Magnetically coupled atmosphere, fast sausage MHD waves, and forced magnetic field reconnection during the SOL2014-09-10T17:45 flare

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Volume 643 (November 2020)

A&A, 643 (2020) A140

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Table 3.

Characteristic parameters of (E)UV tadpole waves – part II.

Channel	Mach	NPS ^(a)	Coefficient ^(b)	Time
	number			shift
	M₀	a_ph	CC₁₇₀₀	TS₁₇₀₀
[Å]				[s]
	Corona

94	1.05	1.32	0.82	192
131	0.99	1.18	0.85	156
171	1.11	1.22	0.89	180
193	1.06	1.03	0.90	108
211	1.11	1.22	0.89	108
335	1.06	1.09	0.90	60

Mean	1.06	1.18

	Chromosphere and transition region

304	1.15	1.02	0.87	48
1400	1.05	1.23	0.87 ^(c)	95
1600	1.22	1.59	0.98	0
2796	1.04	1.79	0.80 ^(c)	152

Mean	1.12	1.42

	Photosphere

1700	1.12	1.54

Notes.

^(a)

NPS = normalised phase speed

^(b)

coefficient = cross-correlation coefficient. (Note: We doubled each value of the AIA 1600 and 1700Å time series to get them with 12 s cadence instead of the original 24 s.

^(c)

The 1700 time series length and cadence were adapted to the IRIS time series).

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