Sun  ID: 2404

First Flare Movie for the RHESSI Instrument (Speed 26x Normal)

Visualizations by Tom Bridgman Released on March 20, 2002
An animation of an M-class flare viewed by the RHESSI instrument on February 20, 2002. On tape, this version plays at a speed of four video frames corresponding to 3.75 seconds of data collection time. The flare was located at -17.8 degrees South, 9.8 degrees West (heliographic coordinates) in NOAA active region number 9830.
Download Options
Movie zoomed in on the RHESSI flare and played at a slower speed.
Download Options
Full Sun at 195 angstroms from SOHO-EIT.
Download Options
First x-ray flash visible to RHESSI. The color scale runs from red (low intensity) thru green to blue (highest intensity).
Download Options
First flare location fades as second flash is on the rise.
Download Options
X-rays from the second portion of this flare event.
Download Options
The event in Hydrogen-alpha from Big Bear Solar Observatory. Early stage of gas ejection.
Download Options
The event in Hydrogen-alpha from Big Bear Solar Observatory. Later stage of gas ejection.
Download Options
Video slate image reads "HESSI's first M-class X-ray flare February 20, 2002. Quarter speed version.".

For More Information

http://www.gsfc.nasa.gov/topstory/20020320hessixray.html

Visualization Credits

Tom Bridgman (Global Science and Technology, Inc.): Lead Animator
Brian Dennis (NASA/GSFC): Scientist
Robert Lin (University of California at Berkeley): Scientist
Peter T. Gallagher (L-3 Communications Analytics Corporation/GSFC): Scientist
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio

Short URL to share this page:
https://svs.gsfc.nasa.gov/2404

Missions:
RHESSI
SOHO

Data Used:
RHESSI/X-ray Imaging Spectrometer
The RHESSI instrument is an imaging spectrometer observing the Sun at X-ray to gamma-rays (photon energies of 3 keV to 17 MeV) at time resolutions of a few seconds. (eV stands for "electron volt" and is a unit of energy. Note that photons of visible light have energies of 2-3 eV. 1 keV is a thousand electron volts and 1 MeV is a million electron volts.
view all stories where this data set is used
Big Bear Solar Observatory/H-alpha Telescope/H-alpha
Observed Data - BBSO
Solar imagery in Hydrogen-alpha spectral line
view all stories where this data set is used
SOHO/Extreme-UV Imaging Telescope (EIT)/195 Filter also referred to as: SOHO/EIT 195
NASA and ESA
view all stories where this data set is used
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.

Dates of Data Used:
(2002-02-20T20:48:11.142Z)-(2002-02-20T21:23:48.068Z)

This item is part of this series:
RHESSI First Release

Keywords:
SVS >> Active Region 9830
SVS >> Hydrogen-Alpha
SVS >> SOHO
DLESE >> Space science
SVS >> X-ray
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Active Regions
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Flares
SVS >> RHESSI
NASA Science >> Sun
SVS >> Extreme Ultraviolet Imaging
SVS >> EUV Imaging
SVS >> X-ray Imaging

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