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Solar magnetic field confinement and coronal mass ejection / Alshaimaa Saad Ameen ; Supervised Shahinaz Mostafa Youssef , Ashraf Hamdy Owis

By: Contributor(s): Material type: TextTextLanguage: English Publication details: Cairo : Alshaimaa Saad Ameen , 2012Description: 139P. : facsimiles ; 25cmOther title:
  • احتباس المجال المغناطيسى وقذف مادة الاكليل الشمسى [Added title page title]
Subject(s): Online resources: Available additional physical forms:
  • Issued also as CD
Dissertation note: Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology Summary: A magnetic field possesses a known property that it tends to expand in electrically highly conducting plasmas . In stellar atmospheres , particularly in the solar corona , the atmospere has no boundary that faces the magnetic field to be self confined , but other factors such as gravity provide a suitable constraint . From times to times this confinement fails at some regions leading to the release of some of the atmospheric material
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Item type Current library Home library Call number Copy number Status Barcode
Thesis Thesis قاعة الرسائل الجامعية - الدور الاول المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2012.Al.S (Browse shelf(Opens below)) Not for loan 01010110058863000
CD - Rom CD - Rom مخـــزن الرســائل الجـــامعية - البدروم المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2012.Al.S (Browse shelf(Opens below)) 58863.CD Not for loan 01020110058863000

Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology

A magnetic field possesses a known property that it tends to expand in electrically highly conducting plasmas . In stellar atmospheres , particularly in the solar corona , the atmospere has no boundary that faces the magnetic field to be self confined , but other factors such as gravity provide a suitable constraint . From times to times this confinement fails at some regions leading to the release of some of the atmospheric material

Issued also as CD

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