On the power spectrum of solar surface flows | Astronomy & Astrophysics (A&A)

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Table 1:

The position and amplitude of the supergranulation peak for various data sets.
Date	Instrument	FOV (Mm²)	Filter	Time slot	$\lambda_{\rm SG}$ (Mm)	$E_{\rm SG}$ (km $^3/{\rm s}^2$ )
Wide-field data
1996 May-Jul.	SOHO/MDI	global	Ni I, 676.8 nm	62d	36.4	(200)
2000 Apr. 22	TRACE	$225\times 250$	WL	$6\times 3$ h	35.6	200
2007 Apr. 24	TRACE	$238\times 275$	WL	$2\times 3.4$ h	29.8	490
2007 Mar. 13	CALAS	$290\times 216$	575 nm	$2\times 3$ h	36.4	350
Small-field data
2007 Mar. 8	Hinode/SOT	$75.9\times 76.8$	G-band	4h	no peak	220
2007 Mar. 15	Hinode/SOT	$77.3\times 33.9$	G-band	$3\times 3$ h	57/17-27	240/350
2007 Aug. 29-30	Hinode/SOT	$76.6\times 76.6$	blue	$11\times 3$ h	28.7	600
2007 Oct. 1	Hinode/SOT	$2\times (76\times76)$	blue	$2\times3.8$ h	27/31	460/545

Source LaTeX | All tables | In the text

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