Sun  ID: 4166

March 2014: Erupting Solar Prominence

A solar filament, in the upper left quadrant of the image, erupts from the Sun (about time stamp 2014 March 29 01:54:00 UTC).

There is a gap of 40 minutes in the data coverage, from 03:00 - 03:40 UT.
 

Related


Visualization Credits

Tom Bridgman (GST): Lead Animator
Genna Duberstein (USRA): Producer
Laurence Schuler (ADNET Systems Inc.): Project Support
Ian Jones (ADNET Systems Inc.): Project Support
William D. Pesnell (NASA/GSFC): Scientist
Please give credit for this item to:
NASA's Scientific Visualization Studio, the SDO Science Team, and the Virtual Solar Observatory.

Short URL to share this page:
http://svs.gsfc.nasa.gov/4166

Mission:
SDO

Data Used:
SDO/AIA/304 Filter
SDO/AIA/171 Filter
SDO/AIA/193 Filter
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 5

Keywords:
SVS >> Solar Wind
SVS >> Sun
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Flares
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Prominences
SVS >> Space Weather
SVS >> Heliophysics
SVS >> Corona
NASA Science >> Sun
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Coronal Mass Ejections

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