SDO HMI 2014-08-19 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.18 | 290.44 | 34.24 | 211.13 | 8.46 | 343.39 | -47.51 | 84.79 | 0.7346 | -726.2 | -302.6 | |
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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 |
| 2.97 | 281.26 | 2.13 | 203.89 | 8.34 | 344.31 | -46.60 | 84.97 | 0.7240 | -1129.6 | -332.6 | |
| 5.76 | -1.00 | 4.17 | -1.00 | 8.63 | 343.76 | -47.14 | 84.55 | 0.7303 | -1291.5 | 999999 | |
| 17.65 | -1.00 | 12.75 | -1.00 | 8.30 | 343.77 | -47.13 | 85.02 | 0.7303 | -1171.2 | 999999 | |
| 17.11 | -1.00 | 12.48 | -1.00 | 8.56 | 343.23 | -47.68 | 84.64 | 0.7366 | -945.5 | 999999 | |
| 1.53 | -1.00 | 1.12 | -1.00 | 7.70 | 343.27 | -47.64 | 85.80 | 0.7365 | -212.1 | 999999 | |
| 2.16 | -1.00 | 1.59 | -1.00 | 8.08 | 342.66 | -48.24 | 85.27 | 0.7434 | -166.8 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.60 | 8.02 | 342.35 | -48.56 | 85.33 | 0.7471 | -257.0 | -167.6 | |
| 0.00 | 0.27 | 0.00 | 0.20 | 10.56 | 341.69 | -49.22 | 81.92 | 0.7542 | 238.0 | 321.3 | |
| 0.00 | 0.99 | 0.00 | 0.75 | 8.57 | 341.27 | -49.64 | 84.56 | 0.7592 | 394.0 | 391.9 | |
| 0.00 | 2.25 | 0.00 | 1.76 | 9.99 | 339.73 | -51.18 | 82.66 | 0.7759 | 644.0 | 584.5 | |
| 0.00 | 0.72 | 0.00 | 0.57 | 10.23 | 339.03 | -51.88 | 82.34 | 0.7834 | 485.0 | 423.2 | |
| 0.00 | 0.27 | 0.00 | 0.22 | 10.43 | 338.17 | -52.74 | 82.08 | 0.7925 | 599.0 | 572.3 | |
| 0.00 | 1.08 | 0.00 | 0.87 | 10.21 | 338.12 | -52.79 | 82.35 | 0.7931 | 544.0 | 476.7 | |
| 0.00 | 1.17 | 0.00 | 0.95 | 10.89 | 337.80 | -53.11 | 81.50 | 0.7964 | 535.0 | 417.8 | |
| 0.00 | 1.62 | 0.00 | 1.32 | 10.04 | 337.95 | -52.96 | 82.56 | 0.7948 | 445.0 | 332.8 | |
| 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. | |