SDO HMI 2014-05-16 14:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.30 | 38.28 | 2.73 | 19.65 | -15.33 | 193.56 | -8.24 | 148.17 | 0.2631 | 457.0 | 336.2 | |
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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 | 0.99 | 0.00 | 0.51 | -15.15 | 194.95 | -6.85 | 152.28 | 0.2487 | 977.0 | 787.7 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -15.03 | 194.73 | -7.07 | 151.30 | 0.2486 | 953.0 | 686.8 | |
| 0.81 | 1.89 | 0.42 | 0.97 | -16.02 | 194.50 | -7.30 | 152.45 | 0.2651 | 958.1 | 738.2 | |
| 0.00 | 0.72 | 0.00 | 0.37 | -16.30 | 194.30 | -7.50 | 152.32 | 0.2708 | 858.0 | 659.9 | |
| 0.00 | 2.25 | 0.00 | 1.15 | -15.46 | 194.33 | -7.47 | 150.85 | 0.2582 | 133.0 | 259.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -15.27 | 193.93 | -7.87 | 149.17 | 0.2589 | 747.0 | 606.4 | |
| 0.00 | 3.14 | 0.00 | 1.61 | -15.02 | 193.88 | -7.92 | 148.48 | 0.2558 | 924.0 | 785.9 | |
| 0.00 | 3.41 | 0.00 | 1.75 | -15.08 | 193.59 | -8.21 | 147.70 | 0.2592 | 1119.0 | 830.1 | |
| 4.49 | 16.35 | 2.31 | 8.40 | -15.27 | 193.29 | -8.50 | 147.19 | 0.2645 | 942.4 | 387.5 | |
| 0.00 | 2.34 | 0.00 | 1.20 | -15.70 | 193.24 | -8.56 | 147.95 | 0.2710 | -120.0 | -309.5 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -15.67 | 193.05 | -8.74 | 147.32 | 0.2723 | -663.0 | -486.1 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -15.54 | 192.87 | -8.93 | 146.51 | 0.2723 | -712.0 | -624.9 | |
| 0.00 | 2.42 | 0.00 | 1.25 | -15.32 | 192.47 | -9.33 | 144.87 | 0.2731 | -1022.0 | -629.6 | |
| 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. | |