SDO HMI 2014-04-17 11:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.42 | 332.62 | 31.51 | 176.37 | -9.37 | 247.31 | 20.59 | 257.54 | 0.3566 | 351.7 | 199.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.57 | 0.00 | 1.38 | -6.89 | 249.57 | 22.84 | 265.09 | 0.3885 | 899.0 | 626.8 | |
| 36.93 | 210.85 | 19.79 | 112.89 | -9.11 | 249.00 | 22.28 | 259.20 | 0.3827 | 1369.4 | 470.0 | |
| 0.27 | -2.00 | 0.14 | -2.00 | -9.43 | 248.63 | 21.91 | 258.23 | 0.3776 | 992.7 | 999999 | |
| 0.00 | 1.86 | 0.00 | 0.99 | -10.19 | 248.58 | 21.86 | 256.23 | 0.3789 | 566.0 | 475.1 | |
| 0.97 | -2.00 | 0.52 | -2.00 | -9.68 | 248.45 | 21.72 | 257.50 | 0.3753 | 1094.0 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -8.26 | 248.26 | 21.54 | 261.21 | 0.3692 | 811.0 | 719.0 | |
| 1.95 | 4.96 | 1.04 | 2.64 | -8.57 | 248.18 | 21.46 | 260.36 | 0.3685 | 1114.9 | 845.4 | |
| 0.00 | 2.75 | 0.00 | 1.46 | -8.62 | 247.66 | 20.94 | 260.06 | 0.3603 | 833.0 | 684.1 | |
| 0.00 | 7.79 | 0.00 | 4.12 | -10.33 | 246.79 | 20.07 | 254.86 | 0.3512 | -933.0 | -739.6 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -8.87 | 246.34 | 19.62 | 258.82 | 0.3397 | 814.0 | 668.8 | |
| 2.39 | 7.97 | 1.26 | 4.20 | -10.32 | 246.37 | 19.64 | 254.65 | 0.3444 | -1080.7 | -281.1 | |
| 0.53 | -11.00 | 0.28 | -11.00 | -10.33 | 245.98 | 19.25 | 254.37 | 0.3383 | 905.2 | 999999 | |
| 0.00 | 1.42 | 0.00 | 0.74 | -8.82 | 244.73 | 18.01 | 258.17 | 0.3135 | 860.0 | 616.9 | |
| 0.00 | 3.28 | 0.00 | 1.71 | -10.36 | 244.69 | 17.96 | 253.35 | 0.3181 | -686.0 | -603.9 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -9.07 | 244.58 | 17.86 | 257.32 | 0.3118 | 979.0 | 818.8 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -10.88 | 244.59 | 17.87 | 251.69 | 0.3187 | -725.0 | -642.8 | |
| 0.00 | 3.54 | 0.00 | 1.85 | -10.77 | 244.36 | 17.63 | 251.85 | 0.3146 | -720.0 | -695.0 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -10.38 | 244.24 | 17.52 | 252.96 | 0.3110 | -792.0 | -676.6 | |
| 3.01 | 4.07 | 1.56 | 2.12 | -8.45 | 244.11 | 17.38 | 259.06 | 0.3024 | 1025.1 | 768.8 | |
| 0.00 | 3.54 | 0.00 | 1.84 | -10.47 | 244.05 | 17.33 | 252.51 | 0.3084 | -1011.0 | -828.9 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -9.45 | 243.87 | 17.15 | 255.64 | 0.3015 | -523.0 | -318.5 | |
| 0.00 | 2.83 | 0.00 | 1.47 | -10.15 | 243.81 | 17.09 | 253.34 | 0.3032 | -839.0 | -771.8 | |
| 0.00 | 2.48 | 0.00 | 1.29 | -10.82 | 243.65 | 16.93 | 251.07 | 0.3037 | -850.0 | -729.5 | |
| 2.04 | 7.97 | 1.06 | 4.13 | -9.88 | 243.57 | 16.85 | 254.01 | 0.2983 | -988.4 | -759.7 | |
| 0.00 | 1.95 | 0.00 | 1.01 | -9.22 | 243.51 | 16.78 | 256.15 | 0.2949 | -529.0 | -514.5 | |
| 0.00 | 0.89 | 0.00 | 0.46 | -11.12 | 243.45 | 16.72 | 249.90 | 0.3020 | -707.0 | -479.5 | |
| 1.15 | 44.28 | 0.60 | 22.90 | -9.64 | 243.34 | 16.61 | 254.61 | 0.2937 | -968.5 | -188.6 | |
| 0.00 | 1.59 | 0.00 | 0.83 | -11.28 | 243.20 | 16.48 | 249.15 | 0.2990 | -1020.0 | -866.8 | |
| 6.29 | -27.00 | 3.25 | -27.00 | -9.74 | 243.05 | 16.33 | 254.06 | 0.2895 | -1105.2 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -11.10 | 243.13 | 16.40 | 249.65 | 0.2969 | -1126.0 | -973.8 | |
| 0.97 | 2.39 | 0.50 | 1.24 | -10.71 | 243.07 | 16.35 | 250.86 | 0.2941 | -952.7 | -761.4 | |
| 0.00 | 1.51 | 0.00 | 0.78 | -9.99 | 242.75 | 16.03 | 252.95 | 0.2856 | -805.0 | -655.8 | |
| 1.59 | -27.00 | 0.82 | -27.00 | -9.48 | 242.69 | 15.97 | 254.66 | 0.2826 | 1085.7 | 999999 | |
| 1.33 | 2.75 | 0.69 | 1.42 | -10.78 | 242.57 | 15.84 | 250.11 | 0.2865 | -994.7 | -764.6 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -8.71 | 239.23 | 12.51 | 254.43 | 0.2233 | -837.0 | -634.3 | |
| 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. | |