SDO HMI 2011-02-26 10:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.75 | 160.90 | 37.58 | 301.92 | 26.54 | 163.42 | -68.52 | 59.81 | 0.9641 | -110.2 | -209.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.72 | 4.39 | 2.39 | 6.14 | 24.72 | 168.86 | -63.08 | 60.07 | 0.9361 | -384.9 | -248.0 | |
| 0.00 | 1.72 | 0.00 | 2.85 | 26.78 | 165.64 | -66.30 | 58.96 | 0.9553 | -340.0 | -251.8 | |
| 0.00 | 1.38 | 0.00 | 2.26 | 26.57 | 165.73 | -66.22 | 59.16 | 0.9546 | -374.0 | -334.9 | |
| 3.88 | 145.75 | 7.51 | 276.91 | 27.81 | 162.92 | -69.02 | 58.69 | 0.9678 | -453.7 | -222.0 | |
| 0.00 | 0.34 | 0.00 | 0.51 | 24.07 | 167.00 | -64.95 | 61.30 | 0.9445 | -269.0 | -199.0 | |
| 1.46 | 1.98 | 2.50 | 3.38 | 26.01 | 164.68 | -67.26 | 60.01 | 0.9583 | 238.6 | 127.7 | |
| 4.91 | -4.00 | 9.41 | -4.00 | 26.85 | 162.80 | -69.14 | 59.67 | 0.9671 | -572.8 | 999999 | |
| 7.32 | -4.00 | 13.08 | -4.00 | 26.01 | 163.80 | -68.15 | 60.25 | 0.9621 | 340.6 | 999999 | |
| 1.46 | -4.00 | 2.69 | -4.00 | 26.17 | 163.32 | -68.62 | 60.21 | 0.9642 | -120.6 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.95 | 23.48 | 165.42 | -66.52 | 62.34 | 0.9512 | 377.0 | 372.6 | |
| 0.00 | 1.12 | 0.00 | 2.16 | 24.90 | 162.03 | -69.92 | 61.81 | 0.9677 | 316.0 | 316.6 | |
| 0.00 | 0.95 | 0.00 | 1.65 | 23.62 | 163.48 | -68.46 | 62.73 | 0.9602 | 164.0 | 127.8 | |
| 0.00 | 1.03 | 0.00 | 2.07 | 24.91 | 161.43 | -70.51 | 61.95 | 0.9700 | 108.0 | 72.5 | |
| 0.00 | 1.64 | 0.00 | 3.04 | 23.65 | 162.33 | -69.61 | 62.98 | 0.9650 | -14.0 | -26.2 | |
| 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. | |