SDO HMI 2014-10-08 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 34.22 | 0.00 | 17.45 | 12.05 | 96.01 | 9.67 | 255.77 | 0.2354 | -167.6 | -179.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.50 | 9.48 | 103.80 | 17.47 | 281.50 | 0.3034 | -886.0 | -711.5 | |
| 0.00 | 1.75 | 0.00 | 0.91 | 8.88 | 103.70 | 17.37 | 279.58 | 0.3005 | -996.0 | -881.3 | |
| 0.00 | 2.54 | 0.00 | 1.32 | 8.71 | 103.41 | 17.08 | 279.13 | 0.2953 | -1030.0 | -860.0 | |
| 0.00 | 3.77 | 0.00 | 1.95 | 9.34 | 102.49 | 16.16 | 281.75 | 0.2817 | 973.0 | 831.6 | |
| 0.00 | 1.67 | 0.00 | 0.85 | 10.46 | 100.25 | 13.91 | 287.70 | 0.2493 | -671.0 | -547.2 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 10.10 | 100.17 | 13.83 | 286.38 | 0.2465 | -928.0 | -709.6 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 12.63 | 100.17 | 13.84 | 295.86 | 0.2605 | -777.0 | -687.0 | |
| 0.00 | 8.69 | 0.00 | 4.41 | 10.26 | 98.80 | 12.46 | 288.56 | 0.2251 | -815.0 | -771.9 | |
| 0.00 | 2.11 | 0.00 | 1.06 | 9.45 | 97.43 | 11.10 | 286.62 | 0.1991 | -851.0 | -716.4 | |
| 0.00 | 1.84 | 0.00 | 0.92 | 13.35 | 90.14 | 3.80 | 332.25 | 0.1393 | 887.0 | 626.5 | |
| 0.00 | 3.51 | 0.00 | 1.79 | 19.76 | 86.83 | 0.50 | 357.97 | 0.2337 | 311.0 | 370.2 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 15.03 | 84.15 | -2.18 | 13.65 | 0.1567 | 859.0 | 723.9 | |
| 0.00 | 2.72 | 0.00 | 1.36 | 14.73 | 84.09 | -2.24 | 14.50 | 0.1519 | 725.0 | 666.5 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 22.57 | 78.65 | -7.68 | 23.73 | 0.3081 | 853.0 | 668.6 | |
| 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. | |