SDO HMI 2014-09-26 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.62 | 22.26 | 2.44 | 14.98 | 6.80 | 206.84 | -42.77 | 87.51 | 0.6769 | 102.2 | 95.1 | |
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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 | 1.06 | 0.00 | 0.68 | 6.31 | 210.41 | -39.20 | 88.55 | 0.6307 | -746.0 | -615.4 | |
| 0.00 | 0.80 | 0.00 | 0.51 | 5.92 | 210.13 | -39.48 | 89.13 | 0.6348 | -467.0 | -429.7 | |
| 0.00 | 1.68 | 0.00 | 1.08 | 7.02 | 209.43 | -40.18 | 87.35 | 0.6433 | -821.0 | -553.8 | |
| 1.06 | 2.39 | 0.68 | 1.54 | 6.44 | 209.41 | -40.20 | 88.25 | 0.6440 | -704.7 | -562.7 | |
| 0.00 | 1.41 | 0.00 | 0.92 | 5.77 | 208.95 | -40.66 | 89.24 | 0.6506 | -710.0 | -570.6 | |
| 0.00 | 0.53 | 0.00 | 0.35 | 6.51 | 208.76 | -40.84 | 88.08 | 0.6524 | -473.0 | -403.5 | |
| 0.00 | 0.97 | 0.00 | 0.64 | 6.89 | 208.24 | -41.37 | 87.46 | 0.6590 | -571.0 | -422.7 | |
| 0.00 | 0.97 | 0.00 | 0.66 | 6.52 | 206.52 | -43.09 | 87.90 | 0.6815 | 757.0 | 594.3 | |
| 0.00 | 1.59 | 0.00 | 1.09 | 6.67 | 205.83 | -43.78 | 87.62 | 0.6901 | 724.0 | 652.7 | |
| 0.53 | 5.74 | 0.36 | 3.94 | 7.10 | 205.57 | -44.04 | 86.97 | 0.6931 | 869.8 | 609.1 | |
| 2.03 | -10.00 | 1.40 | -10.00 | 7.00 | 205.41 | -44.19 | 87.11 | 0.6951 | 659.3 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.67 | 7.38 | 205.32 | -44.28 | 86.55 | 0.6960 | 388.0 | 336.1 | |
| 0.00 | 0.53 | 0.00 | 0.37 | 8.70 | 204.84 | -44.76 | 84.63 | 0.7015 | 662.0 | 569.0 | |
| 0.00 | 0.88 | 0.00 | 0.61 | 8.30 | 204.73 | -44.88 | 85.21 | 0.7030 | 516.0 | 416.1 | |
| 0.00 | 1.15 | 0.00 | 0.80 | 8.14 | 204.62 | -44.98 | 85.43 | 0.7043 | 434.0 | 390.3 | |
| 0.00 | 1.59 | 0.00 | 1.12 | 5.39 | 204.22 | -45.39 | 89.30 | 0.7112 | 360.0 | 368.6 | |
| 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. | |