Sun  ID: 3286

Flight through the Coronal Loops

Here we illustrate the potential benefits of the 3-D views of the Sun which STEREO will provide. Starting with a simple 2-D EIT ultraviolet image from SOHO, we transition to a 3-D model and move through the coronal loops which are constructed along solar magnetic fields. The solar model is constructed from magnetogram data collected by SOHO/MDI. Because we do not see the full solar surface at any one time, the magnetograms collected over the course of a solar rotation are processed through a time-evolving solar surface model to provide a snapshot of the surface at a fixed time. The resulting magnetogram is then processed through the Potential Field Source Surface (PFSS) model. Coronal loops are visible at the higher temperatures of ultraviolet light, in this case, 195 angstroms, the filter wavelength of SOHO/EIT. For this version, we color the coronal loops green for ready comparison to the EIT 195 angstrom imagery using the EIT 'standard color table'.
 

Newer Versions


Visualization Credits

Tom Bridgman (GST): Lead Animator
Michael Kaiser (NASA/GSFC): Scientist
Therese Kucera (NASA/GSFC): Scientist
Don Michels (NRL): Scientist
Russ Howard (NRL): Scientist
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio

Short URL to share this page:
http://svs.gsfc.nasa.gov/3286

Mission:
SOHO

Data Used:
SOHO/Michelson Doppler Interferometer (MDI)/Magnetogram 2001-12-09
SOHO/Extreme-UV Imaging Telescope (EIT)/195 Filter 2001-12-09
PFSS/Magnetic Field Lines 2001-12-09
Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.

This item is part of this series:
STEREO Pre-launch

Keywords:
SVS >> Coronal Loop
SVS >> SOHO
SVS >> Sun
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Ultraviolet
SVS >> Stereo Display
NASA Science >> Sun

GCMD keywords can be found on the Internet with the following citation: Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version 8.0.0.0.0