| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.68 | 167.21 | 18.40 | 94.06 | 17.80 | 223.61 | 23.33 | 307.24 | 0.4757 | -441.1 | -323.8 | |
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back to the solar disc SDO HMI 2011-11-28 09:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.84 | 17.24 | 226.64 | 26.36 | 303.21 | 0.5089 | 518.0 | 434.6 | |
| 0.00 | 0.43 | 0.00 | 0.24 | 15.01 | 225.84 | 25.57 | 299.92 | 0.4829 | 684.0 | 571.8 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 16.88 | 225.83 | 25.55 | 303.33 | 0.4960 | 651.0 | 574.4 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 16.48 | 225.70 | 25.42 | 302.74 | 0.4914 | 796.0 | 662.5 | |
| 10.01 | 145.74 | 5.66 | 82.11 | 17.76 | 224.28 | 24.00 | 306.42 | 0.4834 | -1003.0 | -424.6 | |
| 1.20 | -5.00 | 0.67 | -5.00 | 17.63 | 223.96 | 23.68 | 306.55 | 0.4784 | -1011.9 | 999999 | |
| 21.47 | -5.00 | 12.07 | -5.00 | 17.98 | 223.50 | 23.22 | 307.66 | 0.4757 | -1156.5 | 999999 | |
| 0.00 | 2.91 | 0.00 | 1.61 | 15.80 | 222.91 | 22.64 | 304.31 | 0.4503 | 639.0 | 288.1 | |
| 0.00 | 3.76 | 0.00 | 2.09 | 16.26 | 222.77 | 22.49 | 305.35 | 0.4522 | -86.0 | -52.8 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 16.08 | 222.71 | 22.44 | 305.07 | 0.4499 | 466.0 | 302.3 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 15.32 | 222.43 | 22.15 | 303.92 | 0.4400 | 967.0 | 817.0 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 15.59 | 222.16 | 21.88 | 304.76 | 0.4388 | 846.0 | 669.6 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 15.38 | 222.07 | 21.79 | 304.45 | 0.4359 | 737.0 | 573.3 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 17.65 | 222.21 | 21.93 | 308.56 | 0.4571 | -759.0 | -554.7 | |
| 0.00 | 2.74 | 0.00 | 1.53 | 19.92 | 221.61 | 21.33 | 313.23 | 0.4713 | -844.0 | -707.9 | |
| 0.00 | 2.39 | 0.00 | 1.32 | 18.56 | 219.79 | 19.51 | 313.33 | 0.4372 | 699.0 | 578.7 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 21.03 | 219.07 | 18.79 | 318.47 | 0.4554 | 710.0 | 618.8 | |
| 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. | |