SDO HMI 2011-11-13 06:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.27 | 380.72 | 29.75 | 212.40 | 16.09 | 64.21 | 24.58 | 299.90 | 0.4630 | -938.3 | -399.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.29 | 0.00 | 0.73 | 14.30 | 66.73 | 27.10 | 294.39 | 0.4866 | 586.0 | 369.7 | |
| 0.86 | 368.57 | 0.48 | 205.75 | 16.01 | 64.90 | 25.27 | 299.13 | 0.4717 | -572.2 | -420.1 | |
| 52.07 | -2.00 | 29.08 | -2.00 | 16.06 | 64.33 | 24.69 | 299.71 | 0.4642 | -1364.8 | 999999 | |
| 0.34 | -2.00 | 0.19 | -2.00 | 15.76 | 63.95 | 24.32 | 299.47 | 0.4571 | -1373.5 | 999999 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 14.21 | 62.46 | 22.83 | 297.65 | 0.4264 | -924.0 | -771.7 | |
| 0.00 | 0.52 | 0.00 | 0.29 | 17.54 | 62.39 | 22.76 | 304.50 | 0.4494 | -605.0 | -675.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 17.32 | 62.23 | 22.59 | 304.26 | 0.4457 | -709.0 | -580.4 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 17.02 | 62.06 | 22.42 | 303.86 | 0.4410 | -922.0 | -731.6 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 18.60 | 59.74 | 20.11 | 309.70 | 0.4253 | 841.0 | 679.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 18.39 | 59.72 | 20.08 | 309.32 | 0.4230 | 643.0 | 555.1 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 16.91 | 58.04 | 18.40 | 308.65 | 0.3884 | 733.0 | 597.6 | |
| 0.00 | 1.98 | 0.00 | 1.07 | 17.80 | 57.67 | 18.03 | 311.03 | 0.3925 | 849.0 | 709.7 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 18.46 | 56.76 | 17.12 | 313.76 | 0.3883 | 874.0 | 668.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 21.99 | 56.16 | 16.52 | 321.02 | 0.4211 | 690.0 | 541.2 | |
| 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. | |