SDO HMI 2014-09-26 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.83 | 19.96 | 1.87 | 13.14 | 7.36 | 206.60 | -41.37 | 86.81 | 0.6586 | 47.6 | -11.6 | |
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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 |
| 0.00 | 1.24 | 0.00 | 0.78 | 6.01 | 209.75 | -38.21 | 89.11 | 0.6175 | -621.0 | -486.7 | |
| 0.44 | 1.41 | 0.28 | 0.89 | 6.98 | 209.47 | -38.49 | 87.50 | 0.6206 | -634.2 | -501.9 | |
| 0.00 | 2.03 | 0.00 | 1.28 | 6.38 | 209.53 | -38.44 | 88.48 | 0.6203 | -860.0 | -642.0 | |
| 0.00 | 1.06 | 0.00 | 0.67 | 5.71 | 209.00 | -38.96 | 89.50 | 0.6280 | -577.0 | -483.5 | |
| 0.00 | 2.03 | 0.00 | 1.31 | 6.96 | 207.90 | -40.06 | 87.44 | 0.6417 | -632.0 | -474.7 | |
| 0.00 | 0.44 | 0.00 | 0.29 | 5.65 | 207.03 | -40.93 | 89.38 | 0.6543 | 558.0 | 563.4 | |
| 0.00 | 1.41 | 0.00 | 0.93 | 5.83 | 206.61 | -41.35 | 89.07 | 0.6597 | 587.0 | 452.2 | |
| 2.39 | 5.22 | 1.59 | 3.49 | 7.04 | 205.51 | -42.45 | 87.15 | 0.6730 | 746.0 | 571.0 | |
| 0.00 | 0.62 | 0.00 | 0.41 | 7.24 | 205.41 | -42.56 | 86.85 | 0.6743 | 520.0 | 454.4 | |
| 0.00 | 0.97 | 0.00 | 0.66 | 8.74 | 204.88 | -43.08 | 84.60 | 0.6804 | 671.0 | 505.5 | |
| 0.00 | 0.88 | 0.00 | 0.60 | 8.24 | 204.70 | -43.26 | 85.33 | 0.6829 | 546.0 | 464.1 | |
| 0.00 | 0.88 | 0.00 | 0.60 | 7.55 | 204.37 | -43.59 | 86.33 | 0.6873 | 450.0 | 420.3 | |
| 0.00 | 1.77 | 0.00 | 1.23 | 12.05 | 203.06 | -44.90 | 79.84 | 0.7037 | -356.0 | -314.9 | |
| 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. | |