SDO HMI 2014-07-05 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.71 | 0.00 | 7.45 | 6.40 | 263.84 | -1.20 | 223.94 | 0.1927 | 471.8 | 445.0 | |
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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 | 1.45 | 0.00 | 0.75 | 2.82 | 280.92 | 15.89 | 268.63 | 0.2747 | -794.0 | -660.4 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 4.42 | 279.49 | 14.46 | 274.86 | 0.2510 | -645.0 | -471.8 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 3.76 | 276.82 | 11.78 | 272.53 | 0.2048 | -810.0 | -556.4 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 8.93 | 269.43 | 4.39 | 322.33 | 0.1243 | 800.0 | 576.7 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 11.82 | 268.13 | 3.09 | 340.35 | 0.1578 | 1062.0 | 864.9 | |
| 0.00 | 2.54 | 0.00 | 1.27 | 9.80 | 266.74 | 1.71 | 345.41 | 0.1172 | 931.0 | 751.6 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 10.11 | 266.59 | 1.56 | 347.26 | 0.1218 | 804.0 | 646.9 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 1.46 | 260.09 | -4.95 | 110.45 | 0.0924 | 968.0 | 842.0 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 8.57 | 251.70 | -13.33 | 67.81 | 0.2474 | 800.0 | 637.9 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 3.52 | 250.81 | -14.22 | 88.77 | 0.2463 | 912.0 | 701.4 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 3.95 | 249.23 | -15.81 | 87.20 | 0.2733 | 770.0 | 639.0 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 3.58 | 248.85 | -16.18 | 88.57 | 0.2795 | 863.0 | 689.9 | |
| 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. | |