SDO HMI 2011-10-14 12:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.46 | 81.11 | 8.82 | 46.10 | 19.88 | 98.55 | 26.58 | 300.94 | 0.4924 | -470.3 | -287.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.54 | 6.29 | 2.61 | 3.62 | 20.18 | 99.72 | 27.76 | 300.49 | 0.5094 | -695.9 | -305.3 | |
| 3.23 | 50.78 | 1.85 | 28.99 | 19.67 | 99.45 | 27.48 | 299.77 | 0.5026 | -801.7 | -485.1 | |
| 4.28 | -2.00 | 2.44 | -2.00 | 19.52 | 99.28 | 27.31 | 299.63 | 0.4995 | -1096.8 | 999999 | |
| 0.00 | 2.88 | 0.00 | 1.65 | 20.14 | 99.39 | 27.43 | 300.66 | 0.5048 | -814.0 | -679.7 | |
| 1.66 | -2.00 | 0.95 | -2.00 | 19.57 | 99.03 | 27.07 | 299.89 | 0.4966 | -1081.7 | 999999 | |
| 0.00 | 3.06 | 0.00 | 1.75 | 19.97 | 98.97 | 27.00 | 300.69 | 0.4982 | -881.0 | -709.5 | |
| 0.00 | 0.52 | 0.00 | 0.30 | 19.74 | 98.60 | 26.64 | 300.55 | 0.4920 | -558.0 | -588.5 | |
| 0.00 | 1.84 | 0.00 | 1.04 | 19.75 | 98.36 | 26.39 | 300.77 | 0.4889 | -832.0 | -656.4 | |
| 0.00 | 1.75 | 0.00 | 0.98 | 19.59 | 97.16 | 25.20 | 301.46 | 0.4722 | -938.0 | -709.3 | |
| 0.00 | 6.55 | 0.00 | 3.67 | 21.06 | 96.04 | 24.08 | 305.28 | 0.4683 | 552.0 | 751.3 | |
| 1.75 | 4.46 | 0.97 | 2.46 | 20.59 | 94.57 | 22.61 | 305.90 | 0.4461 | 1027.2 | 791.4 | |
| 0.00 | 1.49 | 0.00 | 0.82 | 20.87 | 94.34 | 22.38 | 306.71 | 0.4455 | 726.0 | 638.4 | |
| 0.00 | 1.49 | 0.00 | 0.82 | 20.53 | 93.63 | 21.67 | 306.83 | 0.4338 | 841.0 | 667.1 | |
| 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. | |