SDO HMI 2014-07-04 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.24 | 0.00 | 9.64 | 5.44 | 266.97 | -1.37 | 139.92 | 0.1203 | 506.2 | 463.3 | |
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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 | 1.18 | 0.00 | 0.60 | 3.50 | 280.71 | 12.37 | 271.39 | 0.2149 | -811.0 | -608.8 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 4.28 | 279.38 | 11.04 | 275.53 | 0.1927 | -835.0 | -734.3 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 1.06 | 274.96 | 6.63 | 251.64 | 0.1222 | -777.0 | -558.2 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 8.86 | 269.86 | 1.52 | 344.91 | 0.1013 | 959.0 | 758.6 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 11.91 | 268.07 | -0.26 | 1.73 | 0.1508 | 733.0 | 577.6 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 2.55 | 267.91 | -0.42 | 149.70 | 0.0147 | 928.0 | 762.8 | |
| 0.00 | 2.54 | 0.00 | 1.26 | 2.73 | 267.79 | -0.55 | 134.80 | 0.0135 | 1070.0 | 787.0 | |
| 0.00 | 1.73 | 0.00 | 0.86 | 2.55 | 266.97 | -1.37 | 117.85 | 0.0271 | 904.0 | 677.4 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 12.25 | 266.76 | -1.57 | 9.77 | 0.1590 | 883.0 | 659.6 | |
| 0.00 | 0.82 | 0.00 | 0.41 | -0.03 | 261.34 | -6.99 | 115.15 | 0.1351 | 750.0 | 632.3 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 9.37 | 260.95 | -7.39 | 49.96 | 0.1665 | 733.0 | 570.6 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 1.59 | 260.36 | -7.98 | 101.79 | 0.1424 | 1006.0 | 853.0 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 7.10 | 259.44 | -8.90 | 66.32 | 0.1684 | 705.0 | 428.1 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 9.42 | 256.03 | -12.31 | 62.75 | 0.2377 | 839.0 | 612.1 | |
| 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. | |