Relationship between CML and io's phase according to jupiter's actual radio storms observations
أخذت الارصادات الحقيقة للعواصف الراديوية من كوكب المشتري لموقع هاوي خلال عدة سنوات من سنة (2012-2001)، حسب خط الطول المركزي و طور القمر لكل سنة من برنامج الراديو جوفا، كانت نتائج خط الطول للعواصف الراديوية لسنة (300-180) = A 2006 و (239-15) = B و (280-60) = C الطور (260-182) = A و (109-40) = B و (26...
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Veröffentlicht in: | Iraqi Journal of Physics : a Refereed Journal Issued. 2013, Vol.11 (20), p.100-109 |
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container_title | Iraqi Journal of Physics : a Refereed Journal Issued. |
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creator | Abbud, Kamal Muhammad Ibrahim, Rasha Hashim |
description | أخذت الارصادات الحقيقة للعواصف الراديوية من كوكب المشتري لموقع هاوي خلال عدة سنوات من سنة (2012-2001)، حسب خط الطول المركزي و طور القمر لكل سنة من برنامج الراديو جوفا، كانت نتائج خط الطول للعواصف الراديوية لسنة (300-180) = A 2006 و (239-15) = B و (280-60) = C الطور (260-182) = A و (109-40) = B و (260-200) = C و كانت قريبة للنتائج النظرية، خط الطول (300-180) = A و (240-15) = B و (280 – 60) = C و الطور (260-180) = A و (110-40) = B و (260-60) = C.
The actual observations for Jupiter radio storm were taken for Hawaii station within multi years from 2001 to 2012. The Central Meridian Longitude (CMLІІІ) and Io's phase (γIo) were calculated for each year from Radio Jove program, the results of CMLІІІ for year 2006 was A = (180-300)º, B = (15-239)º, C = (60-280)º, phase was A = (182-260)º, B = (40-109)º, C = (200-260)º, which were close to the theoretical values, longitude was A = (180-300)º, B = (15-240)º, C = (60-280)º and phase was A = (180-260)º, B = (40-110)º and C = (200-260)º. |
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The actual observations for Jupiter radio storm were taken for Hawaii station within multi years from 2001 to 2012. The Central Meridian Longitude (CMLІІІ) and Io's phase (γIo) were calculated for each year from Radio Jove program, the results of CMLІІІ for year 2006 was A = (180-300)º, B = (15-239)º, C = (60-280)º, phase was A = (182-260)º, B = (40-109)º, C = (200-260)º, which were close to the theoretical values, longitude was A = (180-300)º, B = (15-240)º, C = (60-280)º and phase was A = (180-260)º, B = (40-110)º and C = (200-260)º.</description><identifier>ISSN: 2070-4003</identifier><language>ara ; eng</language><publisher>Baghdad, Iraq: University of Baghdad, College of Science</publisher><subject>Antenna arrays ; Antennas (Electronics) ; Wireless communication systems ; الهوائيات</subject><ispartof>Iraqi Journal of Physics : a Refereed Journal Issued., 2013, Vol.11 (20), p.100-109</ispartof><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,778,782</link.rule.ids></links><search><creatorcontrib>Abbud, Kamal Muhammad</creatorcontrib><creatorcontrib>Ibrahim, Rasha Hashim</creatorcontrib><title>Relationship between CML and io's phase according to jupiter's actual radio storms observations</title><title>Iraqi Journal of Physics : a Refereed Journal Issued.</title><description>أخذت الارصادات الحقيقة للعواصف الراديوية من كوكب المشتري لموقع هاوي خلال عدة سنوات من سنة (2012-2001)، حسب خط الطول المركزي و طور القمر لكل سنة من برنامج الراديو جوفا، كانت نتائج خط الطول للعواصف الراديوية لسنة (300-180) = A 2006 و (239-15) = B و (280-60) = C الطور (260-182) = A و (109-40) = B و (260-200) = C و كانت قريبة للنتائج النظرية، خط الطول (300-180) = A و (240-15) = B و (280 – 60) = C و الطور (260-180) = A و (110-40) = B و (260-60) = C.
The actual observations for Jupiter radio storm were taken for Hawaii station within multi years from 2001 to 2012. The Central Meridian Longitude (CMLІІІ) and Io's phase (γIo) were calculated for each year from Radio Jove program, the results of CMLІІІ for year 2006 was A = (180-300)º, B = (15-239)º, C = (60-280)º, phase was A = (182-260)º, B = (40-109)º, C = (200-260)º, which were close to the theoretical values, longitude was A = (180-300)º, B = (15-240)º, C = (60-280)º and phase was A = (180-260)º, B = (40-110)º and C = (200-260)º.</description><subject>Antenna arrays</subject><subject>Antennas (Electronics)</subject><subject>Wireless communication systems</subject><subject>الهوائيات</subject><issn>2070-4003</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqFjD0LwjAUADMoWLQ_QXibUyH9ULsXxUEXcS-v7auNtEnISxX_vQXdne7g4GYiSOReRpmU6UKEzKqS23gns1wmgSiv1KNXRnOnLFTkX0QaissZUDegzIbBdsgEWNfGNUrfwRt4jFZ5clPE2o_Yg8NGGWBv3MBgKib3_F5XYt5izxT-uBTr4-FWnCIa0FGLpXVqsneZZkmcy_Rf_wByZ0DS</recordid><startdate>2013</startdate><enddate>2013</enddate><creator>Abbud, Kamal Muhammad</creator><creator>Ibrahim, Rasha Hashim</creator><general>University of Baghdad, College of Science</general><scope>ADJCN</scope><scope>AHFXO</scope></search><sort><creationdate>2013</creationdate><title>Relationship between CML and io's phase according to jupiter's actual radio storms observations</title><author>Abbud, Kamal Muhammad ; Ibrahim, Rasha Hashim</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-emarefa_primary_3421803</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>ara ; eng</language><creationdate>2013</creationdate><topic>Antenna arrays</topic><topic>Antennas (Electronics)</topic><topic>Wireless communication systems</topic><topic>الهوائيات</topic><toplevel>online_resources</toplevel><creatorcontrib>Abbud, Kamal Muhammad</creatorcontrib><creatorcontrib>Ibrahim, Rasha Hashim</creatorcontrib><collection>الدوريات العلمية والإحصائية - e-Marefa Academic and Statistical Periodicals</collection><collection>معرفة - المحتوى العربي الأكاديمي المتكامل - e-Marefa Academic Complete</collection><jtitle>Iraqi Journal of Physics : a Refereed Journal Issued.</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abbud, Kamal Muhammad</au><au>Ibrahim, Rasha Hashim</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Relationship between CML and io's phase according to jupiter's actual radio storms observations</atitle><jtitle>Iraqi Journal of Physics : a Refereed Journal Issued.</jtitle><date>2013</date><risdate>2013</risdate><volume>11</volume><issue>20</issue><spage>100</spage><epage>109</epage><pages>100-109</pages><issn>2070-4003</issn><abstract>أخذت الارصادات الحقيقة للعواصف الراديوية من كوكب المشتري لموقع هاوي خلال عدة سنوات من سنة (2012-2001)، حسب خط الطول المركزي و طور القمر لكل سنة من برنامج الراديو جوفا، كانت نتائج خط الطول للعواصف الراديوية لسنة (300-180) = A 2006 و (239-15) = B و (280-60) = C الطور (260-182) = A و (109-40) = B و (260-200) = C و كانت قريبة للنتائج النظرية، خط الطول (300-180) = A و (240-15) = B و (280 – 60) = C و الطور (260-180) = A و (110-40) = B و (260-60) = C.
The actual observations for Jupiter radio storm were taken for Hawaii station within multi years from 2001 to 2012. The Central Meridian Longitude (CMLІІІ) and Io's phase (γIo) were calculated for each year from Radio Jove program, the results of CMLІІІ for year 2006 was A = (180-300)º, B = (15-239)º, C = (60-280)º, phase was A = (182-260)º, B = (40-109)º, C = (200-260)º, which were close to the theoretical values, longitude was A = (180-300)º, B = (15-240)º, C = (60-280)º and phase was A = (180-260)º, B = (40-110)º and C = (200-260)º.</abstract><cop>Baghdad, Iraq</cop><pub>University of Baghdad, College of Science</pub><tpages>10</tpages></addata></record> |
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subjects | Antenna arrays Antennas (Electronics) Wireless communication systems الهوائيات |
title | Relationship between CML and io's phase according to jupiter's actual radio storms observations |
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