SDO HMI 2014-08-17 11:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 92.61 | 470.12 | 85.18 | 436.80 | -17.66 | 105.94 | 52.98 | 244.04 | 0.8467 | -42.1 | -18.6 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.44 | 242.18 | 41.63 | 243.13 | -17.00 | 109.20 | 56.25 | 246.08 | 0.8718 | 784.6 | 182.6 | |
| 0.90 | 2.16 | 0.84 | 2.02 | -17.35 | 106.26 | 53.30 | 244.61 | 0.8491 | 362.3 | 363.9 | |
| 0.36 | 1.26 | 0.33 | 1.17 | -17.53 | 106.01 | 53.05 | 244.33 | 0.8476 | 369.2 | 353.1 | |
| 0.00 | 1.62 | 0.00 | 1.50 | -17.67 | 105.80 | 52.85 | 244.09 | 0.8464 | 570.0 | 417.3 | |
| 0.00 | 1.26 | 0.00 | 1.14 | -17.98 | 104.57 | 51.61 | 243.25 | 0.8370 | -417.0 | -313.1 | |
| 0.00 | 1.08 | 0.00 | 0.98 | -19.25 | 104.39 | 51.43 | 241.76 | 0.8400 | -506.0 | -379.2 | |
| 2.61 | 6.94 | 2.38 | 6.31 | -19.74 | 104.24 | 51.28 | 241.16 | 0.8405 | -613.3 | -426.7 | |
| 0.00 | 1.89 | 0.00 | 1.72 | -20.06 | 104.13 | 51.17 | 240.75 | 0.8408 | -454.0 | -299.9 | |
| 0.00 | 0.63 | 0.00 | 0.55 | -19.66 | 102.67 | 49.72 | 240.56 | 0.8271 | -353.0 | -227.9 | |
| 0.27 | 211.10 | 0.23 | 178.28 | -18.75 | 102.25 | 49.30 | 241.38 | 0.8199 | -246.7 | -301.1 | |
| 3.06 | -10.00 | 2.60 | -10.00 | -17.99 | 101.91 | 48.95 | 242.09 | 0.8139 | -355.4 | 999999 | |
| 24.51 | -10.00 | 20.82 | -10.00 | -18.70 | 101.69 | 48.73 | 241.19 | 0.8148 | -750.7 | 999999 | |
| 19.46 | -10.00 | 16.35 | -10.00 | -18.20 | 101.36 | 48.40 | 241.59 | 0.8098 | -1092.3 | 999999 | |
| 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. | |