Sun  ID: 4101

August 2013: SDO Observes Large Coronal Hole

On the Sun, coronal holes represent regions where the solar magnetic field does not connect back to the Sun. In these cases, the magnetic field guides the charged particles of the solar wind into distant space, forming the fast solar wind.

Visualization Credits

Tom Bridgman (Global Science and Technology, Inc.): Animator
Scott Wiessinger (USRA): Producer
SDO Science Team and the Virtual Solar Observatory: Scientist
Please give credit for this item to:
NASA's Goddard Space Flight Center Scientific Visualization Studio

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https://svs.gsfc.nasa.gov/4101

Mission:
SDO

Data Used:
SDO/AIA/193 Filter also referred to as: AIA 193
JOINT SCIENCE OPERATIONS CENTER
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:
Solar Dynamics Observatory: Year 4

Keywords:
SVS >> HDTV
SVS >> Solar Wind
GCMD >> Earth Science >> Sun-earth Interactions
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Ultraviolet
SVS >> Space Weather
SVS >> Hyperwall
SVS >> SDO
SVS >> Solar Dynamics Observatory
SVS >> Heliophysics
SVS >> Corona
NASA Science >> Sun
SVS >> Extreme Ultraviolet Imaging
SVS >> EUV Imaging
SVS >> Coronal Holes

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