| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.56 | 105.71 | 41.91 | 98.06 | -9.27 | 194.29 | 55.49 | 254.16 | 0.8469 | 89.4 | 79.8 | |
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back to the solar disc SDO HMI 2014-09-07 05:00:36 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.61 | 42.68 | 11.52 | 41.93 | -9.50 | 196.69 | 57.89 | 254.61 | 0.8685 | 321.6 | 329.3 | |
| 11.34 | -1.00 | 11.12 | -1.00 | -9.30 | 196.29 | 57.49 | 254.72 | 0.8647 | 740.3 | 999999 | |
| 2.68 | -1.00 | 2.60 | -1.00 | -9.21 | 196.04 | 57.24 | 254.76 | 0.8624 | 782.5 | 999999 | |
| 0.00 | 1.61 | 0.00 | 1.55 | -8.97 | 195.81 | 57.01 | 254.97 | 0.8599 | 511.0 | 496.6 | |
| 0.71 | 2.50 | 0.68 | 2.39 | -9.20 | 195.36 | 56.56 | 254.58 | 0.8565 | 662.6 | 580.7 | |
| 0.00 | 1.34 | 0.00 | 1.27 | -8.81 | 195.27 | 56.47 | 254.99 | 0.8549 | 397.0 | 411.0 | |
| 0.00 | 0.98 | 0.00 | 0.93 | -9.37 | 195.18 | 56.38 | 254.33 | 0.8554 | 168.0 | 207.3 | |
| 0.36 | 1.25 | 0.34 | 1.18 | -8.93 | 194.90 | 56.11 | 254.75 | 0.8520 | 499.2 | 424.4 | |
| 0.00 | 2.59 | 0.00 | 2.41 | -8.92 | 194.52 | 55.72 | 254.65 | 0.8486 | 285.0 | 232.1 | |
| 0.00 | 1.16 | 0.00 | 1.05 | -8.05 | 193.68 | 54.88 | 255.41 | 0.8390 | -529.0 | -434.1 | |
| 0.00 | 1.16 | 0.00 | 1.07 | -9.70 | 193.89 | 55.09 | 253.57 | 0.8448 | 595.0 | 540.5 | |
| 0.00 | 0.98 | 0.00 | 0.88 | -8.74 | 193.13 | 54.33 | 254.45 | 0.8356 | -109.0 | -163.5 | |
| 0.00 | 0.89 | 0.00 | 0.80 | -9.22 | 192.92 | 54.12 | 253.83 | 0.8349 | -306.0 | -180.2 | |
| 0.00 | 0.71 | 0.00 | 0.64 | -9.87 | 192.86 | 54.06 | 253.06 | 0.8360 | 346.0 | 370.1 | |
| 0.00 | 1.61 | 0.00 | 1.39 | -8.39 | 191.92 | 53.12 | 254.48 | 0.8234 | -566.0 | -505.4 | |
| 17.86 | 40.98 | 15.65 | 35.99 | -9.35 | 192.07 | 53.27 | 253.41 | 0.8273 | -663.5 | -61.8 | |
| 0.00 | 5.27 | 0.00 | 4.58 | -8.70 | 191.88 | 53.08 | 254.10 | 0.8238 | -681.0 | -548.8 | |
| 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. | |