SDO HMI 2014-08-23 16:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 110.84 | 592.51 | 56.44 | 301.34 | 8.73 | 343.90 | 13.00 | 278.53 | 0.2270 | -569.9 | -298.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.44 | 0.00 | 0.75 | 12.68 | 347.83 | 16.93 | 290.20 | 0.3040 | -887.0 | -696.1 | |
| 0.00 | 2.60 | 0.00 | 1.34 | 8.85 | 346.87 | 15.97 | 277.83 | 0.2756 | 860.0 | 623.2 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 8.55 | 346.82 | 15.92 | 276.75 | 0.2743 | 836.0 | 527.9 | |
| 8.26 | 14.64 | 4.27 | 7.57 | 12.28 | 346.93 | 16.03 | 289.81 | 0.2880 | -1088.2 | -787.4 | |
| 0.00 | 1.80 | 0.00 | 0.93 | 13.08 | 346.92 | 16.01 | 292.43 | 0.2920 | -573.0 | -545.5 | |
| 1.71 | 5.39 | 0.88 | 2.78 | 13.05 | 345.79 | 14.88 | 293.71 | 0.2745 | 988.6 | 688.9 | |
| 2.25 | 5.30 | 1.15 | 2.71 | 7.23 | 345.47 | 14.57 | 271.91 | 0.2508 | -1108.7 | -845.4 | |
| 5.57 | 431.77 | 2.84 | 219.51 | 7.85 | 344.86 | 13.96 | 274.52 | 0.2408 | -1064.5 | -476.9 | |
| 0.99 | 3.59 | 0.51 | 1.84 | 13.63 | 344.79 | 13.89 | 297.10 | 0.2632 | 934.5 | 778.7 | |
| 0.00 | 2.25 | 0.00 | 1.14 | 7.71 | 344.51 | 13.61 | 273.99 | 0.2347 | -1055.0 | -742.2 | |
| 0.00 | 2.43 | 0.00 | 1.24 | 13.49 | 344.59 | 13.69 | 296.90 | 0.2592 | 967.0 | 748.8 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 6.36 | 344.22 | 13.31 | 268.12 | 0.2300 | 652.0 | 509.6 | |
| 1.08 | -8.00 | 0.55 | -8.00 | 8.33 | 344.25 | 13.35 | 276.70 | 0.2310 | -855.0 | 999999 | |
| 0.00 | 4.85 | 0.00 | 2.47 | 7.57 | 344.22 | 13.32 | 273.42 | 0.2298 | -15.0 | -205.1 | |
| 8.35 | 79.94 | 4.25 | 40.61 | 6.70 | 343.92 | 13.01 | 269.56 | 0.2246 | 918.9 | 277.4 | |
| 0.00 | 1.98 | 0.00 | 1.01 | 12.58 | 344.12 | 13.22 | 294.33 | 0.2460 | -980.0 | -810.0 | |
| 73.02 | -8.00 | 37.11 | -8.00 | 8.83 | 343.80 | 12.89 | 279.10 | 0.2243 | -1458.0 | 999999 | |
| 1.53 | -15.00 | 0.78 | -15.00 | 7.37 | 343.75 | 12.84 | 272.58 | 0.2216 | -805.9 | 999999 | |
| 2.51 | -15.00 | 1.28 | -15.00 | 6.47 | 343.63 | 12.72 | 268.45 | 0.2199 | 1049.6 | 999999 | |
| 4.85 | -15.00 | 2.46 | -15.00 | 6.83 | 343.57 | 12.67 | 270.11 | 0.2188 | 1027.5 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 7.53 | 343.50 | 12.60 | 273.33 | 0.2175 | -754.0 | -545.0 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 6.72 | 343.35 | 12.45 | 269.55 | 0.2150 | 1002.0 | 833.5 | |
| 0.00 | 4.13 | 0.00 | 2.09 | 6.51 | 343.16 | 12.25 | 268.54 | 0.2119 | 1014.0 | 854.0 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 7.24 | 342.87 | 11.96 | 272.04 | 0.2067 | 770.0 | 642.1 | |
| 0.00 | 3.95 | 0.00 | 2.01 | 13.13 | 343.07 | 12.17 | 298.17 | 0.2338 | -997.0 | -821.0 | |
| 0.00 | 4.76 | 0.00 | 2.41 | 7.46 | 342.62 | 11.72 | 273.13 | 0.2026 | 149.0 | 166.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 11.88 | 342.15 | 11.25 | 294.68 | 0.2110 | -834.0 | -814.9 | |
| 0.00 | 1.80 | 0.00 | 0.91 | 12.91 | 340.97 | 10.06 | 301.70 | 0.2011 | 844.0 | 663.6 | |
| 0.72 | 2.34 | 0.36 | 1.18 | 13.18 | 340.92 | 10.01 | 303.01 | 0.2027 | 1000.0 | 816.2 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 10.02 | 340.80 | 9.89 | 287.99 | 0.1787 | 869.0 | 770.1 | |
| 0.00 | 2.07 | 0.00 | 1.04 | 9.88 | 340.61 | 9.70 | 287.49 | 0.1748 | 762.0 | 661.3 | |
| 0.00 | 1.98 | 0.00 | 0.99 | 9.30 | 340.56 | 9.65 | 284.33 | 0.1716 | 839.0 | 655.2 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 9.58 | 340.44 | 9.54 | 286.06 | 0.1708 | 984.0 | 888.9 | |
| 0.00 | 2.43 | 0.00 | 1.22 | 9.19 | 340.24 | 9.34 | 284.07 | 0.1659 | 1084.0 | 843.8 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 13.76 | 339.61 | 8.71 | 309.10 | 0.1903 | 842.0 | 619.5 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 12.66 | 337.91 | 7.01 | 310.03 | 0.1561 | 875.0 | 654.5 | |
| 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. | |