SDO HMI 2011-11-10 12:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.53 | 344.62 | 41.40 | 258.95 | -13.98 | 121.67 | 45.76 | 247.92 | 0.7519 | 436.3 | 219.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.74 | 210.09 | 3.70 | 163.39 | -14.87 | 123.55 | 47.65 | 247.57 | 0.7750 | 549.2 | 287.2 | |
| 5.60 | -1.00 | 4.38 | -1.00 | -15.58 | 123.49 | 47.59 | 246.67 | 0.7768 | 703.1 | 999999 | |
| 3.96 | -1.00 | 3.07 | -1.00 | -14.76 | 123.16 | 47.25 | 247.56 | 0.7706 | 845.5 | 999999 | |
| 20.41 | -1.00 | 15.82 | -1.00 | -15.22 | 123.11 | 47.20 | 246.97 | 0.7717 | 1037.9 | 999999 | |
| 2.33 | -1.00 | 1.79 | -1.00 | -14.84 | 122.86 | 46.96 | 247.35 | 0.7678 | 1051.2 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.67 | -6.56 | 120.75 | 44.85 | 257.47 | 0.7200 | 501.0 | 383.6 | |
| 0.00 | 0.60 | 0.00 | 0.45 | -14.00 | 121.57 | 45.66 | 247.90 | 0.7513 | 490.0 | 461.7 | |
| 17.49 | 95.18 | 12.64 | 68.89 | -11.07 | 120.56 | 44.65 | 251.33 | 0.7304 | 977.6 | 277.3 | |
| 0.00 | 1.03 | 0.00 | 0.77 | -14.29 | 121.07 | 45.17 | 247.33 | 0.7471 | 610.0 | 588.1 | |
| 0.00 | 3.01 | 0.00 | 2.12 | -9.31 | 119.45 | 43.54 | 253.30 | 0.7121 | 675.0 | 594.7 | |
| 0.00 | 0.95 | 0.00 | 0.66 | -10.26 | 118.90 | 42.99 | 251.80 | 0.7087 | 612.0 | 546.5 | |
| 0.00 | 1.03 | 0.00 | 0.73 | -11.12 | 119.01 | 43.10 | 250.68 | 0.7129 | 679.0 | 487.9 | |
| 0.00 | 0.95 | 0.00 | 0.70 | -16.19 | 120.15 | 44.25 | 244.53 | 0.7445 | 489.0 | 423.6 | |
| 0.00 | 1.64 | 0.00 | 1.18 | -14.44 | 119.35 | 43.44 | 246.42 | 0.7289 | -557.0 | -450.2 | |
| 0.00 | 1.98 | 0.00 | 1.40 | -14.14 | 118.14 | 42.24 | 246.28 | 0.7143 | -659.0 | -556.9 | |
| 0.00 | 2.41 | 0.00 | 1.70 | -14.35 | 118.15 | 42.25 | 246.00 | 0.7153 | -621.0 | -479.9 | |
| 0.00 | 0.95 | 0.00 | 0.65 | -11.79 | 117.41 | 41.50 | 249.11 | 0.6966 | 690.0 | 591.9 | |
| 0.00 | 1.29 | 0.00 | 0.91 | -14.16 | 117.86 | 41.95 | 246.12 | 0.7112 | -385.0 | -481.6 | |
| 0.00 | 1.46 | 0.00 | 1.02 | -14.02 | 117.58 | 41.67 | 246.17 | 0.7075 | -557.0 | -515.8 | |
| 0.00 | 1.21 | 0.00 | 0.84 | -14.34 | 117.12 | 41.21 | 245.53 | 0.7037 | -715.0 | -614.0 | |
| 0.00 | 0.69 | 0.00 | 0.48 | -14.53 | 117.16 | 41.26 | 245.30 | 0.7050 | -606.0 | -442.9 | |
| 0.00 | 0.95 | 0.00 | 0.66 | -14.66 | 117.15 | 41.24 | 245.12 | 0.7054 | -612.0 | -542.9 | |
| 0.00 | 2.76 | 0.00 | 1.93 | -17.42 | 116.32 | 40.42 | 241.07 | 0.7092 | -452.0 | -449.2 | |
| 0.00 | 0.78 | 0.00 | 0.54 | -19.48 | 115.35 | 39.44 | 237.87 | 0.7096 | -503.0 | -361.7 | |
| 0.00 | 0.95 | 0.00 | 0.64 | -20.79 | 112.39 | 36.48 | 234.34 | 0.6865 | -291.0 | -284.3 | |
| 0.00 | 0.69 | 0.00 | 0.45 | -17.25 | 111.19 | 35.28 | 238.18 | 0.6515 | -459.0 | -456.2 | |
| 0.00 | 0.34 | 0.00 | 0.22 | -15.25 | 109.81 | 33.90 | 240.04 | 0.6234 | -644.0 | -502.0 | |
| 0.00 | 2.84 | 0.00 | 1.79 | -14.84 | 109.66 | 33.75 | 240.53 | 0.6191 | -797.0 | -625.3 | |
| 0.00 | 1.29 | 0.00 | 0.81 | -14.68 | 109.52 | 33.61 | 240.67 | 0.6165 | -732.0 | -594.4 | |
| 0.00 | 1.46 | 0.00 | 0.93 | -16.25 | 109.62 | 33.72 | 238.49 | 0.6274 | -532.0 | -400.6 | |
| 0.00 | 1.72 | 0.00 | 1.07 | -14.47 | 108.78 | 32.88 | 240.47 | 0.6063 | -602.0 | -502.5 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -14.84 | 108.77 | 32.87 | 239.91 | 0.6085 | -608.0 | -525.7 | |
| 0.00 | 1.03 | 0.00 | 0.64 | -14.90 | 108.53 | 32.62 | 239.66 | 0.6059 | -670.0 | -465.1 | |
| 0.00 | 1.98 | 0.00 | 1.21 | -13.58 | 107.34 | 31.43 | 240.77 | 0.5831 | -663.0 | -626.3 | |
| 0.00 | 1.55 | 0.00 | 0.96 | -18.81 | 105.29 | 29.38 | 231.40 | 0.5965 | -733.0 | -591.6 | |
| 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. | |