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Pietro Zucca, Eoin Carley, Shaun Bloomfield, Peter Gallagher

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1 Pietro Zucca, Eoin Carley, Shaun Bloomfield, Peter Gallagher
Trinity College Dublin The formation heights of CME-driven shocks using empirical Alfvén maps of the solar corona Pietro Zucca, Eoin Carley, Shaun Bloomfield, Peter Gallagher School of Physics, Trinity College Dublin, Ireland

2 Overview Shocks in the solar corona and their radio signature
Density and Alfvén speed of the solar corona Study of 2011 September 22 Type II radio burst Results and conclusions

3 Type II radio burst Plasma Emission Shock Condition
Rosse Solar Terrestrial Observatory (RSTO; Zucca et al. 2012)

4 From density to height (ne,t) ne(r) model (r,t) 2 orders of magnitude

5 Alfvén Speed Mann et al. 2002

6 Alfvén Speed 2D Model Warmuth et al. (2005)

7 Density Map with SDO/AIA and SOHO/LASCO
B-Field with PSFF Density Map with SDO/AIA and SOHO/LASCO

8 Emission Measure 18 19 20 21 22 23 Aschwanden et al. (2011)

9 Emission Measure to Density
The density can be estimated if we know the LOS length S(x,y) Menzel (1936)

10 Density with SOHO/LASCO
Hayes et al. (2001)

11 Density Models SDO/AIA data Spherical Symmetric Solution
Combined Model SOHO/LASCO data Plane Parallel Solution

12 Polar density Map SDO/AIA 1-1.3 R Model 1.3 - 2.5 R SOHO/LASCO
Electron Density [cm-3]

13 Density / Position Angle

14 Electron Density Map LASCO 2.5 R MODEL 1.3 R SDO

15 Magnetic Field zuccap@tcd.ie Magnetic field [Gauss] 0.1 0.5 2.5 15 90
500 Magnetic field [Gauss]

16 Alfvén Speed Map zuccap@tcd.ie 2 RSun Zucca et al. 2013, A&A in prep
150 300 600 1250 2500 5000 2 RSun Zucca et al. 2013, A&A in prep

17 Study of 2011 Sep 22 Type II radio burst
Using the 2D density and Alfvén maps

18 CME eruption

19 Non-radial kinematics
EUV Height time Type II Height Time

20 Height-time comparison
EUV propagating feature Type II radio burst

21 Matching Kinematics 90-70 MHz

22 Matching Kinematics 150 MHz

23 Matching Kinematics 150 MHz 150 MHz from NRH

24 Alfven Speed

25 Matching Kinematics 90-70 MHz

26 Conclusions 2D density and Alfvén maps
Non-radial study of Type II burst – CME Shock formed in the ‘Upper-flank’ region


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