SDO HMI 2014-05-17 07:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 83.97 | 166.31 | 42.81 | 84.80 | -15.98 | 194.38 | 1.97 | 187.81 | 0.2383 | 131.9 | 304.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.51 | -17.09 | 196.20 | 3.78 | 193.98 | 0.2623 | 841.0 | 670.3 | |
| 3.15 | 67.24 | 1.61 | 34.40 | -16.16 | 195.70 | 3.29 | 193.07 | 0.2449 | 1074.9 | 623.6 | |
| 10.34 | -2.00 | 5.29 | -2.00 | -16.56 | 195.62 | 3.20 | 192.36 | 0.2513 | 1180.3 | 999999 | |
| 1.62 | -2.00 | 0.83 | -2.00 | -15.94 | 195.51 | 3.10 | 192.53 | 0.2406 | 1096.7 | 999999 | |
| 18.43 | -2.00 | 9.44 | -2.00 | -16.88 | 195.43 | 3.02 | 191.41 | 0.2559 | 1131.7 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.01 | -15.75 | 195.32 | 2.91 | 191.95 | 0.2368 | 881.0 | 717.7 | |
| 0.00 | 2.52 | 0.00 | 1.29 | -16.88 | 194.89 | 2.48 | 189.41 | 0.2542 | 853.0 | 731.0 | |
| 0.00 | 0.90 | 0.00 | 0.45 | -12.78 | 194.54 | 2.13 | 191.38 | 0.1843 | -851.0 | -654.3 | |
| 0.00 | 3.42 | 0.00 | 1.75 | -16.81 | 194.54 | 2.13 | 188.14 | 0.2523 | 895.0 | 685.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -15.56 | 194.09 | 1.68 | 187.07 | 0.2302 | -535.0 | -409.3 | |
| 7.19 | 82.16 | 3.65 | 41.78 | -15.10 | 193.71 | 1.30 | 185.68 | 0.2216 | 728.1 | -23.7 | |
| 35.06 | -11.00 | 17.83 | -11.00 | -15.44 | 193.49 | 1.08 | 184.60 | 0.2271 | -815.9 | 999999 | |
| 4.67 | -11.00 | 2.38 | -11.00 | -15.85 | 193.33 | 0.92 | 183.82 | 0.2338 | -958.9 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -14.94 | 193.11 | 0.70 | 183.12 | 0.2181 | 841.0 | 610.3 | |
| 3.51 | 5.03 | 1.78 | 2.56 | -15.32 | 192.48 | 0.07 | 180.31 | 0.2242 | -985.1 | -678.6 | |
| 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. | |