SDO HMI 2011-11-15 03:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.42 | 148.53 | 55.57 | 255.36 | 19.68 | 87.83 | 72.92 | 289.74 | 0.9563 | -78.4 | -150.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.41 | 60.89 | 4.94 | 123.36 | 19.38 | 91.09 | 76.18 | 289.26 | 0.9714 | 330.5 | -135.7 | |
| 5.25 | -1.00 | 10.45 | -1.00 | 19.24 | 90.63 | 75.72 | 289.13 | 0.9696 | -553.4 | 999999 | |
| 1.46 | -1.00 | 2.94 | -1.00 | 19.68 | 90.72 | 75.82 | 289.58 | 0.9700 | -468.1 | 999999 | |
| 0.00 | 1.12 | 0.00 | 1.96 | 18.46 | 88.55 | 73.65 | 288.40 | 0.9605 | -507.0 | -430.7 | |
| 2.58 | 4.90 | 4.40 | 8.38 | 18.20 | 88.14 | 73.24 | 288.15 | 0.9585 | 242.4 | 28.1 | |
| 0.00 | 6.02 | 0.00 | 10.06 | 19.19 | 87.63 | 72.72 | 289.21 | 0.9563 | -494.0 | -393.5 | |
| 0.00 | 0.69 | 0.00 | 1.08 | 18.43 | 86.50 | 71.59 | 288.47 | 0.9505 | -121.0 | -172.9 | |
| 3.96 | 10.75 | 6.11 | 16.57 | 18.17 | 86.14 | 71.23 | 288.21 | 0.9485 | 303.8 | 35.4 | |
| 2.67 | 4.39 | 3.95 | 6.50 | 18.39 | 85.29 | 70.39 | 288.50 | 0.9440 | 344.7 | 241.5 | |
| 0.00 | 2.15 | 0.00 | 3.29 | 21.20 | 85.79 | 70.89 | 291.43 | 0.9478 | 199.0 | 147.0 | |
| 0.00 | 0.77 | 0.00 | 1.15 | 20.66 | 85.11 | 70.20 | 290.92 | 0.9439 | 221.0 | 165.6 | |
| 0.00 | 1.98 | 0.00 | 2.89 | 20.83 | 84.82 | 69.91 | 291.12 | 0.9425 | 304.0 | 169.4 | |
| 7.57 | 54.87 | 10.69 | 80.12 | 20.52 | 84.04 | 69.13 | 290.85 | 0.9380 | 378.5 | -228.6 | |
| 5.68 | -13.00 | 8.04 | -13.00 | 20.84 | 84.08 | 69.18 | 291.18 | 0.9384 | -585.8 | 999999 | |
| 2.84 | -13.00 | 4.05 | -13.00 | 21.18 | 84.25 | 69.34 | 291.53 | 0.9395 | -623.0 | 999999 | |
| 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. | |