SDO HMI 2011-09-04 22:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.16 | 100.83 | 22.80 | 134.61 | 23.00 | 303.58 | 69.18 | 292.02 | 0.9277 | -156.5 | -44.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.52 | 79.85 | 2.19 | 113.58 | 22.46 | 305.58 | 71.19 | 291.32 | 0.9405 | 156.5 | -109.9 | |
| 12.24 | -1.00 | 17.31 | -1.00 | 22.51 | 305.14 | 70.74 | 291.38 | 0.9380 | -570.9 | 999999 | |
| 0.00 | 1.07 | 0.00 | 1.36 | 23.87 | 302.44 | 68.04 | 292.90 | 0.9224 | -392.0 | -347.6 | |
| 0.00 | 0.89 | 0.00 | 1.04 | 24.72 | 300.10 | 65.70 | 293.95 | 0.9077 | -402.0 | -382.0 | |
| 0.00 | 1.07 | 0.00 | 1.15 | 25.39 | 297.27 | 62.87 | 294.92 | 0.8884 | 253.0 | 229.7 | |
| 0.45 | 2.23 | 0.44 | 2.22 | 25.18 | 294.67 | 60.27 | 294.94 | 0.8687 | 480.8 | 372.6 | |
| 0.00 | 1.07 | 0.00 | 1.07 | 25.61 | 294.90 | 60.50 | 295.41 | 0.8709 | 332.0 | 296.8 | |
| 0.00 | 1.96 | 0.00 | 1.93 | 25.83 | 294.13 | 59.73 | 295.75 | 0.8651 | 413.0 | 373.5 | |
| 0.00 | 0.71 | 0.00 | 0.70 | 25.65 | 293.98 | 59.58 | 295.56 | 0.8637 | 563.0 | 483.6 | |
| 0.00 | 1.70 | 0.00 | 1.65 | 25.83 | 293.74 | 59.34 | 295.81 | 0.8620 | 522.0 | 419.3 | |
| 1.43 | 3.22 | 1.40 | 3.16 | 26.53 | 294.05 | 59.65 | 296.57 | 0.8653 | 422.3 | 260.0 | |
| 0.00 | 0.45 | 0.00 | 0.42 | 25.14 | 292.86 | 58.46 | 295.12 | 0.8542 | 485.0 | 454.0 | |
| 0.00 | 2.59 | 0.00 | 2.48 | 25.79 | 293.18 | 58.78 | 295.84 | 0.8575 | 642.0 | 526.9 | |
| 1.52 | 4.02 | 1.46 | 3.85 | 26.01 | 293.29 | 58.89 | 296.08 | 0.8587 | 483.5 | 527.0 | |
| 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. | |