SDO HMI 2011-10-29 11:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.55 | 24.95 | 2.53 | 17.14 | 17.38 | 277.48 | 42.80 | 290.46 | 0.6943 | 188.9 | 165.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.73 | 0.00 | 1.22 | 15.46 | 279.67 | 44.99 | 287.15 | 0.7154 | 465.0 | 295.1 | |
| 3.55 | 5.89 | 2.53 | 4.20 | 16.54 | 279.94 | 45.26 | 288.59 | 0.7207 | -719.4 | -523.6 | |
| 0.00 | 3.12 | 0.00 | 2.17 | 16.66 | 278.40 | 43.72 | 289.12 | 0.7031 | -440.0 | -419.1 | |
| 0.00 | 0.69 | 0.00 | 0.49 | 18.52 | 278.84 | 44.15 | 291.58 | 0.7127 | -541.0 | -503.8 | |
| 0.00 | 1.13 | 0.00 | 0.78 | 16.83 | 278.14 | 43.46 | 289.42 | 0.7005 | -423.0 | -278.7 | |
| 0.00 | 0.61 | 0.00 | 0.42 | 17.44 | 277.55 | 42.87 | 290.45 | 0.6950 | 589.0 | 494.7 | |
| 0.00 | 2.08 | 0.00 | 1.41 | 16.96 | 276.78 | 42.10 | 289.98 | 0.6846 | 635.0 | 448.0 | |
| 0.00 | 2.34 | 0.00 | 1.58 | 17.01 | 276.50 | 41.81 | 290.13 | 0.6814 | 748.0 | 572.5 | |
| 0.00 | 0.95 | 0.00 | 0.64 | 17.25 | 276.56 | 41.88 | 290.45 | 0.6828 | 718.0 | 613.3 | |
| 0.00 | 2.08 | 0.00 | 1.40 | 17.54 | 276.35 | 41.67 | 290.93 | 0.6811 | 741.0 | 594.9 | |
| 0.00 | 0.78 | 0.00 | 0.52 | 21.09 | 274.79 | 40.11 | 296.58 | 0.6745 | 554.0 | 430.8 | |
| 0.00 | 1.30 | 0.00 | 0.86 | 21.92 | 273.94 | 39.26 | 298.12 | 0.6680 | 389.0 | 345.1 | |
| 0.00 | 1.04 | 0.00 | 0.69 | 21.73 | 273.88 | 39.20 | 297.88 | 0.6665 | 565.0 | 496.5 | |
| 0.00 | 1.21 | 0.00 | 0.76 | 16.68 | 271.45 | 36.77 | 291.31 | 0.6178 | 754.0 | 610.6 | |
| 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. | |