SDO HMI 2014-05-28 08:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.19 | 29.94 | 7.34 | 18.96 | -10.70 | 83.61 | 37.27 | 253.68 | 0.6215 | 152.9 | 105.8 | |
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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 |
| 11.19 | 16.16 | 7.34 | 10.59 | -9.77 | 86.55 | 40.21 | 256.32 | 0.6570 | 865.3 | 557.8 | |
| 0.00 | 1.26 | 0.00 | 0.81 | -8.30 | 85.32 | 38.97 | 258.26 | 0.6379 | 416.0 | 413.6 | |
| 0.00 | 1.26 | 0.00 | 0.80 | -11.96 | 83.50 | 37.16 | 252.01 | 0.6236 | 633.0 | 489.8 | |
| 0.00 | 3.07 | 0.00 | 1.90 | -12.22 | 81.92 | 35.58 | 250.97 | 0.6037 | 648.0 | 569.4 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -10.17 | 80.73 | 34.39 | 253.89 | 0.5808 | -407.0 | -438.3 | |
| 0.00 | 1.17 | 0.00 | 0.71 | -10.41 | 80.72 | 34.38 | 253.47 | 0.5815 | -674.0 | -510.6 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -10.32 | 80.56 | 34.22 | 253.56 | 0.5790 | -683.0 | -616.2 | |
| 0.00 | 1.62 | 0.00 | 0.99 | -12.33 | 80.27 | 33.93 | 250.07 | 0.5821 | -131.0 | -244.2 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -9.77 | 77.20 | 30.85 | 253.15 | 0.5301 | -744.0 | -598.4 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -11.10 | 76.30 | 29.96 | 250.26 | 0.5226 | -484.0 | -502.6 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -14.13 | 74.07 | 27.73 | 243.27 | 0.5072 | -642.0 | -587.2 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -13.78 | 73.95 | 27.61 | 243.81 | 0.5036 | -707.0 | -622.0 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -17.05 | 73.35 | 27.01 | 237.50 | 0.5168 | -619.0 | -529.1 | |
| 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. | |