| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.12 | 211.99 | 62.38 | 357.25 | 6.18 | 256.83 | 73.25 | 275.19 | 0.9562 | -298.8 | -96.5 | |
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back to the solar disc SDO HMI 2011-11-02 08:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.74 | 187.00 | 15.74 | 327.75 | 6.04 | 257.96 | 74.38 | 275.07 | 0.9627 | 601.3 | -92.9 | |
| 24.49 | -1.00 | 42.57 | -1.00 | 5.99 | 257.39 | 73.81 | 274.99 | 0.9600 | -727.6 | 999999 | |
| 0.00 | 3.29 | 0.00 | 4.99 | 6.02 | 254.86 | 71.28 | 274.90 | 0.9468 | -510.0 | -404.2 | |
| 0.00 | 1.38 | 0.00 | 2.08 | 5.71 | 254.58 | 71.00 | 274.56 | 0.9453 | -457.0 | -464.8 | |
| 0.00 | 1.99 | 0.00 | 2.82 | 7.80 | 253.46 | 69.89 | 276.74 | 0.9383 | -42.0 | -174.1 | |
| 0.00 | 2.08 | 0.00 | 2.84 | 5.72 | 252.63 | 69.05 | 274.49 | 0.9337 | -452.0 | -367.7 | |
| 0.00 | 0.95 | 0.00 | 1.29 | 6.34 | 252.38 | 68.80 | 275.14 | 0.9319 | -498.0 | -423.2 | |
| 1.04 | 1.90 | 1.19 | 2.18 | 9.98 | 248.35 | 64.78 | 279.03 | 0.9039 | -216.2 | -97.2 | |
| 0.00 | 1.38 | 0.00 | 1.44 | 8.58 | 245.32 | 61.75 | 277.45 | 0.8804 | -354.0 | -359.5 | |
| 1.38 | 1.73 | 1.43 | 1.79 | 8.89 | 245.28 | 61.70 | 277.80 | 0.8800 | -522.1 | -418.2 | |
| 0.00 | 1.47 | 0.00 | 1.47 | 8.81 | 244.19 | 60.61 | 277.71 | 0.8709 | -493.0 | -413.8 | |
| 0.00 | 1.21 | 0.00 | 1.19 | 8.24 | 243.67 | 60.09 | 277.05 | 0.8665 | 378.0 | 302.9 | |
| 0.00 | 1.56 | 0.00 | 1.51 | 8.70 | 243.01 | 59.43 | 277.59 | 0.8607 | 502.0 | 425.9 | |
| 1.47 | 2.60 | 1.45 | 2.56 | 11.14 | 243.62 | 60.04 | 280.40 | 0.8663 | 387.0 | 318.8 | |
| 0.00 | 1.12 | 0.00 | 1.10 | 11.63 | 243.49 | 59.91 | 280.98 | 0.8653 | 532.0 | 430.8 | |
| 0.00 | 0.69 | 0.00 | 0.67 | 11.01 | 243.27 | 59.69 | 280.27 | 0.8633 | 476.0 | 421.9 | |
| 0.00 | 1.64 | 0.00 | 1.57 | 11.11 | 242.53 | 58.95 | 280.41 | 0.8568 | 647.0 | 578.2 | |
| 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. | |