| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 96.96 | 370.71 | 72.05 | 269.02 | 19.46 | 192.15 | -44.38 | 64.53 | 0.7311 | -90.2 | -187.6 | |
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back to the solar disc SDO HMI 2011-11-25 15:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.03 | 215.72 | 0.71 | 149.42 | 18.09 | 195.04 | -41.48 | 65.24 | 0.6957 | -1145.1 | -394.2 | |
| 1.11 | -1.00 | 0.77 | -1.00 | 19.05 | 194.67 | -41.85 | 64.09 | 0.7035 | -765.2 | 999999 | |
| 6.59 | -1.00 | 4.57 | -1.00 | 18.83 | 194.70 | -41.83 | 64.38 | 0.7024 | -938.5 | 999999 | |
| 25.67 | -1.00 | 17.80 | -1.00 | 18.30 | 194.52 | -42.01 | 65.17 | 0.7024 | -1061.2 | 999999 | |
| 0.60 | -1.00 | 0.42 | -1.00 | 17.77 | 194.34 | -42.19 | 65.97 | 0.7026 | -561.3 | 999999 | |
| 2.57 | 27.04 | 1.82 | 19.20 | 19.12 | 193.54 | -42.98 | 64.45 | 0.7164 | -755.5 | -418.9 | |
| 8.64 | -6.00 | 6.13 | -6.00 | 18.74 | 193.28 | -43.25 | 65.06 | 0.7179 | -743.8 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.61 | 19.11 | 192.94 | -43.58 | 64.70 | 0.7229 | -465.0 | -381.6 | |
| 2.40 | -6.00 | 1.71 | -6.00 | 18.64 | 192.83 | -43.69 | 65.36 | 0.7225 | -453.8 | 999999 | |
| 0.00 | 7.62 | 0.00 | 5.50 | 19.35 | 192.42 | -44.10 | 64.58 | 0.7294 | -372.0 | -322.6 | |
| 2.40 | 6.59 | 1.74 | 4.79 | 19.78 | 192.19 | -44.34 | 64.10 | 0.7335 | -508.1 | -448.5 | |
| 0.00 | 1.71 | 0.00 | 1.23 | 19.01 | 192.45 | -44.07 | 65.02 | 0.7279 | -465.0 | -344.1 | |
| 2.31 | -11.00 | 1.69 | -11.00 | 20.03 | 191.96 | -44.56 | 63.86 | 0.7367 | -438.7 | 999999 | |
| 0.00 | 2.74 | 0.00 | 1.98 | 19.03 | 192.18 | -44.35 | 65.08 | 0.7309 | -223.0 | -70.4 | |
| 0.00 | 1.63 | 0.00 | 1.19 | 19.81 | 191.87 | -44.66 | 64.19 | 0.7369 | 258.0 | 194.4 | |
| 0.00 | 1.54 | 0.00 | 1.11 | 17.95 | 192.32 | -44.21 | 66.47 | 0.7258 | -434.0 | -347.3 | |
| 0.00 | 0.94 | 0.00 | 0.67 | 17.61 | 192.29 | -44.23 | 66.93 | 0.7250 | -555.0 | -438.3 | |
| 2.31 | 6.42 | 1.71 | 4.75 | 20.30 | 191.33 | -45.20 | 63.75 | 0.7443 | -433.6 | -70.0 | |
| 0.00 | 1.03 | 0.00 | 0.76 | 19.89 | 191.08 | -45.45 | 64.38 | 0.7456 | 502.0 | 472.1 | |
| 0.00 | 1.11 | 0.00 | 0.82 | 19.11 | 191.09 | -45.44 | 65.38 | 0.7429 | 543.0 | 502.6 | |
| 4.71 | 7.96 | 3.51 | 5.92 | 19.60 | 190.64 | -45.88 | 64.90 | 0.7492 | 689.4 | 642.1 | |
| 2.05 | 2.40 | 1.55 | 1.81 | 19.87 | 190.04 | -46.49 | 64.77 | 0.7563 | 547.4 | 482.8 | |
| 8.04 | 19.25 | 6.12 | 14.61 | 20.30 | 189.69 | -46.84 | 64.34 | 0.7613 | 793.2 | 474.9 | |
| 0.00 | 0.86 | 0.00 | 0.66 | 21.61 | 189.05 | -47.48 | 62.91 | 0.7719 | 544.0 | 476.5 | |
| 1.20 | 1.63 | 0.93 | 1.27 | 21.67 | 188.74 | -47.79 | 62.95 | 0.7752 | 556.1 | 494.4 | |
| 3.34 | 4.62 | 2.71 | 3.74 | 21.72 | 186.82 | -49.71 | 63.51 | 0.7939 | 706.9 | 542.1 | |
| 0.00 | 0.94 | 0.00 | 0.79 | 23.55 | 185.90 | -50.63 | 61.61 | 0.8078 | 292.0 | 289.5 | |
| 20.54 | 47.06 | 16.94 | 38.85 | 22.35 | 186.17 | -50.36 | 62.97 | 0.8018 | 784.5 | 447.7 | |
| 1.45 | 2.40 | 1.22 | 2.01 | 22.81 | 185.57 | -50.95 | 62.59 | 0.8086 | 410.4 | 356.8 | |
| 0.00 | 0.77 | 0.00 | 0.64 | 22.02 | 185.72 | -50.80 | 63.50 | 0.8051 | 345.0 | 361.8 | |
| 0.00 | 1.28 | 0.00 | 1.07 | 22.20 | 185.48 | -51.05 | 63.35 | 0.8078 | 403.0 | 344.3 | |
| 0.00 | 1.88 | 0.00 | 1.59 | 22.55 | 185.10 | -51.43 | 63.05 | 0.8123 | 373.0 | 254.9 | |
| 0.00 | 2.40 | 0.00 | 2.03 | 22.32 | 184.90 | -51.62 | 63.38 | 0.8134 | 512.0 | 358.4 | |
| 0.00 | 1.71 | 0.00 | 1.47 | 22.09 | 184.30 | -52.23 | 63.84 | 0.8183 | 441.0 | 359.3 | |
| 0.00 | 0.60 | 0.00 | 0.53 | 22.76 | 183.13 | -53.40 | 63.37 | 0.8303 | 290.0 | 230.6 | |
| 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. | |