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2013 MESSENGER FR Experiment. E.A. Jensen, C. Heiles, A. Kepley, I. Chashei, T. Howard, C. deKoning, T. Kuiper, W. Majid, M. Bisi, T. Robinshaw, R. Fallows, P. Demorest, F. Vilas. May 10, 2013. Space weather (CMEs, solar wind) Coronal heating problem (MHD waves) Approaching solar maximum - PowerPoint PPT Presentation
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2013 MESSENGER FR Experiment
E.A. Jensen, C. Heiles, A. Kepley, I. Chashei, T. Howard, C. deKoning, T. Kuiper, W. Majid, M. Bisi, T. Robinshaw, R. Fallows,
P. Demorest, F. Vilas
May 10, 2013Space weather(CMEs, solar wind)
Coronal heating problem(MHD waves)
Approaching solar maximum
Simultaneous GBT & DSN
SOHO/LASCO 2 to 5 solar radii-->electron density
remember FR gives componentof magnetic field parallel to theline of sight......weighted by the electron density & integrated
Play Movie
4
The Type 3 radio burst occurringaround 1800UT is correlatedwith the CME observedcrossing MESSENGER’sline of sight
MHD Waves
8
Figure 6 (Panel A) Monte Carlosimulated FRF spectra for 10November 2009 (black).Spectrum from Figure 4 (right,0.5 mHz highpass) is shown inblue; there are five possiblespectral lines present. (