SDO HMI 2014-05-17 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.28 | 297.44 | 25.18 | 158.57 | -23.99 | 191.99 | -1.52 | 176.35 | 0.3703 | 832.0 | 366.2 | |
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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 | 2.52 | 0.00 | 1.31 | -19.70 | 195.25 | 1.74 | 185.51 | 0.2995 | -790.0 | -654.0 | |
| 16.81 | 281.69 | 8.94 | 150.06 | -23.81 | 192.48 | -1.03 | 177.42 | 0.3664 | 1426.0 | 426.9 | |
| 19.05 | -2.00 | 10.16 | -2.00 | -24.13 | 192.11 | -1.40 | 176.56 | 0.3720 | 1177.4 | 999999 | |
| 10.07 | -2.00 | 5.36 | -2.00 | -23.77 | 192.08 | -1.43 | 176.42 | 0.3662 | 1408.6 | 999999 | |
| 1.35 | -2.00 | 0.72 | -2.00 | -23.90 | 191.52 | -1.99 | 175.04 | 0.3690 | 892.7 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -22.73 | 191.08 | -2.43 | 173.56 | 0.3507 | 752.0 | 611.9 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -23.97 | 190.62 | -2.89 | 172.85 | 0.3715 | 738.0 | 608.2 | |
| 0.00 | 2.61 | 0.00 | 1.39 | -23.69 | 187.40 | -6.10 | 164.98 | 0.3772 | -862.0 | -681.0 | |
| 0.00 | 2.43 | 0.00 | 1.34 | -27.71 | 185.77 | -7.74 | 164.42 | 0.4455 | -777.0 | -674.2 | |
| 0.00 | 2.34 | 0.00 | 1.29 | -27.11 | 185.58 | -7.93 | 163.62 | 0.4373 | -1124.0 | -886.1 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -27.58 | 185.23 | -8.28 | 163.30 | 0.4458 | -884.0 | -770.0 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -28.11 | 185.01 | -8.49 | 163.28 | 0.4547 | -738.0 | -612.2 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -25.54 | 185.04 | -8.47 | 161.32 | 0.4165 | -781.0 | -660.5 | |
| 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. | |