SDO HMI 2014-05-28 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.39 | 165.76 | 17.59 | 87.47 | -8.89 | 24.93 | -18.67 | 113.39 | 0.3459 | 815.4 | 385.8 | |
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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 |
| 6.59 | 146.01 | 3.46 | 76.82 | -8.72 | 25.63 | -17.97 | 113.63 | 0.3342 | 1287.3 | 405.7 | |
| 11.64 | -1.00 | 6.13 | -1.00 | -9.02 | 25.42 | -18.18 | 114.24 | 0.3393 | 1238.2 | 999999 | |
| 10.47 | -1.00 | 5.51 | -1.00 | -8.78 | 25.27 | -18.32 | 113.40 | 0.3400 | 1245.6 | 999999 | |
| 3.16 | -1.00 | 1.67 | -1.00 | -8.83 | 25.01 | -18.59 | 113.28 | 0.3444 | 877.3 | 999999 | |
| 0.90 | -1.00 | 0.48 | -1.00 | -8.83 | 24.78 | -18.81 | 113.04 | 0.3478 | 702.6 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -8.16 | 24.79 | -18.81 | 111.21 | 0.3439 | 646.0 | 517.2 | |
| 0.00 | 3.88 | 0.00 | 2.06 | -8.18 | 23.61 | -19.98 | 110.18 | 0.3620 | 783.0 | 749.9 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -8.49 | 23.40 | -20.20 | 110.79 | 0.3668 | 705.0 | 576.2 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -9.83 | 22.86 | -20.74 | 113.67 | 0.3826 | 729.0 | 560.6 | |
| 0.00 | 4.24 | 0.00 | 2.28 | -9.77 | 22.57 | -21.03 | 113.24 | 0.3866 | 831.0 | 745.7 | |
| 0.63 | 2.53 | 0.34 | 1.36 | -9.71 | 22.31 | -21.29 | 112.85 | 0.3901 | 939.9 | 749.7 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -8.70 | 20.14 | -23.46 | 108.79 | 0.4174 | -602.0 | -482.2 | |
| 0.00 | 1.62 | 0.00 | 0.89 | -9.44 | 19.99 | -23.61 | 110.35 | 0.4232 | -855.0 | -675.9 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -9.56 | 19.88 | -23.72 | 110.55 | 0.4254 | -740.0 | -544.7 | |
| 0.00 | 2.71 | 0.00 | 1.48 | -8.67 | 19.30 | -24.30 | 108.15 | 0.4298 | -856.0 | -591.6 | |
| 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. | |