SDO HMI 2011-02-14 22:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.69 | 88.71 | 21.77 | 66.32 | 19.91 | 64.42 | 41.05 | 304.45 | 0.7504 | 99.9 | 295.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.99 | 22.35 | 9.56 | 17.86 | 19.29 | 68.53 | 45.16 | 301.31 | 0.7856 | -707.9 | -136.4 | |
| 0.00 | 1.11 | 0.00 | 0.88 | 19.04 | 68.26 | 44.89 | 301.16 | 0.7819 | -734.0 | -540.0 | |
| 0.00 | 1.20 | 0.00 | 0.94 | 19.01 | 67.94 | 44.57 | 301.30 | 0.7788 | -695.0 | -606.6 | |
| 0.00 | 1.28 | 0.00 | 0.97 | 18.88 | 65.69 | 42.32 | 302.40 | 0.7569 | 517.0 | 410.0 | |
| 0.00 | 1.11 | 0.00 | 0.84 | 18.67 | 65.50 | 42.13 | 302.27 | 0.7539 | 529.0 | 389.1 | |
| 0.00 | 1.28 | 0.00 | 0.94 | 19.28 | 63.80 | 40.43 | 304.01 | 0.7409 | 605.0 | 573.4 | |
| 2.48 | 2.91 | 1.87 | 2.19 | 21.92 | 63.74 | 40.37 | 307.10 | 0.7557 | -496.0 | -478.4 | |
| 6.34 | 52.24 | 4.60 | 37.95 | 19.81 | 62.73 | 39.36 | 305.33 | 0.7337 | 896.1 | 461.7 | |
| 7.88 | -8.00 | 5.74 | -8.00 | 20.14 | 62.66 | 39.29 | 305.75 | 0.7350 | 813.5 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.75 | 20.53 | 62.62 | 39.25 | 306.24 | 0.7370 | -30.0 | 13.2 | |
| 0.00 | 2.23 | 0.00 | 1.63 | 23.25 | 61.04 | 37.67 | 310.42 | 0.7399 | 677.0 | 537.1 | |
| 0.00 | 0.94 | 0.00 | 0.66 | 20.59 | 59.55 | 36.18 | 308.45 | 0.7081 | 636.0 | 556.2 | |
| 0.00 | 1.03 | 0.00 | 0.71 | 21.44 | 57.95 | 34.58 | 310.66 | 0.6988 | 472.0 | 336.7 | |
| 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. | |