SDO HMI 2014-07-03 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.17 | 0.00 | 8.51 | 6.00 | 260.29 | -26.83 | 83.03 | 0.4518 | 555.9 | 472.1 | |
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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 | 1.45 | 0.00 | 0.74 | 1.51 | 274.05 | -13.07 | 96.72 | 0.2287 | -852.0 | -702.3 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 11.15 | 267.91 | -19.20 | 66.16 | 0.3543 | 555.0 | 630.2 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 2.83 | 267.67 | -19.44 | 90.36 | 0.3339 | 790.0 | 639.4 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 6.85 | 267.46 | -19.66 | 78.47 | 0.3423 | 705.0 | 525.0 | |
| 0.00 | 1.64 | 0.00 | 0.86 | 8.41 | 267.35 | -19.76 | 74.10 | 0.3493 | 739.0 | 524.4 | |
| 0.00 | 0.55 | 0.00 | 0.30 | 9.20 | 260.79 | -26.32 | 75.72 | 0.4535 | 520.0 | 542.8 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 7.45 | 258.28 | -28.84 | 80.25 | 0.4872 | 809.0 | 688.6 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 4.22 | 258.42 | -28.69 | 86.92 | 0.4815 | 407.0 | 379.0 | |
| 0.00 | 1.64 | 0.00 | 0.93 | 7.68 | 257.80 | -29.31 | 79.90 | 0.4948 | 759.0 | 645.5 | |
| 0.00 | 2.18 | 0.00 | 1.27 | 5.18 | 255.72 | -31.39 | 85.16 | 0.5227 | 834.0 | 676.5 | |
| 0.00 | 1.27 | 0.00 | 0.78 | 5.50 | 250.79 | -36.33 | 84.96 | 0.5942 | 712.0 | 512.6 | |
| 0.00 | 1.27 | 0.00 | 0.82 | 6.49 | 247.47 | -39.64 | 83.59 | 0.6402 | 693.0 | 538.6 | |
| 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. | |