SDO HMI 2010-11-16 20:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 137.64 | 670.75 | 94.30 | 460.80 | 13.72 | 172.73 | 42.76 | 287.39 | 0.6920 | -33.7 | -18.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.13 | 356.42 | 42.20 | 258.28 | 12.84 | 176.33 | 46.37 | 285.12 | 0.7333 | -988.8 | -305.3 | |
| 1.29 | -1.00 | 0.92 | -1.00 | 12.84 | 175.41 | 45.44 | 285.31 | 0.7227 | -849.9 | 999999 | |
| 3.35 | -1.00 | 2.38 | -1.00 | 12.57 | 175.26 | 45.30 | 284.97 | 0.7204 | -852.5 | 999999 | |
| 1.37 | -1.00 | 0.98 | -1.00 | 12.85 | 175.19 | 45.23 | 285.36 | 0.7202 | -828.4 | 999999 | |
| 1.80 | -1.00 | 1.28 | -1.00 | 12.70 | 174.94 | 44.98 | 285.22 | 0.7170 | -951.0 | 999999 | |
| 1.80 | -1.00 | 1.27 | -1.00 | 12.98 | 174.79 | 44.83 | 285.63 | 0.7157 | -800.0 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.97 | 12.35 | 174.61 | 44.64 | 284.80 | 0.7123 | -659.0 | -592.4 | |
| 0.00 | 0.69 | 0.00 | 0.48 | 11.11 | 173.97 | 44.01 | 283.18 | 0.7025 | -539.0 | -558.1 | |
| 0.00 | 0.69 | 0.00 | 0.48 | 12.91 | 174.17 | 44.21 | 285.67 | 0.7083 | -613.0 | -574.6 | |
| 0.00 | 1.72 | 0.00 | 1.20 | 12.73 | 174.01 | 44.05 | 285.46 | 0.7060 | -517.0 | -518.9 | |
| 0.00 | 1.29 | 0.00 | 0.89 | 12.05 | 173.61 | 43.65 | 284.59 | 0.6998 | -684.0 | -541.9 | |
| 0.52 | 1.97 | 0.35 | 1.36 | 12.60 | 173.31 | 43.34 | 285.44 | 0.6973 | -726.3 | -683.2 | |
| 10.22 | 17.34 | 6.94 | 11.78 | 13.21 | 172.31 | 42.35 | 286.54 | 0.6865 | 567.2 | 25.9 | |
| 0.94 | 1.97 | 0.63 | 1.32 | 13.21 | 171.37 | 41.40 | 286.79 | 0.6749 | 530.7 | 558.8 | |
| 0.00 | 1.63 | 0.00 | 1.10 | 15.34 | 171.23 | 41.27 | 289.92 | 0.6790 | 615.0 | 434.6 | |
| 0.00 | 0.86 | 0.00 | 0.58 | 15.79 | 171.22 | 41.26 | 290.58 | 0.6802 | 606.0 | 494.5 | |
| 0.00 | 0.94 | 0.00 | 0.62 | 13.47 | 170.49 | 40.53 | 287.43 | 0.6647 | -243.0 | -343.1 | |
| 2.49 | 4.55 | 1.65 | 3.01 | 13.75 | 170.47 | 40.51 | 287.84 | 0.6651 | -681.2 | -213.2 | |
| 0.00 | 1.97 | 0.00 | 1.30 | 13.33 | 170.30 | 40.34 | 287.27 | 0.6619 | -462.0 | -368.0 | |
| 0.00 | 1.12 | 0.00 | 0.73 | 14.28 | 169.90 | 39.94 | 288.81 | 0.6595 | 408.0 | 286.0 | |
| 3.18 | 4.38 | 2.08 | 2.86 | 14.11 | 169.58 | 39.62 | 288.65 | 0.6551 | 599.1 | 298.5 | |
| 0.00 | 1.12 | 0.00 | 0.73 | 14.66 | 169.38 | 39.42 | 289.54 | 0.6542 | 508.0 | 390.9 | |
| 0.00 | 1.29 | 0.00 | 0.84 | 14.30 | 169.19 | 39.22 | 289.07 | 0.6507 | 735.0 | 651.9 | |
| 0.00 | 1.20 | 0.00 | 0.79 | 14.90 | 169.32 | 39.35 | 289.93 | 0.6541 | 545.0 | 450.3 | |
| 0.00 | 1.20 | 0.00 | 0.77 | 13.53 | 168.56 | 38.60 | 288.11 | 0.6405 | 627.0 | 521.6 | |
| 1.12 | 258.62 | 0.72 | 165.36 | 14.68 | 168.71 | 38.75 | 289.80 | 0.6459 | 660.3 | 423.9 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 14.35 | 168.49 | 38.53 | 289.39 | 0.6420 | 563.0 | 477.3 | |
| 0.43 | -26.00 | 0.28 | -26.00 | 14.81 | 168.46 | 38.50 | 290.09 | 0.6432 | 768.4 | 999999 | |
| 2.23 | -26.00 | 1.44 | -26.00 | 14.99 | 168.46 | 38.50 | 290.36 | 0.6438 | 669.0 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.88 | 13.90 | 168.24 | 38.28 | 288.79 | 0.6375 | 611.0 | 442.9 | |
| 1.72 | -26.00 | 1.11 | -26.00 | 14.84 | 168.35 | 38.39 | 290.18 | 0.6419 | 700.4 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.82 | 13.49 | 167.93 | 37.97 | 288.26 | 0.6322 | -704.0 | -507.4 | |
| 0.00 | 3.61 | 0.00 | 2.29 | 13.92 | 167.51 | 37.55 | 289.08 | 0.6282 | 499.0 | 480.7 | |
| 46.02 | -26.00 | 29.41 | -26.00 | 15.19 | 167.65 | 37.69 | 290.99 | 0.6342 | 1174.2 | 999999 | |
| 1.03 | -26.00 | 0.66 | -26.00 | 15.69 | 167.33 | 37.36 | 291.88 | 0.6319 | 964.1 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.86 | 14.14 | 166.02 | 36.06 | 289.99 | 0.6096 | 625.0 | 531.7 | |
| 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. | |