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Title: Multi-wavelength analysis from tomography study on solar chromosphere

The Sun as the most important star for scientific laboratory in astrophysics as well as encompassing all living aspect on Earth, still holds scientific mystery. As the established model that the Sun’s energy fueled by the nuclear reaction, along with transport process to the typical Solar surface on around 6000-K temperature, many aspects still left as an open questions, such as how the chromosphere responded to the photospheric dynamics. In this preliminary work, we try to analyze the Solar chromosphere respond to the Photospheric dynamics using tomography study implementing multi-wavelength analysis observation obtained from Dutch Open Telescope. Using the Hydrogen-alpha Doppler signal as the primary diagnostic tool, we try to investigate the inter-relation between the magnetic and gas pressure dynamics that occur in the chromosphere.
Authors:
; ;  [1]
  1. Program Studi Astronomi, Jl. Ganesha No. 10, Labtek III, Lantai IV, Bandung, Jawa Barat, Indonesia 40135 nggieng@students.itb.ac.id (Indonesia)
Publication Date:
OSTI Identifier:
22391505
Resource Type:
Journal Article
Resource Relation:
Journal Name: AIP Conference Proceedings; Journal Volume: 1656; Journal Issue: 1; Conference: APS 2012: 5. Asian Physics Symposium, Bandung (Indonesia), 10-12 Jul 2012; Other Information: (c) 2015 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; ASTROPHYSICS; CHROMOSPHERE; DOPPLER BROADENING; HYDROGEN; MAGNETIC FIELDS; NUCLEAR REACTIONS; PHOTOSPHERE; SUN; TELESCOPES; TOMOGRAPHY; WAVELENGTHS