SDO HMI 2011-05-29 19:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.33 | 257.88 | 45.86 | 179.29 | 20.95 | 131.93 | 39.53 | 301.92 | 0.7021 | -215.3 | -226.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.87 | 5.50 | 3.43 | 3.88 | 20.32 | 133.29 | 40.90 | 300.35 | 0.7138 | -648.7 | -681.6 | |
| 0.99 | 184.72 | 0.71 | 130.85 | 22.03 | 133.79 | 41.40 | 302.28 | 0.7273 | -416.5 | -352.4 | |
| 0.72 | -2.00 | 0.52 | -2.00 | 21.90 | 133.65 | 41.26 | 302.18 | 0.7253 | -471.9 | 999999 | |
| 3.16 | -2.00 | 2.27 | -2.00 | 22.10 | 133.59 | 41.20 | 302.46 | 0.7256 | -740.9 | 999999 | |
| 6.32 | -2.00 | 4.50 | -2.00 | 21.86 | 133.34 | 40.94 | 302.30 | 0.7218 | -803.7 | 999999 | |
| 1.08 | -2.00 | 0.78 | -2.00 | 22.29 | 133.44 | 41.05 | 302.79 | 0.7251 | -547.2 | 999999 | |
| 9.11 | -2.00 | 6.46 | -2.00 | 21.50 | 133.12 | 40.73 | 301.95 | 0.7178 | -799.8 | 999999 | |
| 2.80 | -2.00 | 1.98 | -2.00 | 21.17 | 132.97 | 40.58 | 301.61 | 0.7145 | -445.1 | 999999 | |
| 2.71 | -2.00 | 1.91 | -2.00 | 21.46 | 132.72 | 40.33 | 302.12 | 0.7135 | -846.9 | 999999 | |
| 8.93 | -2.00 | 6.26 | -2.00 | 21.03 | 132.54 | 40.14 | 301.67 | 0.7094 | -897.6 | 999999 | |
| 2.44 | -2.00 | 1.71 | -2.00 | 21.29 | 132.41 | 40.02 | 302.08 | 0.7093 | -1091.6 | 999999 | |
| 2.17 | -2.00 | 1.50 | -2.00 | 20.73 | 131.93 | 39.54 | 301.61 | 0.7014 | -841.1 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.55 | 19.39 | 131.19 | 38.80 | 300.25 | 0.6865 | 338.0 | 240.1 | |
| 0.00 | 1.08 | 0.00 | 0.75 | 21.75 | 131.75 | 39.36 | 303.03 | 0.7048 | -627.0 | -503.9 | |
| 0.00 | 3.52 | 0.00 | 2.43 | 21.28 | 131.56 | 39.16 | 302.54 | 0.7003 | -790.0 | -698.5 | |
| 0.00 | 0.99 | 0.00 | 0.68 | 20.23 | 130.94 | 38.55 | 301.51 | 0.6881 | -770.0 | -609.6 | |
| 0.00 | 0.99 | 0.00 | 0.67 | 19.54 | 130.54 | 38.14 | 300.82 | 0.6801 | 455.0 | 350.6 | |
| 0.00 | 4.60 | 0.00 | 3.07 | 18.86 | 130.19 | 37.79 | 300.10 | 0.6726 | 21.0 | 182.7 | |
| 3.34 | 7.22 | 2.22 | 4.78 | 18.60 | 129.87 | 37.48 | 299.92 | 0.6677 | 684.8 | 721.5 | |
| 2.98 | 6.68 | 1.98 | 4.45 | 19.21 | 129.79 | 37.40 | 300.81 | 0.6700 | 714.1 | 399.7 | |
| 0.00 | 3.34 | 0.00 | 2.13 | 14.34 | 128.53 | 36.14 | 294.58 | 0.6305 | -665.0 | -559.1 | |
| 0.00 | 2.44 | 0.00 | 1.62 | 19.50 | 129.63 | 37.23 | 301.30 | 0.6698 | 144.0 | 136.6 | |
| 4.24 | 4.78 | 2.81 | 3.17 | 19.37 | 129.39 | 36.99 | 301.26 | 0.6664 | 670.4 | 568.8 | |
| 0.00 | 1.26 | 0.00 | 0.83 | 19.17 | 129.09 | 36.70 | 301.17 | 0.6620 | 775.0 | 586.6 | |
| 0.00 | 1.35 | 0.00 | 0.89 | 19.36 | 129.06 | 36.67 | 301.45 | 0.6628 | 736.0 | 589.2 | |
| 0.00 | 1.90 | 0.00 | 1.27 | 20.70 | 129.31 | 36.92 | 303.11 | 0.6731 | 493.0 | 331.2 | |
| 0.00 | 0.27 | 0.00 | 0.17 | 17.16 | 127.35 | 34.96 | 299.40 | 0.6306 | -352.0 | -296.3 | |
| 0.00 | 1.26 | 0.00 | 0.83 | 21.05 | 128.19 | 35.80 | 304.29 | 0.6630 | 657.0 | 487.6 | |
| 2.62 | 3.25 | 1.71 | 2.12 | 20.39 | 127.57 | 35.18 | 303.80 | 0.6522 | 751.0 | 513.1 | |
| 0.99 | 2.62 | 0.65 | 1.70 | 20.55 | 127.30 | 34.91 | 304.21 | 0.6502 | 827.4 | 697.8 | |
| 3.88 | 7.04 | 2.53 | 4.59 | 20.87 | 127.19 | 34.79 | 304.73 | 0.6510 | 736.3 | 544.5 | |
| 0.00 | 1.62 | 0.00 | 1.03 | 17.75 | 126.32 | 33.92 | 300.94 | 0.6219 | -728.0 | -592.3 | |
| 0.00 | 1.35 | 0.00 | 0.86 | 17.98 | 126.33 | 33.93 | 301.26 | 0.6234 | -447.0 | -424.3 | |
| 0.00 | 0.36 | 0.00 | 0.23 | 18.30 | 126.20 | 33.81 | 301.80 | 0.6239 | 338.0 | 468.8 | |
| 0.00 | 1.26 | 0.00 | 0.82 | 20.51 | 126.69 | 34.30 | 304.57 | 0.6433 | 904.0 | 813.1 | |
| 2.98 | 5.87 | 1.93 | 3.79 | 20.77 | 126.72 | 34.33 | 304.91 | 0.6453 | 764.3 | 745.7 | |
| 0.00 | 1.80 | 0.00 | 1.13 | 17.94 | 125.86 | 33.46 | 301.52 | 0.6176 | 694.0 | 480.4 | |
| 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. | |