SDO HMI 2011-08-30 08:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.41 | 74.31 | 19.37 | 65.12 | -20.38 | 259.06 | -49.10 | 120.78 | 0.8269 | 413.0 | -7.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 1.04 | -23.20 | 259.52 | -48.65 | 124.06 | 0.8350 | -574.0 | -485.2 | |
| 0.00 | 0.72 | 0.00 | 0.62 | -21.44 | 260.33 | -47.83 | 122.56 | 0.8207 | 692.0 | 561.0 | |
| 0.00 | 0.99 | 0.00 | 0.86 | -22.23 | 259.98 | -48.18 | 123.24 | 0.8270 | 358.0 | 330.5 | |
| 3.05 | 15.06 | 2.60 | 12.86 | -20.55 | 260.42 | -47.74 | 121.62 | 0.8161 | 786.6 | 630.0 | |
| 0.00 | 2.33 | 0.00 | 2.07 | -22.46 | 259.38 | -48.79 | 123.19 | 0.8329 | 578.0 | 407.6 | |
| 4.84 | -4.00 | 4.15 | -4.00 | -20.38 | 260.10 | -48.06 | 121.28 | 0.8180 | 598.5 | 999999 | |
| 14.52 | 26.44 | 12.62 | 23.02 | -20.96 | 259.71 | -48.45 | 121.72 | 0.8238 | 666.5 | 174.3 | |
| 0.00 | 0.81 | 0.00 | 0.73 | -22.38 | 258.46 | -49.71 | 122.67 | 0.8400 | 460.0 | 406.7 | |
| 0.00 | 1.34 | 0.00 | 1.18 | -19.81 | 258.72 | -49.44 | 119.99 | 0.8274 | 298.0 | 242.8 | |
| 0.00 | 19.90 | 0.00 | 17.65 | -19.41 | 258.04 | -50.13 | 119.23 | 0.8316 | -413.0 | -319.2 | |
| 0.00 | 0.90 | 0.00 | 0.82 | -20.51 | 257.09 | -51.08 | 120.02 | 0.8436 | -304.0 | -245.3 | |
| 0.00 | 1.43 | 0.00 | 1.28 | -18.16 | 257.24 | -50.92 | 117.50 | 0.8336 | -501.0 | -454.4 | |
| 0.00 | 1.97 | 0.00 | 1.84 | -19.37 | 255.84 | -52.32 | 118.23 | 0.8496 | -487.0 | -372.5 | |
| 0.00 | 1.25 | 0.00 | 1.15 | -17.73 | 255.72 | -52.44 | 116.37 | 0.8449 | -505.0 | -393.2 | |
| 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. | |