SDO HMI 2014-05-16 01:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.05 | 38.82 | 5.73 | 20.18 | 8.66 | 195.22 | -13.71 | 50.17 | 0.3056 | -283.5 | 150.6 | |
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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 |
| 5.21 | 7.36 | 2.67 | 3.78 | 8.12 | 198.07 | -10.86 | 45.27 | 0.2638 | -1139.0 | -815.4 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 6.67 | 198.01 | -10.92 | 49.64 | 0.2481 | -860.0 | -603.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 8.62 | 197.59 | -11.35 | 45.18 | 0.2754 | -881.0 | -677.1 | |
| 0.00 | 1.71 | 0.00 | 0.88 | 8.56 | 197.15 | -11.78 | 46.41 | 0.2800 | -1024.0 | -914.7 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 8.32 | 196.82 | -12.12 | 47.85 | 0.2814 | -846.0 | -648.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 8.32 | 196.60 | -12.34 | 48.36 | 0.2842 | -763.0 | -597.2 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 7.87 | 194.94 | -13.99 | 53.05 | 0.3010 | -662.0 | -411.5 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 8.28 | 194.84 | -14.10 | 52.20 | 0.3064 | -850.0 | -694.7 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 9.64 | 194.34 | -14.60 | 49.75 | 0.3269 | 670.0 | 553.3 | |
| 1.08 | 5.12 | 0.56 | 2.68 | 9.28 | 194.10 | -14.84 | 51.09 | 0.3261 | 1138.4 | 940.6 | |
| 1.71 | 9.07 | 0.90 | 4.76 | 9.28 | 193.72 | -15.22 | 51.78 | 0.3311 | 995.0 | 744.6 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 8.82 | 193.36 | -15.58 | 53.55 | 0.3314 | 804.0 | 662.4 | |
| 3.05 | 5.39 | 1.60 | 2.83 | 8.48 | 193.24 | -15.69 | 54.58 | 0.3297 | 1089.9 | 848.2 | |
| 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. | |