SDO HMI 2014-07-07 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 98.03 | 608.40 | 55.82 | 346.04 | -19.30 | 255.20 | 18.82 | 218.31 | 0.4933 | 736.5 | 356.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.80 | -21.20 | 266.24 | 29.87 | 228.50 | 0.6222 | 735.0 | 611.5 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -18.44 | 265.20 | 28.82 | 231.25 | 0.5887 | -458.0 | -346.6 | |
| 0.00 | 0.36 | 0.00 | 0.23 | -19.97 | 265.38 | 29.01 | 229.33 | 0.6031 | 738.0 | 642.2 | |
| 0.00 | 0.45 | 0.00 | 0.29 | -23.19 | 265.37 | 29.00 | 225.19 | 0.6304 | 626.0 | 500.6 | |
| 0.00 | 1.64 | 0.00 | 1.01 | -20.91 | 264.64 | 28.27 | 227.39 | 0.6034 | 827.0 | 700.6 | |
| 1.00 | 4.72 | 0.61 | 2.86 | -20.93 | 262.15 | 25.78 | 224.83 | 0.5783 | 836.8 | 743.0 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -21.85 | 256.22 | 19.85 | 216.53 | 0.5315 | -784.0 | -571.8 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -22.63 | 256.16 | 19.79 | 215.52 | 0.5398 | -736.0 | -579.2 | |
| 83.59 | 534.80 | 47.44 | 303.30 | -18.96 | 255.26 | 18.88 | 218.88 | 0.4896 | 1432.3 | 419.0 | |
| 0.00 | 0.73 | 0.00 | 0.43 | -24.12 | 255.79 | 19.42 | 213.34 | 0.5541 | -404.0 | -457.8 | |
| 0.00 | 2.36 | 0.00 | 1.39 | -23.67 | 255.30 | 18.92 | 213.18 | 0.5447 | -400.0 | -327.2 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -20.31 | 254.77 | 18.40 | 216.40 | 0.5007 | -112.0 | -68.2 | |
| 1.27 | 2.82 | 0.74 | 1.65 | -22.84 | 255.00 | 18.63 | 213.70 | 0.5326 | -985.0 | -835.1 | |
| 1.54 | -9.00 | 0.88 | -9.00 | -19.37 | 254.49 | 18.11 | 217.19 | 0.4871 | 989.5 | 999999 | |
| 0.00 | 1.64 | 0.00 | 0.93 | -20.27 | 254.53 | 18.15 | 216.09 | 0.4981 | 63.0 | 78.4 | |
| 1.00 | 13.08 | 0.58 | 7.57 | -21.92 | 254.70 | 18.33 | 214.34 | 0.5191 | 507.1 | 199.1 | |
| 0.00 | 0.73 | 0.00 | 0.43 | -23.14 | 254.80 | 18.42 | 213.08 | 0.5345 | -511.0 | -458.6 | |
| 0.00 | 2.45 | 0.00 | 1.41 | -21.41 | 254.46 | 18.09 | 214.60 | 0.5110 | 916.0 | 707.2 | |
| 0.64 | -9.00 | 0.36 | -9.00 | -18.51 | 253.95 | 17.58 | 217.54 | 0.4719 | 1030.4 | 999999 | |
| 1.36 | 2.82 | 0.78 | 1.62 | -21.50 | 254.20 | 17.82 | 214.10 | 0.5099 | 833.2 | 605.6 | |
| 0.00 | 2.63 | 0.00 | 1.53 | -22.69 | 254.35 | 17.98 | 212.96 | 0.5255 | -564.0 | -584.5 | |
| 0.00 | 0.55 | 0.00 | 0.31 | -20.49 | 253.73 | 17.36 | 214.63 | 0.4937 | 718.0 | 549.3 | |
| 7.63 | 16.08 | 4.43 | 9.32 | -22.61 | 253.96 | 17.59 | 212.48 | 0.5214 | -1047.4 | -672.3 | |
| 0.00 | 0.55 | 0.00 | 0.30 | -18.17 | 253.38 | 17.01 | 217.11 | 0.4625 | 625.0 | 516.8 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -22.95 | 253.69 | 17.32 | 211.72 | 0.5234 | -250.0 | -362.3 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -20.80 | 252.75 | 16.37 | 212.73 | 0.4892 | 422.0 | 456.3 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -20.49 | 252.30 | 15.93 | 212.40 | 0.4817 | 917.0 | 773.4 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -19.13 | 252.17 | 15.79 | 213.86 | 0.4634 | -570.0 | -498.0 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -18.62 | 251.35 | 14.98 | 213.13 | 0.4499 | -785.0 | -626.4 | |
| 0.00 | 0.73 | 0.00 | 0.40 | -18.45 | 251.23 | 14.86 | 213.14 | 0.4468 | -760.0 | -645.6 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -19.17 | 251.03 | 14.66 | 211.88 | 0.4544 | -731.0 | -614.9 | |
| 0.00 | 0.64 | 0.00 | 0.36 | -20.30 | 250.67 | 14.29 | 209.92 | 0.4661 | -616.0 | -506.4 | |
| 0.00 | 1.91 | 0.00 | 1.06 | -19.78 | 249.62 | 13.24 | 208.67 | 0.4513 | -602.0 | -485.2 | |
| 0.00 | 2.18 | 0.00 | 1.21 | -19.84 | 249.09 | 12.72 | 207.64 | 0.4482 | -840.0 | -712.9 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -27.96 | 249.36 | 12.98 | 200.85 | 0.5598 | -656.0 | -527.1 | |
| 0.00 | 0.73 | 0.00 | 0.41 | -24.70 | 245.58 | 9.20 | 197.09 | 0.4963 | -643.0 | -549.4 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |