SDO HMI 2011-11-11 10:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.38 | 296.10 | 45.07 | 200.81 | -17.71 | 101.60 | 37.78 | 239.16 | 0.6808 | -195.3 | 59.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.38 | 0.00 | 1.05 | -14.63 | 110.21 | 46.39 | 247.47 | 0.7608 | -611.0 | -467.3 | |
| 0.00 | 0.95 | 0.00 | 0.72 | -15.71 | 109.76 | 45.94 | 245.95 | 0.7599 | -553.0 | -458.9 | |
| 0.00 | 0.78 | 0.00 | 0.56 | -17.98 | 106.18 | 42.36 | 241.45 | 0.7319 | -103.0 | -115.8 | |
| 0.00 | 0.86 | 0.00 | 0.62 | -17.59 | 105.94 | 42.12 | 241.83 | 0.7276 | 658.0 | 537.0 | |
| 1.46 | 106.36 | 1.04 | 76.00 | -18.17 | 104.56 | 40.74 | 240.37 | 0.7158 | 818.2 | 391.1 | |
| 0.00 | 1.03 | 0.00 | 0.72 | -18.28 | 103.97 | 40.15 | 239.91 | 0.7100 | 683.0 | 587.3 | |
| 0.00 | 0.78 | 0.00 | 0.54 | -17.85 | 103.73 | 39.91 | 240.32 | 0.7053 | 438.0 | 415.4 | |
| 0.00 | 0.52 | 0.00 | 0.36 | -19.17 | 103.98 | 40.16 | 238.77 | 0.7148 | 409.0 | 322.7 | |
| 2.67 | 25.06 | 1.83 | 17.17 | -16.94 | 102.97 | 39.15 | 241.09 | 0.6923 | -558.4 | 85.1 | |
| 0.00 | 1.64 | 0.00 | 1.11 | -16.62 | 102.77 | 38.95 | 241.41 | 0.6884 | -168.0 | -312.5 | |
| 8.01 | -9.00 | 5.49 | -9.00 | -17.44 | 102.89 | 39.08 | 240.39 | 0.6941 | 814.2 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.95 | -17.86 | 102.92 | 39.10 | 239.86 | 0.6965 | 651.0 | 580.7 | |
| 0.00 | 0.60 | 0.00 | 0.41 | -17.92 | 102.90 | 39.08 | 239.76 | 0.6966 | 677.0 | 485.7 | |
| 0.00 | 1.89 | 0.00 | 1.31 | -18.46 | 103.00 | 39.19 | 239.12 | 0.7007 | 687.0 | 595.5 | |
| 1.89 | 2.50 | 1.28 | 1.69 | -17.12 | 102.02 | 38.20 | 240.30 | 0.6827 | 723.5 | 600.0 | |
| 9.73 | 18.52 | 6.59 | 12.56 | -17.47 | 102.02 | 38.20 | 239.84 | 0.6847 | 900.6 | 497.4 | |
| 0.00 | 3.79 | 0.00 | 2.54 | -16.88 | 101.48 | 37.67 | 240.30 | 0.6755 | 877.0 | 762.9 | |
| 0.00 | 1.21 | 0.00 | 0.81 | -17.42 | 101.38 | 37.56 | 239.52 | 0.6772 | 636.0 | 525.1 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -16.98 | 100.76 | 36.95 | 239.73 | 0.6680 | 563.0 | 452.0 | |
| 1.55 | 1.89 | 1.04 | 1.27 | -18.41 | 100.72 | 36.90 | 237.79 | 0.6757 | -637.7 | -549.5 | |
| 3.36 | 4.39 | 2.26 | 2.96 | -19.18 | 100.72 | 36.90 | 236.78 | 0.6802 | -711.5 | -562.8 | |
| 0.00 | 1.98 | 0.00 | 1.30 | -17.08 | 99.90 | 36.08 | 239.05 | 0.6587 | -556.0 | -467.7 | |
| 0.00 | 1.12 | 0.00 | 0.72 | -15.71 | 99.37 | 35.56 | 240.61 | 0.6448 | -627.0 | -566.9 | |
| 5.43 | 8.44 | 3.52 | 5.47 | -16.86 | 99.01 | 35.19 | 238.76 | 0.6473 | -595.6 | -260.6 | |
| 0.00 | 5.86 | 0.00 | 3.78 | -16.35 | 98.86 | 35.04 | 239.37 | 0.6426 | -601.0 | -495.6 | |
| 0.00 | 2.07 | 0.00 | 1.33 | -16.36 | 98.37 | 34.55 | 239.02 | 0.6371 | -833.0 | -647.2 | |
| 0.00 | 1.21 | 0.00 | 0.77 | -16.65 | 98.32 | 34.50 | 238.59 | 0.6382 | -606.0 | -641.4 | |
| 0.00 | 1.55 | 0.00 | 1.00 | -17.44 | 98.37 | 34.55 | 237.53 | 0.6437 | -167.0 | -204.4 | |
| 3.19 | 4.39 | 2.03 | 2.80 | -16.38 | 98.00 | 34.18 | 238.74 | 0.6329 | -908.0 | -752.4 | |
| 7.32 | 63.38 | 4.69 | 40.51 | -17.04 | 97.91 | 34.09 | 237.75 | 0.6360 | -932.3 | -628.6 | |
| 2.58 | 27.04 | 1.67 | 17.50 | -18.12 | 98.03 | 34.21 | 236.35 | 0.6443 | -673.0 | -257.2 | |
| 11.80 | -31.00 | 7.63 | -31.00 | -18.50 | 97.89 | 34.07 | 235.73 | 0.6452 | -775.5 | 999999 | |
| 2.07 | -30.00 | 1.32 | -30.00 | -17.16 | 97.56 | 33.74 | 237.34 | 0.6327 | -1296.7 | 999999 | |
| 7.32 | -30.00 | 4.68 | -30.00 | -17.51 | 97.60 | 33.78 | 236.88 | 0.6354 | -1025.3 | 999999 | |
| 0.00 | 1.46 | 0.00 | 0.94 | -17.88 | 97.34 | 33.52 | 236.18 | 0.6349 | -842.0 | -701.0 | |
| 0.00 | 1.38 | 0.00 | 0.88 | -18.10 | 97.31 | 33.49 | 235.85 | 0.6361 | -739.0 | -642.4 | |
| 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. | |