SDO HMI 2011-02-15 18:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.59 | 57.48 | 23.36 | 53.77 | 19.70 | 64.78 | 52.38 | 298.46 | 0.8493 | 137.5 | 246.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.51 | 13.28 | 0.54 | 13.78 | 19.14 | 69.24 | 56.84 | 296.08 | 0.8825 | 205.2 | -63.7 | |
| 7.88 | -1.00 | 8.16 | -1.00 | 18.93 | 69.01 | 56.61 | 295.93 | 0.8802 | -538.9 | 999999 | |
| 0.00 | 1.28 | 0.00 | 1.32 | 19.39 | 68.46 | 56.05 | 296.63 | 0.8773 | -442.0 | -336.5 | |
| 0.00 | 0.77 | 0.00 | 0.75 | 18.35 | 67.16 | 54.76 | 295.98 | 0.8644 | -458.0 | -400.6 | |
| 0.00 | 1.20 | 0.00 | 1.19 | 19.04 | 67.34 | 54.93 | 296.67 | 0.8678 | -477.0 | -448.4 | |
| 1.20 | 1.71 | 1.18 | 1.69 | 18.87 | 67.19 | 54.79 | 296.53 | 0.8662 | -568.2 | -575.0 | |
| 3.77 | 4.71 | 3.50 | 4.38 | 19.05 | 64.84 | 52.43 | 297.66 | 0.8480 | 421.6 | 281.2 | |
| 0.00 | 3.60 | 0.00 | 3.26 | 19.88 | 63.38 | 50.97 | 299.20 | 0.8390 | 560.0 | 414.9 | |
| 7.20 | 25.53 | 6.40 | 22.67 | 19.94 | 62.61 | 50.20 | 299.60 | 0.8328 | 738.5 | 509.7 | |
| 0.00 | 1.28 | 0.00 | 1.18 | 21.82 | 63.28 | 50.88 | 301.35 | 0.8455 | -417.0 | -288.5 | |
| 4.03 | -9.00 | 3.58 | -9.00 | 20.25 | 62.40 | 49.99 | 300.03 | 0.8322 | 725.1 | 999999 | |
| 0.00 | 1.63 | 0.00 | 1.42 | 21.08 | 61.10 | 48.70 | 301.55 | 0.8248 | 441.0 | 367.7 | |
| 0.00 | 1.63 | 0.00 | 1.40 | 20.81 | 60.70 | 48.29 | 301.45 | 0.8202 | 667.0 | 523.4 | |
| 0.00 | 0.86 | 0.00 | 0.73 | 22.68 | 58.96 | 46.55 | 304.38 | 0.8139 | 597.0 | 554.2 | |
| 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. | |