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GONGMagnetograms and
Coronal Field Modeling
G.J.D. Petrie, J. Bolding, R. Clark, K. Donaldson-Hanna, J.W. Harvey, F. Hill,
C. Toner & T.M. WentzelNational Solar Observatory,
Tucson, AZ 85719
Background• GONG (Global Oscillations Network Group)
obtains 2.5’’-pixel intensity, velocity and magnetic flux images every minute from six sites worldwide
• approximately 90% duty cycle• continuous, high-cadence, low-noise photospheric
line-of-sight magnetograms• new LCD modulators and circuitry reduced
uncertainty in zero-point < 0.1 Gauss, instrumental noise about 3 G/minute
• GONG is the official provider of magnetograms for NASA’s STEREO mission.
QuickTime™ and aYUV420 codec decompressor
are needed to see this picture.
Near-real-time GONG potential magnetic field
products• Principal features of global coronal field structure are
calculated and plotted.• We thank Janet Luhmann, Yan Li and Xuepu Zhao for
source code used in the modeling.• Green represents positive polarity and red negative
polarity.• Features include coronal holes, streamer belt,
heliospheric current sheet and lines open to the ecliptic plane
• Products are produced once per hour, and movies are available at
http://gong.nso.edu/data/magmap/index.html
GONG magnetogram and modeling products to expand
• More ideas are being implemented and more are welcome
• GONG Magnetogram Users’ Group (MUG) meeting today 6.30 pm foyer
• Please exploit this new round-the-clock source of sensitive, high-cadence data http://gong.nso.edu/data/magmap/index.html