| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.27 | 308.31 | 41.55 | 168.05 | 16.58 | 48.15 | -13.80 | 33.20 | 0.4179 | -286.1 | -208.4 | |
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back to the solar disc SDO HMI 2011-05-04 21:59:07 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.07 | 219.62 | 0.58 | 118.96 | 17.39 | 50.05 | -11.90 | 28.62 | 0.4125 | -636.9 | -447.4 | |
| 26.17 | -1.00 | 14.15 | -1.00 | 16.52 | 49.78 | -12.16 | 30.25 | 0.4026 | -1067.6 | 999999 | |
| 1.52 | -1.00 | 0.82 | -1.00 | 16.24 | 49.28 | -12.66 | 31.64 | 0.4029 | -891.2 | 999999 | |
| 12.95 | -1.00 | 7.02 | -1.00 | 16.47 | 49.20 | -12.74 | 31.49 | 0.4066 | -1129.5 | 999999 | |
| 1.52 | -1.00 | 0.82 | -1.00 | 16.76 | 49.15 | -12.79 | 31.20 | 0.4110 | -646.2 | 999999 | |
| 1.88 | -1.00 | 1.02 | -1.00 | 16.21 | 49.09 | -12.85 | 32.06 | 0.4041 | -1016.5 | 999999 | |
| 11.25 | -1.00 | 6.12 | -1.00 | 16.54 | 48.65 | -13.30 | 32.48 | 0.4123 | -934.4 | 999999 | |
| 0.00 | 3.13 | 0.00 | 1.69 | 15.93 | 48.59 | -13.35 | 33.43 | 0.4047 | -600.0 | -516.9 | |
| 1.34 | -1.00 | 0.73 | -1.00 | 16.55 | 48.29 | -13.65 | 33.16 | 0.4155 | -714.0 | 999999 | |
| 0.00 | 5.45 | 0.00 | 2.96 | 16.26 | 48.28 | -13.66 | 33.58 | 0.4118 | -845.0 | -668.0 | |
| 0.00 | 3.66 | 0.00 | 2.00 | 16.55 | 47.93 | -14.01 | 33.82 | 0.4187 | -548.0 | -443.6 | |
| 0.00 | 1.70 | 0.00 | 0.93 | 16.82 | 47.72 | -14.23 | 33.86 | 0.4240 | -629.0 | -447.6 | |
| 0.00 | 1.70 | 0.00 | 0.93 | 16.49 | 47.58 | -14.36 | 34.56 | 0.4211 | -664.0 | -418.5 | |
| 0.00 | 2.14 | 0.00 | 1.17 | 15.98 | 47.52 | -14.42 | 35.41 | 0.4150 | -566.0 | -433.3 | |
| 0.00 | 0.71 | 0.00 | 0.39 | 15.92 | 47.30 | -14.65 | 35.91 | 0.4163 | -617.0 | -483.8 | |
| 0.00 | 1.43 | 0.00 | 0.79 | 18.32 | 46.87 | -15.07 | 33.37 | 0.4507 | -615.0 | -432.6 | |
| 0.00 | 2.32 | 0.00 | 1.29 | 18.56 | 46.62 | -15.33 | 33.50 | 0.4558 | -1021.0 | -776.8 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 14.07 | 46.98 | -14.97 | 39.38 | 0.3965 | 859.0 | 581.2 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 15.99 | 46.80 | -15.14 | 36.70 | 0.4219 | 787.0 | 561.7 | |
| 2.41 | 8.66 | 1.33 | 4.78 | 16.63 | 45.44 | -16.50 | 38.12 | 0.4428 | 956.0 | 802.1 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 16.31 | 45.31 | -16.64 | 38.81 | 0.4403 | 821.0 | 601.9 | |
| 0.00 | 2.77 | 0.00 | 1.56 | 18.76 | 44.47 | -17.48 | 36.72 | 0.4775 | 856.0 | 630.7 | |
| 0.00 | 1.16 | 0.00 | 0.64 | 15.33 | 44.80 | -17.14 | 41.16 | 0.4338 | 868.0 | 706.7 | |
| 0.00 | 1.79 | 0.00 | 1.00 | 17.52 | 44.60 | -17.35 | 38.21 | 0.4615 | 884.0 | 638.4 | |
| 8.75 | 17.24 | 4.84 | 9.53 | 16.13 | 44.53 | -17.41 | 40.34 | 0.4459 | 989.3 | 785.5 | |
| 0.00 | 3.04 | 0.00 | 1.70 | 17.50 | 44.27 | -17.68 | 38.77 | 0.4644 | 754.0 | 748.2 | |
| 4.64 | 13.67 | 2.58 | 7.59 | 16.66 | 44.15 | -17.79 | 40.16 | 0.4558 | 863.3 | 888.3 | |
| 1.43 | -25.00 | 0.79 | -25.00 | 16.05 | 44.18 | -17.77 | 41.04 | 0.4485 | 917.9 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.69 | 15.60 | 44.18 | -17.76 | 41.72 | 0.4433 | 810.0 | 660.8 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 16.86 | 43.90 | -18.05 | 40.26 | 0.4606 | 693.0 | 584.2 | |
| 0.00 | 1.52 | 0.00 | 0.86 | 18.39 | 43.67 | -18.27 | 38.44 | 0.4806 | 785.0 | 594.6 | |
| 0.00 | 1.34 | 0.00 | 0.75 | 16.44 | 43.81 | -18.14 | 41.02 | 0.4568 | 772.0 | 626.7 | |
| 0.00 | 1.25 | 0.00 | 0.70 | 16.28 | 43.66 | -18.29 | 41.49 | 0.4565 | 715.0 | 567.1 | |
| 1.34 | 4.91 | 0.75 | 2.76 | 17.68 | 43.25 | -18.70 | 40.06 | 0.4766 | 818.2 | 725.8 | |
| 0.00 | 3.57 | 0.00 | 2.02 | 17.88 | 43.06 | -18.89 | 40.05 | 0.4807 | 635.0 | 587.8 | |
| 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. | |