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2013 MESSENGER FR Experiment

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

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2013 MESSENGER FR Experiment

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  1. 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

  2. May 10, 2013 Space 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 component of magnetic field parallel to the line of sight... ...weighted by the electron density & integrated Play Movie

  3. Dark Core

  4. The Type 3 radio burst occurring around 1800UT is correlated with the CME observed crossing MESSENGER’s line of sight 4

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  6. May 11, 2013 . X

  7. MHD Waves

  8. MHD Waves Figure 6 (Panel A) Monte Carlo simulated FRF spectra for 10 November 2009 (black). Spectrum from Figure 4 (right, 0.5 mHz highpass) is shown in blue; there are five possible spectral lines present. ( 8

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  10. Thank You! • Tokumaru-san for financial support to participate • We would like to thank Mark Perry, Jean-Luc Margot, Andy Calloway, Scott Murchie, Lu Nguyen, Dan O'Shaughnessy, Josh Steele, MESSENGER Team, Green Bank Telescope Team, Deep Space Network Team 10

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