SDO HMI 2014-07-04 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.70 | 0.00 | 10.69 | 8.29 | 263.16 | -12.92 | 104.64 | 0.2523 | 561.0 | 423.9 | |
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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 | 0.91 | 0.00 | 0.45 | 6.45 | 279.77 | 3.69 | 311.49 | 0.0857 | -862.0 | -674.5 | |
| 0.00 | 2.18 | 0.00 | 1.08 | 4.09 | 276.11 | 0.03 | 357.98 | 0.0152 | -806.0 | -696.5 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 9.30 | 269.90 | -6.18 | 45.03 | 0.1509 | 982.0 | 853.3 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 12.05 | 267.68 | -8.40 | 42.85 | 0.2111 | 795.0 | 621.1 | |
| 0.00 | 3.63 | 0.00 | 1.85 | 12.23 | 266.79 | -9.29 | 45.09 | 0.2238 | 731.0 | 495.0 | |
| 0.00 | 2.36 | 0.00 | 1.20 | 8.65 | 265.17 | -10.91 | 62.93 | 0.2111 | 861.0 | 625.4 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 9.63 | 261.78 | -14.30 | 65.06 | 0.2697 | 894.0 | 670.6 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 9.01 | 261.74 | -14.34 | 67.24 | 0.2664 | 935.0 | 707.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 9.13 | 261.58 | -14.50 | 67.04 | 0.2697 | 996.0 | 803.9 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 7.26 | 259.12 | -16.96 | 75.86 | 0.2997 | 447.0 | 361.1 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 2.60 | 252.74 | -23.35 | 90.90 | 0.3976 | 691.0 | 557.6 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 8.80 | 251.22 | -24.86 | 76.16 | 0.4296 | 769.0 | 644.4 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 7.72 | 250.99 | -25.09 | 78.73 | 0.4303 | 844.0 | 701.7 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 6.27 | 250.46 | -25.62 | 82.22 | 0.4357 | 577.0 | 511.6 | |
| 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. | |