| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 138.75 | 510.79 | 88.94 | 324.20 | 19.50 | 192.26 | -34.93 | 59.81 | 0.6253 | -149.0 | -176.4 | |
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back to the solar disc SDO HMI 2011-11-26 08:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.77 | 0.00 | 0.47 | 19.47 | 195.50 | -31.68 | 57.79 | 0.5875 | -661.0 | -426.8 | |
| 1.54 | 222.39 | 0.94 | 136.24 | 18.77 | 194.95 | -32.24 | 59.24 | 0.5900 | -947.8 | -485.2 | |
| 21.31 | -2.00 | 13.10 | -2.00 | 18.83 | 194.60 | -32.58 | 59.38 | 0.5945 | -1059.9 | 999999 | |
| 19.60 | -2.00 | 12.03 | -2.00 | 18.33 | 194.49 | -32.70 | 60.22 | 0.5930 | -1106.8 | 999999 | |
| 1.20 | -2.00 | 0.73 | -2.00 | 17.81 | 194.45 | -32.73 | 61.07 | 0.5905 | -816.5 | 999999 | |
| 9.24 | 144.84 | 5.74 | 90.67 | 18.79 | 193.68 | -33.51 | 60.05 | 0.6054 | -1011.9 | -274.4 | |
| 2.57 | -6.00 | 1.61 | -6.00 | 19.69 | 193.35 | -33.83 | 58.90 | 0.6144 | -693.3 | 999999 | |
| 25.34 | -6.00 | 15.81 | -6.00 | 19.19 | 193.43 | -33.75 | 59.60 | 0.6106 | -839.7 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.86 | 20.03 | 193.08 | -34.10 | 58.58 | 0.6196 | -13.0 | 9.1 | |
| 1.03 | -6.00 | 0.64 | -6.00 | 18.63 | 193.37 | -33.81 | 60.48 | 0.6082 | -824.6 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.76 | 19.84 | 192.90 | -34.28 | 58.97 | 0.6206 | -535.0 | -384.0 | |
| 1.54 | -6.00 | 0.97 | -6.00 | 19.21 | 192.86 | -34.32 | 59.92 | 0.6176 | -442.8 | 999999 | |
| 1.54 | -6.00 | 0.97 | -6.00 | 18.90 | 192.93 | -34.25 | 60.34 | 0.6150 | -495.1 | 999999 | |
| 1.97 | -6.00 | 1.24 | -6.00 | 19.86 | 192.66 | -34.52 | 59.08 | 0.6236 | -463.9 | 999999 | |
| 1.20 | -6.00 | 0.76 | -6.00 | 19.15 | 192.57 | -34.61 | 60.20 | 0.6207 | -451.3 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.27 | 18.12 | 192.77 | -34.41 | 61.61 | 0.6128 | -503.0 | -426.0 | |
| 0.00 | 1.28 | 0.00 | 0.82 | 19.41 | 191.66 | -35.52 | 60.34 | 0.6329 | 789.0 | 649.6 | |
| 0.00 | 1.20 | 0.00 | 0.77 | 19.47 | 191.22 | -35.96 | 60.51 | 0.6384 | 556.0 | 509.6 | |
| 0.00 | 1.46 | 0.00 | 0.94 | 19.80 | 190.51 | -36.68 | 60.44 | 0.6484 | 830.0 | 671.4 | |
| 11.56 | 72.42 | 7.58 | 47.77 | 19.98 | 189.83 | -37.36 | 60.56 | 0.6572 | 949.7 | 464.3 | |
| 17.63 | -20.00 | 11.66 | -20.00 | 20.44 | 189.33 | -37.85 | 60.17 | 0.6651 | 930.6 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.35 | 23.08 | 188.17 | -39.01 | 57.21 | 0.6913 | 661.0 | 600.5 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 19.56 | 189.19 | -38.00 | 61.48 | 0.6625 | 549.0 | 398.9 | |
| 0.00 | 0.77 | 0.00 | 0.53 | 22.73 | 188.08 | -39.10 | 57.72 | 0.6904 | 545.0 | 533.2 | |
| 0.00 | 1.11 | 0.00 | 0.74 | 20.46 | 188.64 | -38.54 | 60.51 | 0.6730 | 388.0 | 333.5 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 15.21 | 189.19 | -37.99 | 67.81 | 0.6438 | -471.0 | -487.6 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 15.18 | 188.88 | -38.30 | 67.99 | 0.6475 | -671.0 | -621.1 | |
| 1.88 | 9.33 | 1.32 | 6.53 | 22.41 | 186.18 | -41.01 | 59.12 | 0.7091 | 883.4 | 798.2 | |
| 2.57 | 36.38 | 1.81 | 25.73 | 22.73 | 185.98 | -41.21 | 58.80 | 0.7127 | 715.3 | 536.8 | |
| 2.48 | -28.00 | 1.74 | -28.00 | 22.06 | 185.92 | -41.26 | 59.70 | 0.7102 | 774.0 | 999999 | |
| 11.98 | -29.00 | 8.46 | -29.00 | 22.47 | 185.64 | -41.54 | 59.30 | 0.7150 | 822.7 | 999999 | |
| 0.00 | 2.65 | 0.00 | 1.90 | 22.97 | 185.11 | -42.07 | 58.90 | 0.7228 | 551.0 | 501.3 | |
| 2.57 | -29.00 | 1.83 | -29.00 | 22.65 | 185.14 | -42.04 | 59.30 | 0.7211 | 600.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.74 | 23.38 | 184.77 | -42.41 | 58.53 | 0.7281 | 484.0 | 410.2 | |
| 0.00 | 3.00 | 0.00 | 2.13 | 22.33 | 185.09 | -42.09 | 59.74 | 0.7202 | 617.0 | 504.0 | |
| 0.00 | 0.51 | 0.00 | 0.37 | 22.93 | 184.73 | -42.45 | 59.13 | 0.7266 | 418.0 | 310.7 | |
| 0.00 | 1.28 | 0.00 | 0.92 | 22.17 | 184.85 | -42.33 | 60.06 | 0.7221 | 500.0 | 419.7 | |
| 0.00 | 1.46 | 0.00 | 1.05 | 22.64 | 184.63 | -42.56 | 59.55 | 0.7264 | 605.0 | 461.8 | |
| 0.00 | 1.03 | 0.00 | 0.74 | 22.42 | 184.67 | -42.52 | 59.82 | 0.7250 | 453.0 | 452.6 | |
| 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. | |