SDO HMI 2014-07-06 00:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.44 | 0.00 | 8.82 | 4.03 | 259.31 | 4.76 | 185.68 | 0.1817 | 713.3 | 598.7 | |
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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 | 0.82 | 0.00 | 0.44 | 1.51 | 278.94 | 24.39 | 266.18 | 0.4154 | -758.0 | -617.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -4.05 | 270.22 | 15.67 | 244.71 | 0.2994 | 971.0 | 786.9 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 9.07 | 266.93 | 12.38 | 295.35 | 0.2354 | 765.0 | 658.0 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 9.32 | 266.91 | 12.36 | 296.34 | 0.2368 | 800.0 | 586.2 | |
| 0.00 | 2.27 | 0.00 | 1.15 | 10.18 | 264.04 | 9.49 | 306.24 | 0.2022 | 929.0 | 694.8 | |
| 0.00 | 1.18 | 0.00 | 0.60 | -3.35 | 263.74 | 9.19 | 233.83 | 0.1984 | 835.0 | 659.5 | |
| 0.00 | 0.91 | 0.00 | 0.46 | -3.50 | 263.65 | 9.10 | 232.93 | 0.1987 | 884.0 | 710.2 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 7.79 | 251.51 | -3.04 | 34.39 | 0.0934 | 866.0 | 651.9 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 7.78 | 251.05 | -3.50 | 38.25 | 0.0982 | 851.0 | 608.0 | |
| 0.00 | 1.91 | 0.00 | 0.95 | 4.31 | 250.91 | -3.63 | 75.69 | 0.0655 | 885.0 | 714.3 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 3.35 | 248.65 | -5.90 | 90.17 | 0.1031 | 817.0 | 610.7 | |
| 0.00 | 2.36 | 0.00 | 1.18 | 0.33 | 247.25 | -7.30 | 112.60 | 0.1383 | 715.0 | 614.5 | |
| 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. | |