مشاركة
دراسة وتحقيق بشان عدم استقرارية الانجراف المنحني في الغلاف المغناطيسي للنجم النابض بالقرب من منطقة الاسطوانة الضوئية == Study and Investigation of Curvature Drift Instability in Pulsar Magnetosphere Near Light Cylindrical Region
اسم المؤلف:
محمد عبد الستار عبد الرحمن
اسم المشرف:
ماجدة حمدان خضير الكبيسي
الموضوع العام:
علوم الفيزياء
السنة:
2015
الموضوع الدقيق:
الفيزياء
الدرجة:
ماجستير
الجامعة:
الجامعة المستنصرية - كلية العلوم - قسم الفيزياء
اللغة:
الانكليزية
مكان الجامعة:
بغداد
الصفحات الاولى:
26T1925 - p.pdf
المستخلص:
The case of curvature drift instability in pulsar magnetosphere is a phenomenon may be responsible of many properties including radio waves, that was studied its reasons. We studied the magnetic fields around the pulsar, and our study was nearby the light cylinder region, because the curvature of the magnetic field be greater in the light cylinder region (~ 107 cm).The value of magnetic field was calculated by using mat lab program in two ways : The standard model and relativistic model. Where the relativistic model includes two cases : flat space time and curved space time. The values of the two cases were compared, According to standard model the magnitude magnetic field component (Br ) equal to 1012 G and the magnitude magnetic field component (Bθ ) equal to 1011 G but in relativistic model equal to 1019 G and 1014 G respectively and this noticeable increasing in values because the mass factor enter in calculation , This was first part from study.The second part of the study includes the calculation of drift velocity, which was about (107 cm/sec) in standard model, The drift velocity in relativistic model was (102 cm/sec), Where the drift velocity values which can produce the curvature radiation must be in the range between (106 cm/sec) and less than the speed light.The calculated drift velocity was used to calculate the growth rate instability for each the primary particles which its Lorentz factor equal (108), the value of growth rate instability (1013 s - 1), and the energy loss rate (10 - 6 erg.s), while the secondary particles which its Lorentz factor equal to (104), the value of growth rate instability was (1015 s - 1) and the energy loss rate equal to (10 - 21 erg.s)
