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dc.contributor.authorSetiahadi, Bambang
dc.date.accessioned2016-11-01T02:29:36Z
dc.date.available2016-11-01T02:29:36Z
dc.date.issued2016-05-21
dc.identifier.citation[1]. Budhi, G.S., Adipranata, R., Setiahadi, B., Adrian, H.N. (2012), Solar Storm Type Classification Using Probabilistic Neural Network Compared with the Self-Organizing Map, Journal Ilmiah Kursor, V. 6, No. 4, pp. 211- 220. [2]. Setiahadi, B. (2005), Problems of Equilibrium and Instabilities on Solar Coronal Magnetic Fields and Its Evolution Towards Energetic Energy Liberation: Effects to Interplanetary Space, National Seminar on Mathematics, Diponegoro University, p. E.1. [3]. Setiahadi, B. (2007), Daily Observational Sunspot ASCII Data for Long- Term Solar Magnetohydrodynamo Studies at Lapan Watukosek, [4]. Setiahadi, B. (2007), Solar Observation Procedures to Obtain the Watukosek White Light Solar ASCII Data for Statistical Space Warnings, Proceedings of International conference on Rural Information and Communication Technology 2007, ITB Research Center on ICT, pp. 101-105. (ISBN 978-979-15509-1-8). [5]. Setiahadi, B. (2007), MHD Numerical Simulation of Interactions Between the Solar Storm and the Planet, Prosiding Seminar Nasional Sistem dan Teknologi Informasi (SNASTI), STIKOM, Surabaya, pp. III 1-5, (ISBN 978-979-8968-30-3). [6]. Setiahadi, B. (2009), Global MHD Simulation of the Magnetospheric Response due to Transient Solar Wind Studied at LAPAN Watukosek 2009: The Space Early Warnings, Prosiding Nasional Pascasarjana IX – ITS, Surabaya, ISBN: 978-979-96565-51 [7]. Setiahadi, B. (2010), Solar Flare Occurrence by Considering the Zurich Classification, Area of Active Region and Magnetic Topology: Warning to Solar Activity, Univ. Negeri Yogyakarta, pp. 375-385. [8]. Setiahadi, B. (2010), Magnetohydrodynamo Solar Activity Simulation Toward the Next Maunder Minimum: Interplanetary Global Cooling, Prosiding Seminar Nasional Matematika, Universitas Sebelas Maret, Surakarta, pp. 158-170, (ISBN 979-978-3456-79-1). [9]. Setiahadi, B. (2011), Solar Eruption on 4 January 2011: Case Study for Space Early Warning, Seminar Nasional Pendidikan Matematika, LSM XIX, Univ Neg Yogya, pp. 139-149, (ISBN 978-979-17763-3-2). [10]. Tandberg-Hanssen, E., Emslie, A.G. (2009), The Physics of Solar Flares, Cambridge Astrophysics Series, Cambridge Univ. Press, (ISBN 978-0-521- 11552-0 ).in_ID
dc.identifier.issn2527-533X
dc.identifier.urihttp://hdl.handle.net/11617/7903
dc.description.abstractOn early morning on 11 March 2015 a solar exceptionally energy release was calculated by MHDo observational parameters and showed there would be energy liberated by the Sun. Later we observed on 17 March 2015, we did notice geomagnetic large deviation. As preliminary conclusion we supposed that on 11 March 2015 the Sun did release huge energy into interplanetary spacein_ID
dc.language.isoenin_ID
dc.publisherUniversitas Muhammadiyah Surakartain_ID
dc.subjectSolar stormin_ID
dc.subjectenergy liberatedin_ID
dc.subjectinterplanetary effectsin_ID
dc.titleResearch and Observations On Solar Storm: Solar Warning On 11 March 2015in_ID
dc.typeArticlein_ID


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