SDO HMI 2014-06-01 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.58 | 154.02 | 37.66 | 150.04 | -4.43 | 298.39 | -59.42 | 94.73 | 0.8632 | 506.8 | 282.1 | |
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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 |
| 21.68 | 95.30 | 20.72 | 90.93 | -4.25 | 299.07 | -58.74 | 94.54 | 0.8572 | 798.5 | 375.4 | |
| 1.08 | -1.00 | 1.04 | -1.00 | -3.91 | 298.87 | -58.93 | 94.14 | 0.8589 | 580.8 | 999999 | |
| 0.99 | -1.00 | 0.96 | -1.00 | -3.87 | 298.64 | -59.17 | 94.09 | 0.8609 | 332.8 | 999999 | |
| 1.54 | 31.08 | 1.50 | 30.70 | -4.82 | 298.33 | -59.47 | 95.18 | 0.8639 | 608.2 | 290.0 | |
| 1.72 | -4.00 | 1.69 | -4.00 | -4.54 | 298.07 | -59.74 | 94.85 | 0.8661 | 639.6 | 999999 | |
| 4.61 | -4.00 | 4.56 | -4.00 | -4.75 | 297.85 | -59.95 | 95.08 | 0.8680 | 564.7 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.63 | -3.71 | 297.87 | -59.94 | 93.89 | 0.8677 | 115.0 | -38.3 | |
| 0.00 | 1.17 | 0.00 | 1.17 | -3.80 | 297.61 | -60.20 | 93.98 | 0.8699 | 290.0 | 172.3 | |
| 2.08 | 5.69 | 2.11 | 5.77 | -6.27 | 297.16 | -60.65 | 96.80 | 0.8745 | 646.0 | 516.8 | |
| 0.00 | 1.36 | 0.00 | 1.37 | -4.65 | 297.31 | -60.50 | 94.95 | 0.8727 | 355.0 | 244.1 | |
| 0.00 | 3.79 | 0.00 | 3.85 | -4.96 | 297.08 | -60.73 | 95.29 | 0.8747 | -65.0 | -7.3 | |
| 0.00 | 1.99 | 0.00 | 2.05 | -5.90 | 296.59 | -61.21 | 96.34 | 0.8791 | 465.0 | 365.5 | |
| 4.88 | 13.01 | 5.08 | 13.57 | -4.12 | 296.24 | -61.56 | 94.31 | 0.8815 | -578.7 | -434.2 | |
| 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. | |