435\u043B\u0456\u043F\u0442\u0438\u0447\u043D\u0430 \u043E\u0440\u0431\u0456\u0442\u0430 (\u0412\u0415\u041E) \u2014 \u0446\u0435 \u0442\u0438\u043F \u043D\u0430\u0432\u043A\u043E\u043B\u043E\u0437\u0435\u043C\u043D\u043E\u0457 \u043E\u0440\u0431\u0456\u0442\u0438, \u043D\u0430 \u044F\u043A\u0456\u0439 \u0432\u0438\u0441\u043E\u0442\u0430 \u0432 \u0430\u043F\u043E\u0433\u0435\u0457 \u0432 \u0431\u0430\u0433\u0430\u0442\u043E \u0440\u0430\u0437\u0456\u0432 \u043F\u0435\u0440\u0435\u0432\u0438\u0449\u0443\u0454 \u0432\u0438\u0441\u043E\u0442\u0443 \u0432 \u043F\u0435\u0440\u0438\u0433\u0435\u0457."@uk . . "\u9577\u6955\u5186\u8ECC\u9053\uFF08\u3061\u3087\u3046\u3060\u3048\u3093\u304D\u3069\u3046\u3000Highly elliptical orbit,HEO\uFF09\u306F\u3001\u4EBA\u5DE5\u885B\u661F\u306E\u8ECC\u9053\u306E\u5206\u985E\u306E\u4E00\u3002\u6955\u5186\u8ECC\u9053(elliptical orbit)\u306E\u4E00\u7A2E\u3067\u3082\u3042\u308B\u3002\u8ECC\u9053\u96E2\u5FC3\u7387\u304C\u5927\u304D\u306A\u8ECC\u9053\u3067\u3042\u308A\u3001\u30E2\u30EB\u30CB\u30E4\u8ECC\u9053\u3084\u30C4\u30F3\u30C9\u30E9\u8ECC\u9053\u3082\u3053\u308C\u306B\u5206\u985E\u3055\u308C\u308B\u3002 \u3053\u306E\u3088\u3046\u306A\u6975\u7AEF\u306A\u6955\u5186\u8ECC\u9053\u306B\u304A\u3051\u308B\u885B\u661F\u306F\u3001\u9060\u5730\u70B9\u4ED8\u8FD1\u306B\u304A\u3044\u3066\u306F\u3001\u5730\u4E0A\u304B\u3089\u306F\u3086\u3063\u304F\u308A\u3068\u79FB\u52D5\u3057\u3066\u3044\u308B\u3088\u3046\u306B\u898B\u3048\u3001\u89B3\u6E2C\u53EF\u80FD\u6642\u9593\u3082\u9577\u304F\u306A\u308B\u3002\u307E\u305F\u3001\u305D\u306E\u6027\u8CEA\u3092\u5FDC\u7528\u3057\u3001\u5730\u4E0A\u306E\u9AD8\u7DEF\u5EA6\u5730\u5E2F\u306B\u304A\u3044\u3066\u3082\u3001\u885B\u661F\u304C\u6BD4\u8F03\u7684\u9577\u6642\u9593\u3001\u9AD8\u3044\u4EF0\u89D2\u306E\u4F4D\u7F6E\u3092\u4FDD\u3064\u3053\u3068\u304C\u3067\u304D\u308B\u3002\u3053\u308C\u3089\u306E\u7279\u6027\u306F\u3001\u901A\u4FE1\u885B\u661F\u306B\u5411\u3044\u3066\u304A\u308A\u3001\u9759\u6B62\u8ECC\u9053\u4E0A\u306E\u901A\u4FE1\u885B\u661F\u304B\u3089\u3067\u306F\u3001\u9AD8\u7DEF\u5EA6\u5730\u5E2F\u306B\u304A\u3044\u3066\u4EF0\u89D2\u304C\u4F4E\u304F\u306A\u308A\u3059\u304E\u5229\u7528\u3067\u304D\u306A\u3044\u5834\u5408\u304C\u3042\u308B\u3068\u3044\u3046\u6B20\u70B9\u3092\u88DC\u3048\u308B\u3002"@ja . "2506"^^ . . . . . "Orbita altamente ellittica"@it . "Una \u00F3rbita altamente el\u00EDptica u \u00F3rbita muy el\u00EDptica (HEO, por las siglas del ingl\u00E9s Highly Elliptical Orbit) es una \u00F3rbita el\u00EDptica con una alta excentricidad y, normalmente, geoc\u00E9ntrica. Algunos conocidos ejemplos de \u00F3rbitas HEO inclinadas son las \u00F3rbitas M\u00F3lniya y las .\u200B Tales \u00F3rbitas inclinadas extremadamente alargadas tienen la ventaja de ofrecer largos tiempos de permanencia en cierto punto del cielo, al acercarse el sat\u00E9lite al apogeo y luego al descender desde \u00E9ste. Cuando los sat\u00E9lites se mueven cerca del apogeo, desde tierra parecen moverse muy lentamente y permanecen a gran altitud durante largos per\u00EDodos de tiempo sobre determinadas zonas terrestres de alta latitud. Esto hace que estas \u00F3rbitas el\u00EDpticas sean especialmente \u00FAtiles para sat\u00E9lites de comunicaciones, ya que los tradicionales sat\u00E9lites de comunicaciones geoestacionarios no cubren dichas altas latitudes.\u200B"@es . . "\u0412\u044B\u0441\u043E\u043A\u0430\u044F \u044D\u043B\u043B\u0438\u043F\u0442\u0438\u0447\u0435\u0441\u043A\u0430\u044F \u043E\u0440\u0431\u0438\u0442\u0430"@ru . . . . "\u5927\u692D\u5706\u8F68\u9053"@zh . "Orbity silnie eliptyczne"@pl . . . "Orbity silnie eliptyczne (ang. Highly Elliptical Orbits \u2013 HEO) \u2013 orbity oko\u0142oziemskie, maj\u0105ce perygeum na wysoko\u015Bci od ok. 500\u20131000 km nad powierzchni\u0105 Ziemi, a apogeum na wysoko\u015Bci powy\u017Cej 35 786 km. Orbity te maj\u0105 zwykle k\u0105t inklinacji od 50 do 70\u00B0, przy czym najcz\u0119\u015Bciej wybieranym k\u0105tem jest ok. 63,4\u00B0, przy kt\u00F3rym linia apsyd pozostaje nieruchoma."@pl . . . . . "Orbity silnie eliptyczne (ang. Highly Elliptical Orbits \u2013 HEO) \u2013 orbity oko\u0142oziemskie, maj\u0105ce perygeum na wysoko\u015Bci od ok. 500\u20131000 km nad powierzchni\u0105 Ziemi, a apogeum na wysoko\u015Bci powy\u017Cej 35 786 km. Orbity te maj\u0105 zwykle k\u0105t inklinacji od 50 do 70\u00B0, przy czym najcz\u0119\u015Bciej wybieranym k\u0105tem jest ok. 63,4\u00B0, przy kt\u00F3rym linia apsyd pozostaje nieruchoma."@pl . . . . . "Un'orbita altamente ellittica (HEO, Highly Elliptical Orbit), anche indicata come orbita ad elevata eccentricit\u00E0 (High-Eccentricity Orbit), \u00E8 un'orbita geocentrica ellittica con perigeo a bassa quota, generalmente inferiore ai 1.000 chilometri, ed apogeo a quota molto elevata, anche superiore ai 35.000 chilometri. Questa tipologia di orbite presenta un valore piuttosto elevato dell'eccentricit\u00E0 orbitale ed \u00E8 a ci\u00F2 che fanno riferimento entrambe le denominazioni in lingua inglese, da cui sono derivate quelle in italiano."@it . . . . . "654975"^^ . . . . . . . . . . . . "A highly elliptical orbit (HEO) is an elliptic orbit with high eccentricity, usually referring to one around Earth.Examples of inclined HEO orbits include Molniya orbits, named after the Molniya Soviet communication satellites which used them, and Tundra orbits. Such extremely elongated orbits have the advantage of long dwell times at a point in the sky during the approach to, and descent from, apogee. Bodies moving through the long apogee dwell appear to move slowly, and remain at high altitude over high-latitude ground sites for long periods of time. This makes these elliptical orbits useful for communications satellites. Geostationary orbits cannot serve high latitudes because their elevation above the horizon from these ground sites is too low. Sirius Satellite Radio used inclined HEO orbits, specifically the Tundra orbits, to keep two satellites positioned above North America while another satellite quickly sweeps through the southern part of its 24-hour orbit. The longitude above which the satellites dwell at apogee in the small loop remains relatively constant as Earth rotates. The three separate orbits are spaced equally around the Earth, but share a common ground track."@en . "\u00D3rbita altamente el\u00EDptica"@es . . . "Highly elliptical orbit"@en . . "\u5927\u692D\u5706\u8F68\u9053\uFF08Highly Elliptical Orbit\uFF0C\u7F29\u5199\u4E3AHEO\uFF09\u5730\u7403\u8F68\u9053\u7684\u4E00\u79CD\uFF0C\u5E38\u4E3A\u822A\u5929\u5668\u6240\u4F7F\u7528\u3002 \u5927\u692D\u5706\u8F68\u9053\u662F\u4E00\u79CD\u5177\u6709\u8F83\u4F4E\u8FD1\u5730\u70B9\u548C\u6781\u9AD8\u8FDC\u5730\u70B9\u7684\u692D\u5706\u8F68\u9053\uFF0C\u5176\u8FDC\u5730\u70B9\u9AD8\u5EA6\u5927\u4E8E\u9759\u6B62\u536B\u661F\u7684\u9AD8\u5EA6\uFF0835786\u5343\u7C73\uFF09\u3002\u6839\u636E\u5F00\u666E\u52D2\u5B9A\u5F8B\uFF0C\u536B\u661F\u5728\u8FDC\u5730\u70B9\u9644\u8FD1\u533A\u57DF\u7684\u8FD0\u884C\u901F\u5EA6\u8F83\u6162\uFF0C\u56E0\u6B64\u8FD9\u79CD\u6781\u5EA6\u62C9\u957F\u7684\u8F68\u9053\u7684\u7279\u70B9\u662F\u536B\u661F\u5230\u8FBE\u548C\u79BB\u5F00\u8FDC\u5730\u70B9\u7684\u8FC7\u7A0B\u5F88\u957F\uFF0C\u800C\u7ECF\u8FC7\u8FD1\u5730\u70B9\u7684\u8FC7\u7A0B\u6781\u77ED\u3002\u8FD9\u4F7F\u5F97\u536B\u661F\u5BF9\u8FDC\u5730\u70B9\u4E0B\u65B9\u7684\u5730\u9762\u533A\u57DF\u7684\u8986\u76D6\u65F6\u95F4\u53EF\u4EE5\u8D85\u8FC712\u5C0F\u65F6\u3002\u8FD9\u79CD\u7279\u70B9\u80FD\u591F\u88AB\u901A\u4FE1\u536B\u661F\u6240\u5229\u7528\u3002 \u5177\u6709\u5927\u503E\u659C\u89D2\u5EA6\u7684\u9AD8\u692D\u5706\u8F68\u9053\u536B\u661F\u53EF\u4EE5\u8986\u76D6\u5730\u7403\u7684\u6781\u5730\u5730\u533A\uFF0C\u8FD9\u662F\u8FD0\u884C\u4E8E\u5730\u7403\u540C\u6B65\u8F68\u9053\u7684\u536B\u661F\u6240\u65E0\u6CD5\u505A\u5230\u7684\u3002\u7531\u4E8E\u82CF\u8054\uFF08\u4EE5\u53CA\u73B0\u5728\u7684\u4FC4\u7F57\u65AF\uFF09\u5927\u90E8\u5206\u56FD\u571F\u5904\u4E8E\u7EAC\u5EA6\u8F83\u9AD8\u7684\u5730\u533A\uFF0C\u53D1\u5C55\u5730\u7403\u540C\u6B65\u536B\u661F\u5BF9\u5176\u610F\u4E49\u4E0D\u5927\uFF0C\u6240\u4EE5\u82CF\u8054\u662F\u6700\u91CD\u89C6\u53D1\u5C55\u9AD8\u692D\u5706\u8F68\u9053\u536B\u661F\u7684\u56FD\u5BB6\u3002\u4E00\u79CD\u8457\u540D\u7684\u9AD8\u692D\u5706\u8F68\u9053\u7C7B\u578B\uFF0C\u5373\u95EA\u7535\u8F68\u9053\uFF08\u6216\u6709\u97F3\u8B6F\u70BA\u83AB\u5C3C\u4E9E\u8ECC\u9053\uFF0C\u503E\u89D2\u4E3A63.4\u00B0\uFF09\uFF0C\u662F\u4EE5\u82CF\u8054\u7684\u8FD0\u8F7D\u706B\u7BAD\u540D\u79F0\uFF08\u95EA\u7535\u53F7\uFF09\u547D\u540D\u7684\u3002"@zh . "\u00D3rbita el\u00EDptica alta"@pt . . . . "Une orbite elliptique \u00E9lev\u00E9e[r\u00E9f. n\u00E9cessaire] est une orbite terrestre haute avec une p\u00E9riapside de basse altitude et une apoapside de haute altitude (plus de 35 786 kilom\u00E8tres). Contrairement \u00E0 la plupart de ceux situ\u00E9s sur une orbite g\u00E9ostationnaire, les v\u00E9hicules spatiaux situ\u00E9s sur une orbite elliptique \u00E9lev\u00E9e peuvent g\u00E9n\u00E9ralement voir les deux p\u00F4les de la Terre."@fr . . . . . "Un'orbita altamente ellittica (HEO, Highly Elliptical Orbit), anche indicata come orbita ad elevata eccentricit\u00E0 (High-Eccentricity Orbit), \u00E8 un'orbita geocentrica ellittica con perigeo a bassa quota, generalmente inferiore ai 1.000 chilometri, ed apogeo a quota molto elevata, anche superiore ai 35.000 chilometri. Questa tipologia di orbite presenta un valore piuttosto elevato dell'eccentricit\u00E0 orbitale ed \u00E8 a ci\u00F2 che fanno riferimento entrambe le denominazioni in lingua inglese, da cui sono derivate quelle in italiano. Le orbite HEO sono utilizzate soprattutto per garantire i servizi satellitari alle regioni terrestri ad elevata latitudine (prossime cio\u00E8 ai poli), che sono coperte con difficolt\u00E0 da un satellite posto su un'orbita geostazionaria (equatoriale). Inoltre, una o pi\u00F9 orbite HEO possono essere percorse nei trasferimenti verso i punti di Lagrange del sistema Terra-Sole che prevedano una manovra di fionda gravitazionale con la Luna."@it . . . . "\u9577\u6955\u5186\u8ECC\u9053"@ja . . "Orbite elliptique \u00E9lev\u00E9e"@fr . "A highly elliptical orbit (HEO) is an elliptic orbit with high eccentricity, usually referring to one around Earth.Examples of inclined HEO orbits include Molniya orbits, named after the Molniya Soviet communication satellites which used them, and Tundra orbits."@en . . . . "\u0412\u0438\u0441\u043E\u043A\u0430 \u0435\u043B\u0456\u043F\u0442\u0438\u0447\u043D\u0430 \u043E\u0440\u0431\u0456\u0442\u0430 (\u0412\u0415\u041E) \u2014 \u0446\u0435 \u0442\u0438\u043F \u043D\u0430\u0432\u043A\u043E\u043B\u043E\u0437\u0435\u043C\u043D\u043E\u0457 \u043E\u0440\u0431\u0456\u0442\u0438, \u043D\u0430 \u044F\u043A\u0456\u0439 \u0432\u0438\u0441\u043E\u0442\u0430 \u0432 \u0430\u043F\u043E\u0433\u0435\u0457 \u0432 \u0431\u0430\u0433\u0430\u0442\u043E \u0440\u0430\u0437\u0456\u0432 \u043F\u0435\u0440\u0435\u0432\u0438\u0449\u0443\u0454 \u0432\u0438\u0441\u043E\u0442\u0443 \u0432 \u043F\u0435\u0440\u0438\u0433\u0435\u0457."@uk .