Please use this identifier to cite or link to this item: https://repository.uksw.edu//handle/123456789/3080
Title: Helmet Streamer Animation Through Agnetohydrodynamics Computer Simulation Output: Space Early Warning Precursor
Authors: Setiahadi, Bambang
Keywords: CHS formation;MHD simulation;animation;solar early warning precursor
Issue Date: Mar-2012
Publisher: Fakultas Sains dan Matematika Universitas Kristen Satya Wacana
Abstract: Coronal Helmet Streamer (CHS) formation in solar corona is reproduced numerically by assuming a magnetohydrostatic coronal structure at initial condition. Magnetic emerging flux is assumed to enter the helmet structure and makes it to transform from static condition to dynamics condition. The result may give students to understand the helmet streamer formation in solar corona. The importance studying helmet streamer is its strong connection with solar storm initiation
Description: Prosiding Seminar Nasional Sains dan Pendidikan Sains VII UKSW : Pemberdayaan Manusia dan Alam yang Berkelanjutan Melalui Sains, Matematika dan Pendidikan (The Human and Nature Sustainability Empowerment through Science, Mathematic and Education) Vol. 3 No.1 2012 p45- 49
URI: http://repository.uksw.edu/handle/123456789/3080
ISSN: 2087‐0922
Appears in Collections:Bidang Fisika

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