• Login
    View Item 
    •   Home
    • Proceedings
    • Prosiding SNPBS (Seminar Nasional Pendidikan Biologi dan Saintek)
    • Prosiding SNPBS (Seminar Nasional Pendidikan Biologi dan Saintek) Ke-2
    • View Item
    •   Home
    • Proceedings
    • Prosiding SNPBS (Seminar Nasional Pendidikan Biologi dan Saintek)
    • Prosiding SNPBS (Seminar Nasional Pendidikan Biologi dan Saintek) Ke-2
    • View Item
    JavaScript is disabled for your browser. Some features of this site may not work without it.

    Low Solar Coronal Thermal Structure Derived from Magnetohydrostatic Model

    Thumbnail
    View/Open
    fix prosiding SNPBS 2017 Final Akhir fix deal 23 AGUSTUS_p441-p444.pdf (117.1Kb)
    Date
    2017-05
    Author
    Setiahadi, Bambang
    Metadata
    Show full item record
    Abstract
    By assuming the Sun in quiet condition we derived coronal thermal structure for low solar coronal magnetoplasma atmosphere. Ideal gas law in a static equilibrium configuration in coronal magnetic plasma state is derived and the solution may be directed to figure-out the thermal structure in mixed plasma and magnetic fields within the low corona. The results show that corona may have hot and ‘cool’ solution in low corona under the condition when the Sun in quiet condition.
    URI
    http://hdl.handle.net/11617/9361
    Collections
    • Prosiding SNPBS (Seminar Nasional Pendidikan Biologi dan Saintek) Ke-2

    DSpace software copyright © 2002-2016  DuraSpace
    Contact Us | Send Feedback
    Theme by 
    Atmire NV
     

     

    Browse

    Publikasi IlmiahCommunities & CollectionsBy Issue DateAuthorsTitlesSubjectsThis CollectionBy Issue DateAuthorsTitlesSubjects

    My Account

    Login

    DSpace software copyright © 2002-2016  DuraSpace
    Contact Us | Send Feedback
    Theme by 
    Atmire NV