Difference between revisions of "03/08/2012 11:00:00 UTC"
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*A fair ICME event, but strong solar source | *A fair ICME event, but strong solar source | ||
**X1 flare, fast CME, originated from the eastern hemisphere (~N18E42) | **X1 flare, fast CME, originated from the eastern hemisphere (~N18E42) | ||
| − | **Solar wind plasma data is corrupted. | + | **Solar wind plasma data is corrupted. |
| − | |||
=Image Data= | =Image Data= | ||
==In-Situ Data== | ==In-Situ Data== | ||
A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| − | [[File: | + | [[File:plot_sw_mag_plasma_2012030800.png|350px]] |
| − | [[File: | + | [[File:plot_sw_mag_2012030800.png|400px]] |
| − | [[File: | + | [[File:plot_sw_vel_2012030800.png|350px]] <br /> |
The blue lines are an approximation of the CME cloud and the red line denotes the shock. | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
| Line 18: | Line 17: | ||
=Video Data= | =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) | ||
| + | *Chintzoglou, G., Patsourakos, S., and Vourlidas, A., 2015, Formation of Magnetic Flux Ropes During Confined Flaring Well Before the Onset of a Pair of Major Coronal Mass Ejections, Astrophys. J., 809, 34, doi:10.1088/0004-637X/809/1/34. | ||
| + | *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. | ||
| + | *Syntelis, P,, Gontikakis, C, Patsourakos, S, and Tsinganos, K., 2016, The spectroscopic imprint of the pre-eruptive configuration resulting into two major coronal mass ejections, A&A, 588, A16. | ||
Latest revision as of 16:24, 10 March 2017
Contents
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:
Error creating thumbnail: File missing
Error creating thumbnail: File missing
Error creating thumbnail: File missing
The blue lines are an approximation of the CME cloud and the red line denotes the shock.
GOES X-RAY FLUX
Error creating thumbnail: File missing
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)
- Chintzoglou, G., Patsourakos, S., and Vourlidas, A., 2015, Formation of Magnetic Flux Ropes During Confined Flaring Well Before the Onset of a Pair of Major Coronal Mass Ejections, Astrophys. J., 809, 34, doi:10.1088/0004-637X/809/1/34.
- 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.
- Syntelis, P,, Gontikakis, C, Patsourakos, S, and Tsinganos, K., 2016, The spectroscopic imprint of the pre-eruptive configuration resulting into two major coronal mass ejections, A&A, 588, A16.
