SDO HMI 2014-03-02 09:01:13 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.47 | 26.24 | 0.80 | 14.30 | 7.65 | 134.14 | 19.68 | 307.09 | 0.4195 | 345.8 | 364.2 | |
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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 | 1.12 | 0.00 | 0.64 | 7.89 | 140.33 | 25.88 | 299.86 | 0.5005 | -732.0 | -560.1 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 4.39 | 139.45 | 24.99 | 294.23 | 0.4639 | -842.0 | -671.3 | |
| 0.00 | 1.73 | 0.00 | 0.95 | 7.14 | 136.54 | 22.09 | 302.63 | 0.4449 | 778.0 | 605.8 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 7.44 | 136.37 | 21.91 | 303.41 | 0.4451 | 834.0 | 753.6 | |
| 0.00 | 2.68 | 0.00 | 1.48 | 8.51 | 135.72 | 21.26 | 306.23 | 0.4465 | -927.0 | -606.5 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 8.44 | 135.39 | 20.93 | 306.53 | 0.4417 | -944.0 | -782.8 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 6.83 | 134.60 | 20.15 | 304.53 | 0.4169 | 844.0 | 659.7 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 7.03 | 134.26 | 19.80 | 305.40 | 0.4143 | 846.0 | 676.7 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 8.04 | 133.99 | 19.53 | 307.72 | 0.4203 | 742.0 | 591.8 | |
| 0.95 | 6.22 | 0.52 | 3.38 | 8.10 | 133.42 | 18.97 | 308.68 | 0.4140 | 920.5 | 715.3 | |
| 0.52 | 1.55 | 0.28 | 0.84 | 8.19 | 133.14 | 18.68 | 309.26 | 0.4113 | 954.3 | 900.5 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 8.03 | 130.77 | 16.32 | 312.87 | 0.3812 | 759.0 | 600.5 | |
| 0.00 | 2.33 | 0.00 | 1.25 | 8.19 | 130.69 | 16.23 | 313.31 | 0.3818 | 981.0 | 697.0 | |
| 0.00 | 2.94 | 0.00 | 1.56 | 7.29 | 130.49 | 16.04 | 311.89 | 0.3697 | 733.0 | 711.7 | |
| 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. | |