Difference between revisions of "03/08/2012 11:00:00 UTC"

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=References=
 
=References=
  
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*Ying Liu et al. 2013 ApJ
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- Wang, R., Liu, Y. D., Yang, Z., and Hu, H., Magnetic Field Restructuring Associated with Two Successive Solar Eruptions, 2014, Astrophys. J., 791, 84 (http://iopscience.iop.org/article/10.1088/0004-637X/791/2/84/pdf)
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- Liu, Y. D., Luhmann, J. G., Lugaz, N., Möstl, C., Davies, J. A., Bale, S. D., and Lin, R. P., On Sun-to-Earth Propagation of Coronal Mass Ejections, 2013, Astrophys. J., 769, 45 (http://iopscience.iop.org/article/10.1088/0004-637X/769/1/45/pdf)
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- Liu, Y. D., Richardson, J. D., Wang, C., and Luhmann, J. G., Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause, 2014, Astrophys. J. Lett., 788, L28 (http://iopscience.iop.org/article/10.1088/2041-8205/788/2/L28/pdf)
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- Wood, B. E., J. L. Lean, S. E. McDonald, and Y.-M. Wang (2016), Comparative ionospheric impacts and solar origins of nine strong geomagnetic storms in 2010–2015, J. Geophys. Res., 121, 4938–4965, doi:10.1002/2015JA021953.
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- Patsourakos, S. et al., The Major Geoeffective Solar Eruptions of 2012 March 7: Comprehensive Sun-To-Earth Analysis, Astrophys. J., 817, 14, 2016

Revision as of 13:02, 6 March 2017

Comment Section

  • A fair ICME event, but strong solar source
    • X1 flare, fast CME, originated from the eastern hemisphere (~N18E42)
    • Solar wind plasma data is corrupted.

Image Data

In-Situ Data

A combination of SWEPAM and MAG data from the ACE Satellite:

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The blue lines are an approximation of the CME cloud and the red line denotes the shock.

GOES X-RAY FLUX

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The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time.

Video Data

References

- Wang, R., Liu, Y. D., Yang, Z., and Hu, H., Magnetic Field Restructuring Associated with Two Successive Solar Eruptions, 2014, Astrophys. J., 791, 84 (http://iopscience.iop.org/article/10.1088/0004-637X/791/2/84/pdf) - Liu, Y. D., Luhmann, J. G., Lugaz, N., Möstl, C., Davies, J. A., Bale, S. D., and Lin, R. P., On Sun-to-Earth Propagation of Coronal Mass Ejections, 2013, Astrophys. J., 769, 45 (http://iopscience.iop.org/article/10.1088/0004-637X/769/1/45/pdf) - Liu, Y. D., Richardson, J. D., Wang, C., and Luhmann, J. G., Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause, 2014, Astrophys. J. Lett., 788, L28 (http://iopscience.iop.org/article/10.1088/2041-8205/788/2/L28/pdf) - Wood, B. E., J. L. Lean, S. E. McDonald, and Y.-M. Wang (2016), Comparative ionospheric impacts and solar origins of nine strong geomagnetic storms in 2010–2015, J. Geophys. Res., 121, 4938–4965, doi:10.1002/2015JA021953. - Patsourakos, S. et al., The Major Geoeffective Solar Eruptions of 2012 March 7: Comprehensive Sun-To-Earth Analysis, Astrophys. J., 817, 14, 2016

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