PERSAMAAN MOMENTUM ANGIN MATAHARI PADA KEADAAN NON-ISOTHERMAL
The solar wind momentum equation has been derived by Parker in 1965. However, this equation is derived by assuming that the temperature of solar wind is radially constant (isothermal). Meanwhile, based on the Voyager 2 spacecraft's observation, the radial solar wind temperature is not constant...
محفوظ في:
| المؤلفون الرئيسيون: | , |
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| التنسيق: | Theses and Dissertations NonPeerReviewed |
| منشور في: |
[Yogyakarta] : Universitas Gadjah Mada
2014
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| الموضوعات: | |
| الوصول للمادة أونلاين: | https://repository.ugm.ac.id/133618/ http://etd.ugm.ac.id/index.php?mod=penelitian_detail&sub=PenelitianDetail&act=view&typ=html&buku_id=74336 |
| الوسوم: |
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| المؤسسة: | Universitas Gadjah Mada |
| الملخص: | The solar wind momentum equation has been derived by Parker in 1965.
However, this equation is derived by assuming that the temperature of solar wind
is radially constant (isothermal). Meanwhile, based on the Voyager 2 spacecraft's
observation, the radial solar wind temperature is not constant (non-isothermal). In
this study, the solar wind momentum equation derived in the non-isothermal
condition. The obtained equation then solved by Euler method using Matlab
program to obtain the relationship between the solar wind velocity with radial
distance from the Sun. |
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