SDO HMI 2011-10-22 05:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.01 | 379.70 | 57.41 | 300.90 | 15.40 | 279.19 | -51.09 | 74.47 | 0.7801 | -350.9 | -61.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.57 | 0.00 | 1.04 | 13.45 | 288.59 | -41.69 | 75.76 | 0.6697 | -712.0 | -614.6 | |
| 0.00 | 0.96 | 0.00 | 0.64 | 13.85 | 288.17 | -42.11 | 75.25 | 0.6756 | -719.0 | -599.3 | |
| 0.00 | 1.13 | 0.00 | 0.76 | 14.08 | 288.03 | -42.25 | 74.93 | 0.6777 | -663.0 | -531.3 | |
| 0.00 | 0.87 | 0.00 | 0.58 | 13.00 | 288.19 | -42.09 | 76.50 | 0.6740 | -665.0 | -565.1 | |
| 0.00 | 0.96 | 0.00 | 0.64 | 13.01 | 287.85 | -42.43 | 76.54 | 0.6782 | -599.0 | -487.3 | |
| 0.00 | 1.22 | 0.00 | 0.84 | 13.40 | 286.29 | -43.99 | 76.22 | 0.6980 | -447.0 | -315.6 | |
| 13.84 | 288.91 | 10.57 | 224.03 | 15.60 | 280.85 | -49.43 | 74.02 | 0.7634 | -1067.8 | -192.4 | |
| 1.65 | -7.00 | 1.27 | -7.00 | 15.98 | 280.62 | -49.65 | 73.55 | 0.7663 | -742.3 | 999999 | |
| 3.92 | -7.00 | 3.03 | -7.00 | 15.96 | 280.29 | -49.98 | 73.63 | 0.7698 | -621.5 | 999999 | |
| 1.48 | -7.00 | 1.15 | -7.00 | 16.26 | 280.19 | -50.09 | 73.25 | 0.7713 | -443.6 | 999999 | |
| 4.61 | -7.00 | 3.56 | -7.00 | 15.69 | 280.34 | -49.94 | 73.97 | 0.7690 | -673.7 | 999999 | |
| 0.00 | 1.39 | 0.00 | 1.05 | 13.17 | 281.05 | -49.22 | 77.18 | 0.7585 | -550.0 | -423.6 | |
| 0.00 | 0.87 | 0.00 | 0.67 | 14.59 | 280.35 | -49.92 | 75.40 | 0.7675 | -574.0 | -564.9 | |
| 9.06 | -7.00 | 7.01 | -7.00 | 15.21 | 280.11 | -50.17 | 74.62 | 0.7709 | -809.5 | 999999 | |
| 0.35 | -7.00 | 0.27 | -7.00 | 15.14 | 279.89 | -50.39 | 74.75 | 0.7731 | -611.0 | 999999 | |
| 6.44 | -7.00 | 4.99 | -7.00 | 14.29 | 280.01 | -50.26 | 75.83 | 0.7709 | -857.9 | 999999 | |
| 12.80 | -7.00 | 9.97 | -7.00 | 14.85 | 279.78 | -50.49 | 75.12 | 0.7739 | -685.5 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.77 | 16.87 | 278.37 | -51.91 | 72.73 | 0.7909 | -640.0 | -551.1 | |
| 2.53 | 11.23 | 2.04 | 9.11 | 17.02 | 278.26 | -52.01 | 72.56 | 0.7922 | -325.6 | 241.4 | |
| 0.00 | 1.48 | 0.00 | 1.17 | 13.97 | 278.94 | -51.34 | 76.35 | 0.7821 | 117.0 | 104.7 | |
| 5.49 | 19.85 | 4.58 | 16.56 | 16.69 | 276.78 | -53.49 | 73.16 | 0.8066 | 350.4 | 524.6 | |
| 0.00 | 1.04 | 0.00 | 0.85 | 14.47 | 277.46 | -52.82 | 75.85 | 0.7978 | 574.0 | 506.0 | |
| 0.00 | 0.61 | 0.00 | 0.50 | 13.80 | 277.43 | -52.85 | 76.70 | 0.7976 | 623.0 | 530.0 | |
| 0.00 | 0.87 | 0.00 | 0.73 | 16.24 | 276.44 | -53.84 | 73.76 | 0.8096 | 437.0 | 423.0 | |
| 0.00 | 2.26 | 0.00 | 1.92 | 16.42 | 275.99 | -54.28 | 73.58 | 0.8141 | 633.0 | 524.0 | |
| 0.00 | 2.09 | 0.00 | 1.80 | 16.35 | 275.43 | -54.85 | 73.73 | 0.8195 | 719.0 | 630.8 | |
| 0.00 | 0.52 | 0.00 | 0.45 | 16.92 | 275.19 | -55.09 | 73.07 | 0.8223 | 596.0 | 558.0 | |
| 1.57 | 13.58 | 1.38 | 11.88 | 16.55 | 274.46 | -55.82 | 73.58 | 0.8288 | 542.9 | 561.6 | |
| 0.00 | 1.13 | 0.00 | 1.00 | 17.12 | 274.20 | -56.07 | 72.92 | 0.8317 | 634.0 | 547.4 | |
| 0.00 | 2.26 | 0.00 | 2.00 | 16.32 | 274.23 | -56.05 | 73.88 | 0.8308 | 676.0 | 501.0 | |
| 0.00 | 0.61 | 0.00 | 0.53 | 11.42 | 274.86 | -55.42 | 79.78 | 0.8222 | 456.0 | 431.6 | |
| 0.00 | 1.22 | 0.00 | 1.08 | 13.48 | 273.96 | -56.31 | 77.32 | 0.8315 | 479.0 | 411.3 | |
| 0.78 | 4.61 | 0.72 | 4.25 | 15.45 | 272.55 | -57.73 | 75.06 | 0.8456 | 508.4 | 431.4 | |
| 0.00 | 0.78 | 0.00 | 0.72 | 15.63 | 272.47 | -57.81 | 74.85 | 0.8464 | 322.0 | 268.0 | |
| 7.49 | 15.76 | 6.87 | 14.44 | 14.88 | 272.73 | -57.54 | 75.72 | 0.8436 | 555.5 | 326.3 | |
| 0.00 | 0.96 | 0.00 | 0.89 | 14.76 | 272.26 | -58.01 | 75.90 | 0.8478 | -202.0 | -163.7 | |
| 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. | |