SDO HMI 2011-11-15 07:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.96 | 156.84 | 58.78 | 306.75 | 19.74 | 87.83 | 75.11 | 289.72 | 0.9660 | -104.2 | -187.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.32 | 61.05 | 5.62 | 145.59 | 19.32 | 91.29 | 78.57 | 289.14 | 0.9800 | 432.3 | -111.1 | |
| 4.99 | -1.00 | 11.72 | -1.00 | 19.15 | 90.84 | 78.12 | 288.98 | 0.9785 | -499.7 | 999999 | |
| 3.35 | -1.00 | 7.78 | -1.00 | 19.69 | 90.67 | 77.95 | 289.54 | 0.9780 | -442.4 | 999999 | |
| 2.84 | 7.91 | 5.48 | 15.45 | 18.18 | 88.04 | 75.32 | 288.06 | 0.9678 | 211.0 | -194.6 | |
| 0.00 | 0.95 | 0.00 | 1.80 | 19.11 | 87.74 | 75.02 | 289.03 | 0.9667 | -368.0 | -353.5 | |
| 0.00 | 4.30 | 0.00 | 8.29 | 19.35 | 87.94 | 75.22 | 289.27 | 0.9676 | -581.0 | -419.1 | |
| 2.06 | 9.46 | 3.57 | 16.39 | 18.15 | 86.11 | 73.39 | 288.10 | 0.9593 | 223.8 | 1.9 | |
| 0.00 | 2.49 | 0.00 | 4.15 | 18.37 | 85.38 | 72.65 | 288.36 | 0.9558 | 419.0 | 260.8 | |
| 2.15 | 4.47 | 3.99 | 8.37 | 20.83 | 87.26 | 74.54 | 290.83 | 0.9650 | -460.4 | -414.2 | |
| 0.00 | 1.63 | 0.00 | 2.97 | 20.59 | 86.94 | 74.21 | 290.60 | 0.9636 | -269.0 | -204.6 | |
| 0.00 | 0.69 | 0.00 | 1.17 | 21.25 | 85.64 | 72.92 | 291.36 | 0.9579 | 288.0 | 168.5 | |
| 0.00 | 2.06 | 0.00 | 3.07 | 19.54 | 83.08 | 70.36 | 289.73 | 0.9444 | 554.0 | 346.0 | |
| 7.40 | 61.83 | 11.39 | 99.50 | 20.55 | 83.76 | 71.03 | 290.75 | 0.9484 | 375.8 | -343.0 | |
| 3.61 | -13.00 | 5.78 | -13.00 | 21.25 | 84.46 | 71.73 | 291.43 | 0.9522 | -547.1 | 999999 | |
| 2.24 | -13.00 | 3.45 | -13.00 | 20.77 | 83.80 | 71.08 | 290.97 | 0.9487 | -337.7 | 999999 | |
| 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. | |