SDO HMI 2014-10-05 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.94 | 16.32 | 1.51 | 12.08 | 10.87 | 169.59 | 48.08 | 279.09 | 0.7395 | 171.8 | 52.7 | |
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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 | 1.32 | 0.00 | 1.09 | 8.53 | 175.34 | 53.83 | 275.82 | 0.8047 | -690.0 | -608.4 | |
| 1.41 | 2.72 | 1.16 | 2.25 | 9.24 | 175.13 | 53.62 | 276.70 | 0.8024 | -667.8 | -537.3 | |
| 0.00 | 0.88 | 0.00 | 0.72 | 9.44 | 174.97 | 53.46 | 276.94 | 0.8007 | -712.0 | -632.7 | |
| 0.00 | 0.61 | 0.00 | 0.48 | 9.17 | 172.86 | 51.35 | 276.56 | 0.7783 | 478.0 | 410.3 | |
| 0.00 | 0.79 | 0.00 | 0.61 | 8.40 | 172.32 | 50.81 | 275.55 | 0.7726 | 576.0 | 515.8 | |
| 0.00 | 1.58 | 0.00 | 1.21 | 12.69 | 171.52 | 50.01 | 281.15 | 0.7641 | -165.0 | -226.4 | |
| 0.00 | 1.05 | 0.00 | 0.78 | 10.93 | 170.09 | 48.58 | 278.87 | 0.7475 | 432.0 | 347.4 | |
| 0.00 | 0.70 | 0.00 | 0.51 | 8.43 | 168.84 | 47.33 | 275.49 | 0.7330 | 510.0 | 445.5 | |
| 0.00 | 0.88 | 0.00 | 0.64 | 12.17 | 169.00 | 47.49 | 280.60 | 0.7354 | -407.0 | -408.3 | |
| 0.00 | 1.58 | 0.00 | 1.06 | 11.82 | 163.84 | 42.33 | 280.47 | 0.6726 | 603.0 | 502.3 | |
| 0.53 | 1.49 | 0.35 | 0.99 | 11.90 | 163.61 | 42.10 | 280.60 | 0.6697 | 651.7 | 492.0 | |
| 0.00 | 0.26 | 0.00 | 0.17 | 13.74 | 162.99 | 41.48 | 283.43 | 0.6639 | 585.0 | 565.3 | |
| 0.00 | 0.97 | 0.00 | 0.62 | 14.16 | 160.53 | 39.01 | 284.50 | 0.6328 | 665.0 | 559.1 | |
| 0.00 | 1.49 | 0.00 | 0.95 | 14.28 | 160.11 | 38.60 | 284.78 | 0.6276 | 512.0 | 523.6 | |
| 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. | |