SDO HMI 2014-08-02 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.17 | 0.00 | 12.19 | 10.01 | 255.42 | 4.69 | 207.35 | 0.1769 | 871.4 | 682.1 | |
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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 |
| 0.00 | 1.81 | 0.00 | 0.92 | 0.58 | 260.99 | 10.26 | 243.07 | 0.2006 | 809.0 | 624.4 | |
| 0.00 | 1.81 | 0.00 | 0.91 | 9.31 | 260.04 | 9.31 | 291.03 | 0.1718 | 884.0 | 642.3 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 5.54 | 259.89 | 9.16 | 268.40 | 0.1593 | 840.0 | 646.4 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 11.12 | 259.75 | 9.02 | 301.08 | 0.1804 | 764.0 | 573.8 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 8.92 | 259.50 | 8.77 | 289.89 | 0.1609 | 861.0 | 673.4 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 9.85 | 258.90 | 8.17 | 296.71 | 0.1575 | 949.0 | 710.8 | |
| 0.00 | 3.71 | 0.00 | 1.85 | 3.36 | 257.13 | 6.40 | 248.80 | 0.1198 | 928.0 | 774.4 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 17.46 | 257.41 | 6.68 | 331.17 | 0.2312 | 950.0 | 662.3 | |
| 0.00 | 2.35 | 0.00 | 1.17 | 4.09 | 256.70 | 5.97 | 253.69 | 0.1086 | 778.0 | 610.8 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 4.23 | 255.88 | 5.15 | 252.48 | 0.0942 | 852.0 | 598.5 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 4.07 | 255.84 | 5.11 | 250.85 | 0.0946 | 1033.0 | 872.7 | |
| 0.00 | 2.72 | 0.00 | 1.39 | 20.13 | 249.02 | -1.71 | 6.49 | 0.2491 | 829.0 | 657.1 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 15.18 | 248.24 | -2.49 | 14.52 | 0.1681 | 885.0 | 782.6 | |
| 0.00 | 1.99 | 0.00 | 1.04 | 23.23 | 243.97 | -6.76 | 19.88 | 0.3194 | 838.0 | 634.7 | |
| 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. | |