SDO HMI 2014-07-07 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94.66 | 615.60 | 54.29 | 352.78 | -19.41 | 255.17 | 19.90 | 219.68 | 0.5048 | 699.6 | 348.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.91 | 0.00 | 0.59 | -21.68 | 267.47 | 32.20 | 229.88 | 0.6498 | 545.0 | 444.2 | |
| 0.00 | 1.00 | 0.00 | 0.64 | -20.63 | 267.18 | 31.90 | 230.98 | 0.6388 | 584.0 | 481.4 | |
| 0.00 | 1.09 | 0.00 | 0.67 | -18.56 | 264.75 | 29.47 | 231.67 | 0.5967 | -345.0 | -407.3 | |
| 0.00 | 0.91 | 0.00 | 0.58 | -23.16 | 265.33 | 30.06 | 226.19 | 0.6404 | 553.0 | 428.3 | |
| 0.00 | 2.54 | 0.00 | 1.59 | -20.94 | 264.63 | 29.35 | 228.36 | 0.6149 | 781.0 | 647.1 | |
| 0.00 | 1.09 | 0.00 | 0.69 | -21.54 | 264.57 | 29.30 | 227.53 | 0.6193 | 632.0 | 481.1 | |
| 0.82 | 3.72 | 0.50 | 2.28 | -20.93 | 262.15 | 26.87 | 225.97 | 0.5893 | 798.2 | 732.0 | |
| 0.00 | 2.36 | 0.00 | 1.45 | -23.34 | 260.42 | 25.15 | 221.12 | 0.5954 | -275.0 | -275.7 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -22.58 | 256.22 | 20.94 | 217.08 | 0.5494 | -715.0 | -524.2 | |
| 0.00 | 0.64 | 0.00 | 0.38 | -23.09 | 256.05 | 20.77 | 216.27 | 0.5536 | -622.0 | -454.0 | |
| 77.86 | 531.38 | 44.47 | 303.34 | -18.95 | 255.18 | 19.91 | 220.35 | 0.4994 | 1462.1 | 426.9 | |
| 0.00 | 1.54 | 0.00 | 0.95 | -26.84 | 256.43 | 21.15 | 212.67 | 0.5987 | -705.0 | -512.4 | |
| 2.36 | -11.00 | 1.36 | -11.00 | -19.61 | 255.16 | 19.89 | 219.42 | 0.5065 | 896.6 | 999999 | |
| 1.45 | 3.45 | 0.86 | 2.03 | -22.83 | 255.12 | 19.85 | 215.37 | 0.5427 | -933.4 | -772.8 | |
| 3.54 | 12.63 | 2.07 | 7.36 | -22.07 | 254.66 | 19.39 | 215.63 | 0.5300 | 268.7 | 169.2 | |
| 0.00 | 2.00 | 0.00 | 1.17 | -22.65 | 254.75 | 19.47 | 215.07 | 0.5375 | -637.0 | -558.6 | |
| 0.73 | 4.91 | 0.42 | 2.84 | -21.53 | 254.34 | 19.07 | 215.85 | 0.5209 | 834.5 | 646.0 | |
| 0.00 | 1.91 | 0.00 | 1.12 | -22.65 | 254.50 | 19.22 | 214.74 | 0.5353 | -314.0 | -298.1 | |
| 0.00 | 1.64 | 0.00 | 0.95 | -22.00 | 254.37 | 19.10 | 215.32 | 0.5267 | 574.0 | 479.4 | |
| 0.00 | 2.27 | 0.00 | 1.33 | -22.88 | 254.43 | 19.15 | 214.37 | 0.5375 | -865.0 | -682.8 | |
| 1.09 | -17.00 | 0.63 | -17.00 | -21.56 | 254.14 | 18.86 | 215.53 | 0.5195 | 843.2 | 999999 | |
| 6.81 | 16.26 | 3.98 | 9.49 | -22.74 | 254.02 | 18.75 | 213.98 | 0.5324 | -1038.0 | -621.3 | |
| 0.00 | 0.55 | 0.00 | 0.32 | -23.04 | 253.72 | 18.44 | 213.22 | 0.5334 | -553.0 | -404.7 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -22.59 | 253.59 | 18.31 | 213.54 | 0.5271 | -723.0 | -568.1 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -20.88 | 252.61 | 17.33 | 214.11 | 0.4983 | 549.0 | 488.1 | |
| 0.00 | 2.73 | 0.00 | 1.55 | -20.54 | 252.19 | 16.92 | 213.89 | 0.4906 | 787.0 | 546.5 | |
| 0.00 | 3.00 | 0.00 | 1.67 | -18.41 | 251.53 | 16.26 | 215.56 | 0.4586 | -634.0 | -483.6 | |
| 0.00 | 1.82 | 0.00 | 1.02 | -19.22 | 251.07 | 15.80 | 213.74 | 0.4647 | -815.0 | -469.3 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -20.21 | 250.80 | 15.53 | 212.08 | 0.4749 | -708.0 | -538.1 | |
| 0.00 | 2.27 | 0.00 | 1.27 | -20.03 | 249.74 | 14.47 | 210.52 | 0.4640 | -681.0 | -533.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -19.85 | 249.06 | 13.78 | 209.54 | 0.4564 | -825.0 | -645.5 | |
| 0.00 | 3.09 | 0.00 | 1.79 | -24.19 | 249.49 | 14.22 | 205.79 | 0.5169 | -268.0 | -336.2 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -27.90 | 249.32 | 14.04 | 202.40 | 0.5647 | -591.0 | -537.0 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -21.78 | 246.31 | 11.03 | 202.61 | 0.4642 | -495.0 | -406.7 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -26.61 | 246.43 | 11.15 | 199.03 | 0.5324 | -637.0 | -464.6 | |
| 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. | |