. . "Une perturbation ionosph\u00E9rique \u00E0 d\u00E9but brusque ou PIDB (Sudden Ionospheric Disturbance - SID en anglais) r\u00E9sulte d'une ionisation anormalement \u00E9lev\u00E9e de la couche D de l'ionosph\u00E8re faisant suite \u00E0 une \u00E9ruption solaire."@fr . . . . . "Nag\u0142e zak\u0142\u00F3cenia jonosferyczne (ang. SID \u2013 Sudden Ionospheric Disturbance) \u2013 zak\u0142\u00F3cenia mocy i fazy sygna\u0142u radiowego, wynikaj\u0105ce z wysokiej aktywno\u015Bci s\u0142onecznej, powoduj\u0105cej zwi\u0119kszon\u0105 jonizacj\u0119 i absorpcj\u0119 fal radiowych w warstwie D.Mog\u0105 prowadzi\u0107 do cz\u0119\u015Bciowej lub ca\u0142kowitej utraty \u0142\u0105czno\u015Bci na falach kr\u00F3tkich, trwaj\u0105cej od kilku minut do kilku godzin. Poniewa\u017C zjawisko to polepsza propagacj\u0119 fal bardzo d\u0142ugich (VLF), wykorzystywane jest do wykrywania rozb\u0142ysk\u00F3w s\u0142onecznych poprzez monitorowanie mocy sygna\u0142u odleg\u0142ych nadajnik\u00F3w VLF."@pl . "Dum jaroj kun intensa aktiveco de la Suno povas okazi intensa rentgena radiado de la suno, nomita flare en angla. Kiam tiu elektromagneta energio atingas la atmosferon de la Tero, la rentgena radiado povas atingi la D-tavolon de la jonosfero, t.e. \u011Dis \u0109irka\u016D 70 km super la surfaco de la Tero kaj forte ionizi \u011Din. La efiko de Moefel Dellinger malpliigas la disvasti\u011Don de frekvencoj \u011Dis \u0109irka\u016D 300 MHz. Tio okazas nur je la taga flanko de la Tero. Post ripetitaj fortaj radiadoj povas okazi parta \u011Dis tuta fori\u011Do de radio-kontaktoj je mallongaj ondoj. La fenomeno povas da\u016Dri kelkajn minutojn \u011Dis kelkajn horojn. La efiko estis trovita \u0109irka\u016D 1930 de la germano elp. Megel. 1935 la usonano prezentis \u011Din al la usona standardiga oficejo."@eo . "\uB378\uB9B0\uC800 \uD604\uC0C1\uC740 \uC9C0\uAD6C\uC758 \uC911\uAC04\uAD8C\uC5D0 \uC874\uC7AC\uD558\uB294 \uC804\uB9AC\uCE35\uC758 D\uCE35\uC774 \uD0DC\uC591 \uD45C\uBA74\uC758 \uD3ED\uBC1C\uB85C \uC778\uD558\uC5EC \uBC1C\uC0DD\uD55C \uAC15\uD55C \uC804\uC790\uAE30\uD30C\uB4E4\uB85C \uC778\uD574 \uB450\uAEBC\uC6CC\uC838 \uCD08\uB2E8\uD30C\uB97C \uD761\uC218\uD558\uC5EC \uAD6D\uC81C\uD1B5\uC2E0\uC774 \uB450\uC808\uB418\uB294 \uD604\uC0C1\uC774\uB2E4. 1935\uB144 \uBBF8\uAD6D\uC758 \uC874 \uD558\uC6CC\uB4DC \uB378\uB9B0\uC800\uAC00 \uD1B5\uC2E0\uC804\uD30C\uC758 \uBE44\uC815\uC0C1\uC801\uC778 \uAC10\uC1C4\uD604\uC0C1\uC774 \uD0DC\uC591\uACFC \uAD00\uB828\uC774 \uC788\uC74C\uC744 \uBC1C\uACAC\uD558\uC5EC \uB378\uB9B0\uC800 \uD604\uC0C1\uC774\uB77C\uACE0 \uBD88\uB9B0\uB2E4. \uD0DC\uC591\uBA74\uC758 \uD3ED\uBC1C\uB85C \uAC11\uC790\uAE30 \uB9CE\uC740 \uC591\uC774 \uBC29\uCD9C\uB418\uB294 \uC804\uC790\uAE30\uD30C\uAC00 \uC9C0\uAD6C \uC804\uB9AC\uCE35\uC758 \uC774\uC628\uACFC \uCDA9\uB3CC\uD558\uBA74\uC11C \uC804\uC790\uC758 \uBC00\uB3C4\uB97C \uD06C\uAC8C \uC99D\uAC00\uC2DC\uCF1C \uC774\uB85C \uC778\uD574 \uC77C\uC2DC\uC801\uC73C\uB85C \uB2E8\uD30C\uBB34\uC120\uD1B5\uC2E0\uC774 \uB04A\uC5B4\uC9C0\uB294 \uC804\uD30C\uC758 \uC7A5\uC560 \uD604\uC0C1\uC744 \uB9D0\uD55C\uB2E4. \uAD6D\uC81C\uD1B5\uC2E0\uC758 \uB450\uC808\uC740 \uCD5C\uC18C 5~10\uBD84, \uCD5C\uB300\uB294 \uC218 \uC2DC\uAC04\uAE4C\uC9C0 \uACC4\uC18D\uB41C\uB2E4. 1935\uB144 \uD0DC\uC591\uC758 \uC790\uC804\uC8FC\uAE30\uC5D0 \uB530\uB77C \uC804\uD30C\uC758 \uC774\uC0C1\uAC10\uC1C4 \uD604\uC0C1\uC744 \uBC1C\uACAC\uD558\uACE0 \uADF8\uAC83\uC774 \uD0DC\uC591 \uC790\uC804\uC8FC\uAE30\uC758 2\uBC30\uC778 55\uC77C\uB9C8\uB2E4 \uC77C\uC5B4\uB098\uB294 \uACBD\uD5A5\uC774 \uC788\uB2E4\uB294 \uAC83\uC744 \uC9C0\uC801\uD55C \uBBF8\uAD6D\uC758 \uBB3C\uB9AC\uD559\uC790 J. H. \uB378\uB9B0\uC800\uC758 \uC774\uB984\uC774 \uBD99\uC5EC\uC84C\uB2E4."@ko . . "Une perturbation ionosph\u00E9rique \u00E0 d\u00E9but brusque ou PIDB (Sudden Ionospheric Disturbance - SID en anglais) r\u00E9sulte d'une ionisation anormalement \u00E9lev\u00E9e de la couche D de l'ionosph\u00E8re faisant suite \u00E0 une \u00E9ruption solaire."@fr . "\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u73FE\u8C61\uFF08\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u3052\u3093\u3057\u3087\u3046\u3001Dellinger Effect\uFF09\u3068\u306F\u96FB\u96E2\u5C64\u306B\u4F55\u3089\u304B\u306E\u7406\u7531\u3067\u7570\u5E38\u304C\u767A\u751F\u3059\u308B\u3053\u3068\u306B\u3088\u308A\u8D77\u3053\u308B\u901A\u4FE1\u969C\u5BB3\u3067\u3042\u308B\u3002\u77ED\u6CE2\u969C\u5BB3\uFF08SWF\uFF1AShort Wave Fadeout\uFF09\u307E\u305F\u306F\u7A81\u767A\u6027\u96FB\u96E2\u5C64\u64FE\u4E71\uFF08SID\uFF1ASudden Ionospherric Disturbance\uFF09\u3001\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u52B9\u679C\uFF08Dellinger Effect\uFF09\u3068\u3082\u547C\u3070\u308C\u308B\u3002 \u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u73FE\u8C61\u306E\u540D\u524D\u306F\u30011935\u5E74\u306B\u3053\u308C\u3092\u767A\u8868\u3057\u305F\u30A2\u30E1\u30EA\u30AB\u306E\u901A\u4FE1\u6280\u5E2B\u3001\u306B\u7531\u6765\u3059\u308B\u3002\u3053\u306E\u5B9F\u7E3E\u306A\u3069\u306B\u3088\u308A\u3001\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u306F1938\u5E74\u306BIEEE\u6804\u8A89\u8CDE\u3092\u53D7\u8CDE\u3057\u305F\u3002\u3057\u304B\u3057\u5B9F\u306F\u3001\u3053\u306E5\u5E74\u524D\u306E1930\u5E74\u306B\u30C9\u30A4\u30C4\u306E\u30CF\u30F3\u30B9\u30FB\u30E1\u30FC\u30B2\u30EB\uFF08Hans M\u00F6gel\uFF09\u304C\u5148\u306B\u767A\u898B\u3057\u3066\u3044\u305F\u3002\u3053\u306E\u305F\u3081\u3001\u30C9\u30A4\u30C4\u3067\u306FM\u00F6gel-Dellinger-Effekt\uFF08\u30E1\u30FC\u30B2\u30EB=\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u52B9\u679C\uFF09\u3068\u547C\u3070\u308C\u3066\u3044\u308B\u3002"@ja . "Nag\u0142e zak\u0142\u00F3cenia jonosferyczne (ang. SID \u2013 Sudden Ionospheric Disturbance) \u2013 zak\u0142\u00F3cenia mocy i fazy sygna\u0142u radiowego, wynikaj\u0105ce z wysokiej aktywno\u015Bci s\u0142onecznej, powoduj\u0105cej zwi\u0119kszon\u0105 jonizacj\u0119 i absorpcj\u0119 fal radiowych w warstwie D.Mog\u0105 prowadzi\u0107 do cz\u0119\u015Bciowej lub ca\u0142kowitej utraty \u0142\u0105czno\u015Bci na falach kr\u00F3tkich, trwaj\u0105cej od kilku minut do kilku godzin. Poniewa\u017C zjawisko to polepsza propagacj\u0119 fal bardzo d\u0142ugich (VLF), wykorzystywane jest do wykrywania rozb\u0142ysk\u00F3w s\u0142onecznych poprzez monitorowanie mocy sygna\u0142u odleg\u0142ych nadajnik\u00F3w VLF. Nag\u0142e zak\u0142\u00F3cenia jonosferyczne odkry\u0142 niemiecki fizyk oko\u0142o roku 1930, jakkolwiek r\u00F3\u017Cne odmiany SID poznano dopiero w latach p\u00F3\u017Aniejszych."@pl . . . . . . . . . . . . "Perturbation ionosph\u00E9rique \u00E0 d\u00E9but brusque"@fr . "Una perturbaci\u00F3n ionosf\u00E9rica s\u00FAbita (tambi\u00E9n conocida como SID, del ingl\u00E9s \"sudden ionospheric disturbance\" o como Efecto Dellinger) es un fen\u00F3meno de ionizaci\u00F3n de plasma de densidad anormalmente alta en la regi\u00F3n D de la ionosfera causado por una fulguraci\u00F3n solar. El resultado de uno de estos episodios es un aumento repentino de la absorci\u00F3n de las ondas de radio que es m\u00E1s severo en las se\u00F1ales de frecuencia media (MF) y en la gama m\u00E1s baja de las de alta frecuencia, lo que a menudo se traduce en interrupciones o interferencias en los sistemas de telecomunicaciones.\u200B"@es . . . . "Dellinger\u016Fv efekt"@cs . "1089785377"^^ . "A sudden ionospheric disturbance (SID) is any one of several ionospheric perturbations, resulting from abnormally high ionization/plasma density in the D region of the ionosphere and caused by a solar flare and/or solar particle event (SPE). The SID results in a sudden increase in radio-wave absorption that is most severe in the upper medium frequency (MF) and lower high frequency (HF) ranges, and as a result often interrupts or interferes with telecommunications systems."@en . "Dellinger\u016Fv efekt (n\u011Bkdy t\u00E9\u017E M\u00F6gel-Dellinger\u016Fv efekt) se projevuje jako n\u00E1hl\u00E9, kr\u00E1tkodob\u00E9 zhor\u0161en\u00ED \u010Di \u00FApln\u00E9 p\u0159eru\u0161en\u00ED r\u00E1diov\u00E9ho p\u0159\u00EDjmu v p\u00E1smu kr\u00E1tk\u00FDch vln, zp\u016Fsoben\u00E9 slune\u010Dn\u00ED erupc\u00ED. Jev se d\u00E1 vyu\u017E\u00EDt k detekci slune\u010Dn\u00EDch erupc\u00ED."@cs . . . . . "\uB378\uB9B0\uC800 \uD604\uC0C1"@ko . . . . . "Der M\u00F6gel-Dellinger-Effekt beschreibt einen kurzzeitigen Ausfall von prim\u00E4r Kurzwellenverbindungen und deren Ausbreitung \u00FCber die Raumwelle, ausgel\u00F6st durch Sonneneruptionen. Entdeckt wurde der Effekt um das Jahr 1930 von dem Deutschen Hans M\u00F6gel. 1935 hat ihn der Amerikaner John Howard Dellinger dem US-Standardisierungsamt (damals englisch National Bureau of Standards NBS, heute National Institute of Standards and Technology NIST) vorgestellt."@de . "Uma perturba\u00E7\u00E3o ionosf\u00E9rica s\u00FAbita (PIS) \u00E9 qualquer das diversas perturba\u00E7\u00F5es ionosf\u00E9ricas resultantes de ioniza\u00E7\u00E3o ou densidade de plasma anormalmente altas na regi\u00E3o D da ionosfera, causadas por uma erup\u00E7\u00E3o solar e/ou . A PIS resulta num aumento s\u00FAbito na absor\u00E7\u00E3o de ondas de r\u00E1dio, que \u00E9 mais severa nas m\u00E9dias frequ\u00EAncias superiores e nas altas frequ\u00EAncias inferiores, causando frequentemente interrup\u00E7\u00F5es ou interfer\u00EAncias nos sistemas de telecomunica\u00E7\u00F5es."@pt . . . . . "A sudden ionospheric disturbance (SID) is any one of several ionospheric perturbations, resulting from abnormally high ionization/plasma density in the D region of the ionosphere and caused by a solar flare and/or solar particle event (SPE). The SID results in a sudden increase in radio-wave absorption that is most severe in the upper medium frequency (MF) and lower high frequency (HF) ranges, and as a result often interrupts or interferes with telecommunications systems."@en . . . . . "Perturbaci\u00F3n ionosf\u00E9rica s\u00FAbita"@es . "\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u73FE\u8C61\uFF08\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u3052\u3093\u3057\u3087\u3046\u3001Dellinger Effect\uFF09\u3068\u306F\u96FB\u96E2\u5C64\u306B\u4F55\u3089\u304B\u306E\u7406\u7531\u3067\u7570\u5E38\u304C\u767A\u751F\u3059\u308B\u3053\u3068\u306B\u3088\u308A\u8D77\u3053\u308B\u901A\u4FE1\u969C\u5BB3\u3067\u3042\u308B\u3002\u77ED\u6CE2\u969C\u5BB3\uFF08SWF\uFF1AShort Wave Fadeout\uFF09\u307E\u305F\u306F\u7A81\u767A\u6027\u96FB\u96E2\u5C64\u64FE\u4E71\uFF08SID\uFF1ASudden Ionospherric Disturbance\uFF09\u3001\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u52B9\u679C\uFF08Dellinger Effect\uFF09\u3068\u3082\u547C\u3070\u308C\u308B\u3002 \u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u73FE\u8C61\u306E\u540D\u524D\u306F\u30011935\u5E74\u306B\u3053\u308C\u3092\u767A\u8868\u3057\u305F\u30A2\u30E1\u30EA\u30AB\u306E\u901A\u4FE1\u6280\u5E2B\u3001\u306B\u7531\u6765\u3059\u308B\u3002\u3053\u306E\u5B9F\u7E3E\u306A\u3069\u306B\u3088\u308A\u3001\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u306F1938\u5E74\u306BIEEE\u6804\u8A89\u8CDE\u3092\u53D7\u8CDE\u3057\u305F\u3002\u3057\u304B\u3057\u5B9F\u306F\u3001\u3053\u306E5\u5E74\u524D\u306E1930\u5E74\u306B\u30C9\u30A4\u30C4\u306E\u30CF\u30F3\u30B9\u30FB\u30E1\u30FC\u30B2\u30EB\uFF08Hans M\u00F6gel\uFF09\u304C\u5148\u306B\u767A\u898B\u3057\u3066\u3044\u305F\u3002\u3053\u306E\u305F\u3081\u3001\u30C9\u30A4\u30C4\u3067\u306FM\u00F6gel-Dellinger-Effekt\uFF08\u30E1\u30FC\u30B2\u30EB=\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u52B9\u679C\uFF09\u3068\u547C\u3070\u308C\u3066\u3044\u308B\u3002"@ja . . . "Perturba\u00E7\u00E3o ionosf\u00E9rica s\u00FAbita"@pt . . . . "Uma perturba\u00E7\u00E3o ionosf\u00E9rica s\u00FAbita (PIS) \u00E9 qualquer das diversas perturba\u00E7\u00F5es ionosf\u00E9ricas resultantes de ioniza\u00E7\u00E3o ou densidade de plasma anormalmente altas na regi\u00E3o D da ionosfera, causadas por uma erup\u00E7\u00E3o solar e/ou . A PIS resulta num aumento s\u00FAbito na absor\u00E7\u00E3o de ondas de r\u00E1dio, que \u00E9 mais severa nas m\u00E9dias frequ\u00EAncias superiores e nas altas frequ\u00EAncias inferiores, causando frequentemente interrup\u00E7\u00F5es ou interfer\u00EAncias nos sistemas de telecomunica\u00E7\u00F5es."@pt . "Sudden ionospheric disturbance"@en . . . . . . . "Efiko de Moegel Dellinger"@eo . "\u30C7\u30EA\u30F3\u30B8\u30E3\u30FC\u73FE\u8C61"@ja . . . . "5478196"^^ . "Der M\u00F6gel-Dellinger-Effekt beschreibt einen kurzzeitigen Ausfall von prim\u00E4r Kurzwellenverbindungen und deren Ausbreitung \u00FCber die Raumwelle, ausgel\u00F6st durch Sonneneruptionen. Entdeckt wurde der Effekt um das Jahr 1930 von dem Deutschen Hans M\u00F6gel. 1935 hat ihn der Amerikaner John Howard Dellinger dem US-Standardisierungsamt (damals englisch National Bureau of Standards NBS, heute National Institute of Standards and Technology NIST) vorgestellt."@de . . . "5605"^^ . "Dum jaroj kun intensa aktiveco de la Suno povas okazi intensa rentgena radiado de la suno, nomita flare en angla. Kiam tiu elektromagneta energio atingas la atmosferon de la Tero, la rentgena radiado povas atingi la D-tavolon de la jonosfero, t.e. \u011Dis \u0109irka\u016D 70 km super la surfaco de la Tero kaj forte ionizi \u011Din. La efiko de Moefel Dellinger malpliigas la disvasti\u011Don de frekvencoj \u011Dis \u0109irka\u016D 300 MHz. Tio okazas nur je la taga flanko de la Tero. Post ripetitaj fortaj radiadoj povas okazi parta \u011Dis tuta fori\u011Do de radio-kontaktoj je mallongaj ondoj. La fenomeno povas da\u016Dri kelkajn minutojn \u011Dis kelkajn horojn. La efiko estis trovita \u0109irka\u016D 1930 de la germano elp. Megel. 1935 la usonano prezentis \u011Din al la usona standardiga oficejo."@eo . . "Nag\u0142e zak\u0142\u00F3cenia jonosferyczne"@pl . "Una perturbaci\u00F3n ionosf\u00E9rica s\u00FAbita (tambi\u00E9n conocida como SID, del ingl\u00E9s \"sudden ionospheric disturbance\" o como Efecto Dellinger) es un fen\u00F3meno de ionizaci\u00F3n de plasma de densidad anormalmente alta en la regi\u00F3n D de la ionosfera causado por una fulguraci\u00F3n solar. El resultado de uno de estos episodios es un aumento repentino de la absorci\u00F3n de las ondas de radio que es m\u00E1s severo en las se\u00F1ales de frecuencia media (MF) y en la gama m\u00E1s baja de las de alta frecuencia, lo que a menudo se traduce en interrupciones o interferencias en los sistemas de telecomunicaciones.\u200B"@es . . . "Dellinger\u016Fv efekt (n\u011Bkdy t\u00E9\u017E M\u00F6gel-Dellinger\u016Fv efekt) se projevuje jako n\u00E1hl\u00E9, kr\u00E1tkodob\u00E9 zhor\u0161en\u00ED \u010Di \u00FApln\u00E9 p\u0159eru\u0161en\u00ED r\u00E1diov\u00E9ho p\u0159\u00EDjmu v p\u00E1smu kr\u00E1tk\u00FDch vln, zp\u016Fsoben\u00E9 slune\u010Dn\u00ED erupc\u00ED. Jev se d\u00E1 vyu\u017E\u00EDt k detekci slune\u010Dn\u00EDch erupc\u00ED."@cs . . "M\u00F6gel-Dellinger-Effekt"@de . "\uB378\uB9B0\uC800 \uD604\uC0C1\uC740 \uC9C0\uAD6C\uC758 \uC911\uAC04\uAD8C\uC5D0 \uC874\uC7AC\uD558\uB294 \uC804\uB9AC\uCE35\uC758 D\uCE35\uC774 \uD0DC\uC591 \uD45C\uBA74\uC758 \uD3ED\uBC1C\uB85C \uC778\uD558\uC5EC \uBC1C\uC0DD\uD55C \uAC15\uD55C \uC804\uC790\uAE30\uD30C\uB4E4\uB85C \uC778\uD574 \uB450\uAEBC\uC6CC\uC838 \uCD08\uB2E8\uD30C\uB97C \uD761\uC218\uD558\uC5EC \uAD6D\uC81C\uD1B5\uC2E0\uC774 \uB450\uC808\uB418\uB294 \uD604\uC0C1\uC774\uB2E4. 1935\uB144 \uBBF8\uAD6D\uC758 \uC874 \uD558\uC6CC\uB4DC \uB378\uB9B0\uC800\uAC00 \uD1B5\uC2E0\uC804\uD30C\uC758 \uBE44\uC815\uC0C1\uC801\uC778 \uAC10\uC1C4\uD604\uC0C1\uC774 \uD0DC\uC591\uACFC \uAD00\uB828\uC774 \uC788\uC74C\uC744 \uBC1C\uACAC\uD558\uC5EC \uB378\uB9B0\uC800 \uD604\uC0C1\uC774\uB77C\uACE0 \uBD88\uB9B0\uB2E4. \uD0DC\uC591\uBA74\uC758 \uD3ED\uBC1C\uB85C \uAC11\uC790\uAE30 \uB9CE\uC740 \uC591\uC774 \uBC29\uCD9C\uB418\uB294 \uC804\uC790\uAE30\uD30C\uAC00 \uC9C0\uAD6C \uC804\uB9AC\uCE35\uC758 \uC774\uC628\uACFC \uCDA9\uB3CC\uD558\uBA74\uC11C \uC804\uC790\uC758 \uBC00\uB3C4\uB97C \uD06C\uAC8C \uC99D\uAC00\uC2DC\uCF1C \uC774\uB85C \uC778\uD574 \uC77C\uC2DC\uC801\uC73C\uB85C \uB2E8\uD30C\uBB34\uC120\uD1B5\uC2E0\uC774 \uB04A\uC5B4\uC9C0\uB294 \uC804\uD30C\uC758 \uC7A5\uC560 \uD604\uC0C1\uC744 \uB9D0\uD55C\uB2E4. \uAD6D\uC81C\uD1B5\uC2E0\uC758 \uB450\uC808\uC740 \uCD5C\uC18C 5~10\uBD84, \uCD5C\uB300\uB294 \uC218 \uC2DC\uAC04\uAE4C\uC9C0 \uACC4\uC18D\uB41C\uB2E4. 1935\uB144 \uD0DC\uC591\uC758 \uC790\uC804\uC8FC\uAE30\uC5D0 \uB530\uB77C \uC804\uD30C\uC758 \uC774\uC0C1\uAC10\uC1C4 \uD604\uC0C1\uC744 \uBC1C\uACAC\uD558\uACE0 \uADF8\uAC83\uC774 \uD0DC\uC591 \uC790\uC804\uC8FC\uAE30\uC758 2\uBC30\uC778 55\uC77C\uB9C8\uB2E4 \uC77C\uC5B4\uB098\uB294 \uACBD\uD5A5\uC774 \uC788\uB2E4\uB294 \uAC83\uC744 \uC9C0\uC801\uD55C \uBBF8\uAD6D\uC758 \uBB3C\uB9AC\uD559\uC790 J. H. \uB378\uB9B0\uC800\uC758 \uC774\uB984\uC774 \uBD99\uC5EC\uC84C\uB2E4."@ko . .