SDO HMI 2014-08-22 23:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.44 | 438.21 | 38.95 | 217.64 | 8.93 | 343.70 | 3.45 | 300.17 | 0.0703 | -889.9 | -385.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.53 | 0.00 | 0.76 | 8.77 | 347.03 | 6.79 | 285.46 | 0.1217 | 885.0 | 690.1 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 10.42 | 346.57 | 6.32 | 299.33 | 0.1248 | 943.0 | 732.9 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 8.99 | 346.48 | 6.23 | 288.56 | 0.1137 | 875.0 | 683.9 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 6.51 | 346.29 | 6.04 | 265.98 | 0.1053 | -848.0 | -582.1 | |
| 0.00 | 3.77 | 0.00 | 1.88 | 9.12 | 346.02 | 5.77 | 291.01 | 0.1069 | 813.0 | 654.0 | |
| 72.78 | 398.93 | 36.14 | 198.13 | 8.96 | 343.74 | 3.49 | 300.19 | 0.0700 | -1485.8 | -457.7 | |
| 5.66 | 16.26 | 2.81 | 8.07 | 6.81 | 343.51 | 3.26 | 267.44 | 0.0568 | 1012.3 | 104.5 | |
| 0.00 | 1.44 | 0.00 | 0.71 | 7.48 | 343.39 | 3.14 | 279.52 | 0.0554 | -534.0 | -352.8 | |
| 0.00 | 0.99 | 0.00 | 0.49 | 12.92 | 343.39 | 3.14 | 332.77 | 0.1172 | -911.0 | -729.5 | |
| 0.00 | 1.53 | 0.00 | 0.76 | 11.80 | 342.20 | 1.95 | 338.44 | 0.0910 | -791.0 | -656.3 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 12.72 | 340.93 | 0.68 | 353.38 | 0.1013 | 912.0 | 736.1 | |
| 0.00 | 6.47 | 0.00 | 3.21 | 9.74 | 340.64 | 0.39 | 351.99 | 0.0490 | 844.0 | 750.1 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 11.77 | 340.65 | 0.40 | 355.33 | 0.0844 | 810.0 | 685.1 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 9.16 | 340.15 | -0.10 | 2.52 | 0.0385 | 679.0 | 507.4 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 12.87 | 339.28 | -0.96 | 9.07 | 0.1046 | 942.0 | 751.4 | |
| 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. | |