SDO HMI 2011-10-04 07:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.20 | 329.98 | 33.99 | 260.40 | 22.98 | 156.30 | -50.34 | 65.66 | 0.7802 | -714.4 | -253.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.53 | 0.00 | 0.42 | 25.95 | 156.29 | -50.34 | 61.93 | 0.7868 | -560.0 | -503.7 | |
| 0.00 | 1.06 | 0.00 | 0.84 | 25.51 | 156.08 | -50.56 | 62.54 | 0.7878 | -509.0 | -483.5 | |
| 0.00 | 0.70 | 0.00 | 0.56 | 25.08 | 156.33 | -50.31 | 63.01 | 0.7844 | 301.0 | 286.0 | |
| 11.88 | 264.52 | 9.23 | 207.10 | 22.51 | 156.97 | -49.67 | 66.11 | 0.7725 | -1033.3 | -279.1 | |
| 22.17 | -4.00 | 17.41 | -4.00 | 22.98 | 156.48 | -50.16 | 65.62 | 0.7784 | -872.7 | 999999 | |
| 2.55 | -4.00 | 1.99 | -4.00 | 22.10 | 156.66 | -49.98 | 66.69 | 0.7748 | -714.7 | 999999 | |
| 3.61 | 54.89 | 2.93 | 44.68 | 24.11 | 155.09 | -51.55 | 64.51 | 0.7942 | -837.0 | -210.6 | |
| 2.99 | -7.00 | 2.43 | -7.00 | 23.90 | 154.89 | -51.75 | 64.81 | 0.7957 | -668.4 | 999999 | |
| 0.00 | 1.41 | 0.00 | 1.16 | 22.95 | 153.92 | -52.72 | 66.18 | 0.8032 | -441.0 | -314.8 | |
| 0.00 | 3.08 | 0.00 | 2.45 | 20.07 | 155.33 | -51.31 | 69.53 | 0.7848 | 557.0 | 512.2 | |
| 0.00 | 0.88 | 0.00 | 0.71 | 21.08 | 154.69 | -51.95 | 68.36 | 0.7927 | -467.0 | -342.5 | |
| 0.00 | 1.23 | 0.00 | 1.04 | 23.93 | 153.08 | -53.56 | 65.13 | 0.8127 | 645.0 | 570.8 | |
| 0.00 | 1.06 | 0.00 | 0.88 | 23.35 | 153.37 | -53.27 | 65.79 | 0.8090 | -348.0 | -196.7 | |
| 0.00 | 0.62 | 0.00 | 0.56 | 24.09 | 150.26 | -56.37 | 65.42 | 0.8380 | 337.0 | 381.4 | |
| 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. | |