SDO HMI 2014-09-26 04:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.04 | 20.24 | 3.35 | 13.37 | 6.97 | 206.88 | -41.63 | 87.35 | 0.6621 | 59.4 | 57.9 | |
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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 | 6.38 | 210.38 | -38.13 | 88.51 | 0.6160 | -700.0 | -570.3 | |
| 0.00 | 0.88 | 0.00 | 0.56 | 6.22 | 210.24 | -38.27 | 88.76 | 0.6181 | -554.0 | -517.3 | |
| 0.62 | 1.94 | 0.39 | 1.24 | 6.41 | 209.49 | -39.02 | 88.39 | 0.6282 | -714.7 | -602.7 | |
| 0.44 | 1.33 | 0.28 | 0.84 | 7.01 | 209.43 | -39.08 | 87.43 | 0.6286 | -723.8 | -589.5 | |
| 0.00 | 0.88 | 0.00 | 0.57 | 5.74 | 209.00 | -39.51 | 89.41 | 0.6354 | -625.0 | -505.9 | |
| 0.00 | 0.62 | 0.00 | 0.40 | 6.83 | 208.27 | -40.24 | 87.64 | 0.6443 | -425.0 | -467.7 | |
| 0.00 | 1.06 | 0.00 | 0.69 | 6.89 | 207.90 | -40.61 | 87.51 | 0.6491 | -540.0 | -437.4 | |
| 0.00 | 0.35 | 0.00 | 0.23 | 5.67 | 206.93 | -41.58 | 89.30 | 0.6628 | 742.0 | 690.5 | |
| 0.00 | 0.71 | 0.00 | 0.47 | 5.82 | 206.59 | -41.92 | 89.03 | 0.6671 | 607.0 | 521.5 | |
| 0.00 | 1.41 | 0.00 | 0.95 | 6.70 | 205.85 | -42.66 | 87.65 | 0.6759 | 695.0 | 581.5 | |
| 3.98 | 5.92 | 2.68 | 3.99 | 7.03 | 205.48 | -43.03 | 87.14 | 0.6804 | 722.1 | 531.2 | |
| 0.00 | 1.33 | 0.00 | 0.90 | 8.67 | 204.89 | -43.62 | 84.70 | 0.6872 | 606.0 | 418.5 | |
| 0.00 | 1.24 | 0.00 | 0.84 | 8.27 | 204.74 | -43.77 | 85.28 | 0.6893 | 504.0 | 486.1 | |
| 0.00 | 1.33 | 0.00 | 0.91 | 7.65 | 204.52 | -43.99 | 86.18 | 0.6922 | 645.0 | 532.3 | |
| 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. | |