SDO HMI 2011-06-06 01:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.70 | 210.83 | 30.87 | 144.23 | -21.76 | 35.06 | 38.63 | 237.38 | 0.6905 | 104.7 | -29.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.99 | 0.00 | 1.44 | -18.94 | 40.05 | 43.62 | 243.65 | 0.7305 | -625.0 | -397.6 | |
| 0.00 | 2.35 | 0.00 | 1.68 | -18.26 | 39.53 | 43.09 | 244.31 | 0.7222 | -532.0 | -248.9 | |
| 0.00 | 1.99 | 0.00 | 1.44 | -19.52 | 39.80 | 43.36 | 242.79 | 0.7300 | 407.0 | 246.4 | |
| 0.00 | 1.27 | 0.00 | 0.90 | -18.45 | 39.24 | 42.80 | 243.94 | 0.7198 | -254.0 | -156.7 | |
| 0.27 | 34.92 | 0.19 | 24.90 | -19.19 | 39.43 | 42.99 | 243.05 | 0.7248 | 495.7 | 537.2 | |
| 13.66 | -5.00 | 9.74 | -5.00 | -19.39 | 39.05 | 42.61 | 242.63 | 0.7215 | 854.8 | 999999 | |
| 2.26 | 3.08 | 1.59 | 2.17 | -18.45 | 38.67 | 42.23 | 243.69 | 0.7135 | -386.5 | -219.2 | |
| 0.00 | 1.45 | 0.00 | 1.02 | -18.55 | 38.48 | 42.04 | 243.48 | 0.7119 | -472.0 | -243.4 | |
| 0.00 | 1.09 | 0.00 | 0.79 | -21.76 | 39.03 | 42.60 | 239.56 | 0.7314 | 556.0 | 543.5 | |
| 0.00 | 3.26 | 0.00 | 2.28 | -19.19 | 37.94 | 41.51 | 242.38 | 0.7086 | 695.0 | 617.5 | |
| 0.00 | 1.00 | 0.00 | 0.71 | -21.56 | 38.56 | 42.12 | 239.58 | 0.7257 | 547.0 | 468.9 | |
| 0.00 | 1.54 | 0.00 | 1.06 | -20.10 | 36.60 | 40.16 | 240.53 | 0.6980 | 703.0 | 555.4 | |
| 5.52 | 16.38 | 3.84 | 11.37 | -21.17 | 36.77 | 40.33 | 239.20 | 0.7050 | 598.1 | 543.4 | |
| 0.00 | 1.63 | 0.00 | 1.12 | -20.72 | 36.41 | 39.97 | 239.61 | 0.6989 | 725.0 | 677.9 | |
| 0.00 | 2.08 | 0.00 | 1.44 | -21.40 | 36.42 | 39.98 | 238.71 | 0.7023 | 552.0 | 521.8 | |
| 0.00 | 2.26 | 0.00 | 1.57 | -21.83 | 36.30 | 39.87 | 238.09 | 0.7032 | 622.0 | 463.4 | |
| 0.00 | 1.36 | 0.00 | 0.95 | -22.12 | 36.36 | 39.92 | 237.74 | 0.7053 | 490.0 | 382.6 | |
| 0.00 | 0.36 | 0.00 | 0.24 | -19.45 | 35.39 | 38.96 | 240.78 | 0.6816 | -388.0 | -532.5 | |
| 0.00 | 1.09 | 0.00 | 0.74 | -21.37 | 35.56 | 39.12 | 238.29 | 0.6930 | 574.0 | 466.8 | |
| 0.00 | 1.18 | 0.00 | 0.81 | -21.86 | 35.71 | 39.28 | 237.73 | 0.6972 | 555.0 | 484.7 | |
| 0.00 | 1.72 | 0.00 | 1.20 | -24.18 | 35.28 | 38.84 | 234.50 | 0.7052 | -532.0 | -397.9 | |
| 0.00 | 1.99 | 0.00 | 1.31 | -20.00 | 33.41 | 36.97 | 238.92 | 0.6622 | -695.0 | -540.9 | |
| 5.16 | 31.76 | 3.50 | 21.57 | -22.72 | 34.18 | 37.75 | 235.73 | 0.6856 | 710.2 | 211.9 | |
| 1.72 | -23.00 | 1.16 | -23.00 | -22.91 | 33.96 | 37.52 | 235.33 | 0.6844 | 801.9 | 999999 | |
| 6.70 | 9.32 | 4.59 | 6.39 | -24.14 | 34.16 | 37.72 | 233.87 | 0.6936 | -644.2 | -418.4 | |
| 0.00 | 1.81 | 0.00 | 1.21 | -22.35 | 33.16 | 36.72 | 235.58 | 0.6726 | 289.0 | 177.2 | |
| 0.00 | 1.45 | 0.00 | 0.96 | -21.86 | 32.76 | 36.33 | 235.99 | 0.6655 | -704.0 | -595.5 | |
| 0.72 | 72.83 | 0.49 | 48.58 | -23.51 | 33.15 | 36.72 | 234.05 | 0.6795 | 310.1 | -419.6 | |
| 0.00 | 2.17 | 0.00 | 1.43 | -21.70 | 32.27 | 35.83 | 235.90 | 0.6591 | -591.0 | -635.1 | |
| 0.00 | 3.71 | 0.00 | 2.44 | -22.16 | 32.24 | 35.80 | 235.26 | 0.6616 | -803.0 | -717.2 | |
| 5.16 | -28.00 | 3.43 | -28.00 | -23.01 | 32.46 | 36.02 | 234.26 | 0.6692 | -846.5 | 999999 | |
| 3.53 | -28.00 | 2.34 | -28.00 | -22.75 | 32.21 | 35.78 | 234.45 | 0.6649 | -851.2 | 999999 | |
| 0.00 | 1.99 | 0.00 | 1.33 | -23.58 | 32.22 | 35.79 | 233.36 | 0.6702 | -447.0 | -397.0 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -22.85 | 31.79 | 35.36 | 234.04 | 0.6611 | -592.0 | -538.5 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -22.12 | 29.99 | 33.55 | 233.77 | 0.6370 | -647.0 | -548.4 | |
| 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. | |