SDO HMI 2011-11-15 05:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.37 | 144.91 | 50.47 | 264.37 | 19.57 | 88.05 | 74.23 | 289.56 | 0.9623 | -121.3 | -185.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.24 | 58.31 | 4.96 | 127.33 | 19.35 | 91.20 | 77.39 | 289.20 | 0.9760 | 408.0 | -147.4 | |
| 5.93 | -1.00 | 12.85 | -1.00 | 19.21 | 90.84 | 77.02 | 289.06 | 0.9746 | -489.7 | 999999 | |
| 2.32 | -1.00 | 5.00 | -1.00 | 19.71 | 90.77 | 76.96 | 289.58 | 0.9745 | -460.1 | 999999 | |
| 1.72 | 5.42 | 3.11 | 9.87 | 18.18 | 88.04 | 74.23 | 288.09 | 0.9631 | 273.9 | -93.8 | |
| 0.00 | 5.07 | 0.00 | 9.12 | 19.25 | 87.83 | 74.01 | 289.22 | 0.9624 | -492.0 | -448.1 | |
| 3.78 | 10.41 | 6.17 | 17.02 | 18.17 | 86.16 | 72.34 | 288.17 | 0.9542 | 226.0 | -54.6 | |
| 0.00 | 2.41 | 0.00 | 3.78 | 18.37 | 85.33 | 71.52 | 288.41 | 0.9501 | 442.0 | 272.6 | |
| 0.00 | 2.15 | 0.00 | 3.77 | 20.88 | 87.37 | 73.56 | 290.94 | 0.9607 | -455.0 | -373.8 | |
| 0.00 | 0.77 | 0.00 | 1.20 | 18.94 | 85.12 | 71.31 | 289.03 | 0.9492 | 111.0 | 62.1 | |
| 0.00 | 23.65 | 0.00 | 37.69 | 19.70 | 85.63 | 71.81 | 289.80 | 0.9520 | -688.0 | -187.9 | |
| 0.00 | 2.06 | 0.00 | 2.92 | 19.60 | 83.12 | 69.31 | 289.86 | 0.9386 | 346.0 | 225.8 | |
| 5.50 | 34.66 | 8.12 | 51.67 | 20.57 | 83.91 | 70.09 | 290.83 | 0.9434 | 372.5 | -364.7 | |
| 3.70 | -12.00 | 5.45 | -12.00 | 20.76 | 83.92 | 70.10 | 291.03 | 0.9435 | -353.7 | 999999 | |
| 3.18 | -12.00 | 4.81 | -12.00 | 21.18 | 84.38 | 70.56 | 291.44 | 0.9461 | -600.1 | 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. | |