SDO HMI 2011-02-19 06:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93.75 | 523.12 | 125.36 | 708.15 | -19.15 | 35.79 | 69.47 | 252.08 | 0.9299 | 65.2 | 64.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.18 | 0.00 | 4.93 | -17.10 | 38.93 | 72.61 | 254.26 | 0.9490 | 82.0 | 56.3 | |
| 0.00 | 0.94 | 0.00 | 1.45 | -17.39 | 38.80 | 72.48 | 253.96 | 0.9483 | 212.0 | 217.8 | |
| 4.38 | 209.18 | 7.15 | 325.27 | -18.54 | 39.93 | 73.61 | 252.72 | 0.9539 | -335.0 | 73.2 | |
| 14.25 | -3.00 | 22.79 | -3.00 | -18.52 | 39.57 | 73.25 | 252.75 | 0.9521 | 450.6 | 999999 | |
| 4.89 | -3.00 | 7.41 | -3.00 | -18.42 | 38.50 | 72.18 | 252.88 | 0.9466 | -307.8 | 999999 | |
| 15.63 | -3.00 | 23.20 | -3.00 | -18.44 | 38.02 | 71.69 | 252.86 | 0.9440 | 676.2 | 999999 | |
| 4.12 | 9.19 | 5.83 | 12.95 | -18.00 | 36.99 | 70.67 | 253.35 | 0.9383 | 506.3 | 476.9 | |
| 0.00 | 2.49 | 0.00 | 3.51 | -19.32 | 36.93 | 70.61 | 251.94 | 0.9378 | 539.0 | 404.3 | |
| 0.00 | 2.58 | 0.00 | 3.35 | -17.86 | 34.96 | 68.64 | 253.52 | 0.9260 | 482.0 | 321.0 | |
| 5.75 | 252.37 | 7.46 | 309.37 | -18.61 | 34.90 | 68.58 | 252.71 | 0.9257 | 704.8 | 77.3 | |
| 0.00 | 1.29 | 0.00 | 1.74 | -19.96 | 35.89 | 69.57 | 251.25 | 0.9318 | 455.0 | 392.3 | |
| 0.00 | 0.77 | 0.00 | 0.95 | -17.66 | 33.63 | 67.31 | 253.74 | 0.9175 | 389.0 | 354.3 | |
| 1.03 | -10.00 | 1.31 | -10.00 | -19.60 | 34.40 | 68.08 | 251.63 | 0.9225 | -216.8 | 999999 | |
| 1.03 | -10.00 | 1.32 | -10.00 | -19.81 | 34.50 | 68.18 | 251.41 | 0.9232 | -149.8 | 999999 | |
| 2.66 | -10.00 | 3.34 | -10.00 | -19.98 | 34.06 | 67.74 | 251.22 | 0.9204 | 296.3 | 999999 | |
| 0.00 | 1.12 | 0.00 | 1.42 | -20.86 | 34.36 | 68.04 | 250.27 | 0.9224 | -204.0 | -124.8 | |
| 0.00 | 0.69 | 0.00 | 0.86 | -21.04 | 34.11 | 67.79 | 250.06 | 0.9209 | -299.0 | -250.2 | |
| 6.18 | -10.00 | 7.33 | -10.00 | -19.33 | 32.54 | 66.22 | 251.89 | 0.9102 | -627.7 | 999999 | |
| 3.43 | -10.00 | 4.12 | -10.00 | -19.71 | 32.84 | 66.52 | 251.49 | 0.9124 | -372.0 | 999999 | |
| 2.40 | -10.00 | 2.92 | -10.00 | -20.36 | 33.16 | 66.84 | 250.78 | 0.9146 | -342.6 | 999999 | |
| 1.03 | 2.49 | 1.18 | 2.85 | -18.61 | 31.52 | 65.19 | 252.68 | 0.9030 | -520.7 | -439.2 | |
| 1.20 | -10.00 | 1.41 | -10.00 | -19.77 | 32.26 | 65.94 | 251.41 | 0.9084 | -772.3 | 999999 | |
| 3.52 | -10.00 | 4.17 | -10.00 | -20.21 | 32.55 | 66.23 | 250.93 | 0.9104 | -518.5 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.19 | -19.40 | 31.89 | 65.57 | 251.80 | 0.9058 | -559.0 | -552.9 | |
| 0.00 | 1.20 | 0.00 | 1.45 | -21.00 | 33.08 | 66.75 | 250.08 | 0.9141 | 37.0 | -17.1 | |
| 1.46 | -10.00 | 1.73 | -10.00 | -20.55 | 32.60 | 66.28 | 250.56 | 0.9109 | 721.5 | 999999 | |
| 0.26 | -10.00 | 0.30 | -10.00 | -20.32 | 32.40 | 66.08 | 250.81 | 0.9095 | 228.0 | 999999 | |
| 1.72 | -10.00 | 2.00 | -10.00 | -20.13 | 32.09 | 65.77 | 251.00 | 0.9073 | -767.2 | 999999 | |
| 1.12 | -10.00 | 1.31 | -10.00 | -20.62 | 32.19 | 65.87 | 250.46 | 0.9081 | 709.1 | 999999 | |
| 0.00 | 1.29 | 0.00 | 1.46 | -20.25 | 31.27 | 64.95 | 250.84 | 0.9016 | -500.0 | -369.3 | |
| 3.26 | 4.21 | 3.83 | 4.93 | -21.48 | 32.14 | 65.82 | 249.52 | 0.9080 | -506.9 | -510.8 | |
| 1.63 | 2.06 | 1.83 | 2.31 | -21.93 | 30.85 | 64.53 | 248.96 | 0.8992 | -237.8 | -8.5 | |
| 4.04 | 4.89 | 4.45 | 5.39 | -22.12 | 30.27 | 63.94 | 248.71 | 0.8951 | -449.1 | -294.2 | |
| 0.00 | 0.60 | 0.00 | 0.65 | -22.32 | 29.85 | 63.53 | 248.46 | 0.8922 | -332.0 | -284.7 | |
| 3.95 | 16.23 | 4.06 | 16.58 | -20.96 | 28.16 | 61.84 | 249.89 | 0.8787 | -448.2 | -545.0 | |
| 4.81 | -35.00 | 4.91 | -35.00 | -20.87 | 27.83 | 61.51 | 249.97 | 0.8761 | -750.9 | 999999 | |
| 0.00 | 3.69 | 0.00 | 3.86 | -21.99 | 28.52 | 62.20 | 248.75 | 0.8821 | -555.0 | -439.2 | |
| 0.00 | 1.63 | 0.00 | 1.68 | -22.04 | 28.08 | 61.75 | 248.66 | 0.8787 | -657.0 | -542.3 | |
| 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. | |