SDO HMI 2014-07-02 21:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.36 | 0.00 | 11.05 | 6.76 | 267.53 | -28.38 | 81.27 | 0.4759 | 470.4 | 212.8 | |
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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 | 4.18 | 0.00 | 2.16 | 4.69 | 279.65 | -16.26 | 83.70 | 0.2820 | -905.0 | -711.9 | |
| 0.00 | 1.73 | 0.00 | 0.92 | 4.27 | 274.59 | -21.32 | 86.04 | 0.3651 | -807.0 | -684.9 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 8.13 | 268.85 | -27.06 | 78.17 | 0.4620 | 776.0 | 621.1 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 9.13 | 268.67 | -27.24 | 76.10 | 0.4675 | 692.0 | 526.7 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 10.52 | 267.53 | -28.38 | 73.73 | 0.4888 | 756.0 | 652.2 | |
| 0.00 | 1.09 | 0.00 | 0.62 | 10.75 | 266.98 | -28.94 | 73.52 | 0.4977 | 712.0 | 463.1 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 2.96 | 267.41 | -28.50 | 89.40 | 0.4785 | 739.0 | 617.9 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 3.14 | 267.34 | -28.58 | 89.02 | 0.4796 | 686.0 | 525.2 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 10.87 | 266.68 | -29.24 | 73.42 | 0.5024 | 711.0 | 640.7 | |
| 0.00 | 2.09 | 0.00 | 1.22 | 9.60 | 264.04 | -31.88 | 76.80 | 0.5369 | 740.0 | 617.1 | |
| 0.00 | 0.64 | 0.00 | 0.39 | 8.60 | 260.96 | -34.96 | 79.38 | 0.5785 | 770.0 | 695.4 | |
| 0.00 | 0.91 | 0.00 | 0.55 | 9.29 | 260.43 | -35.49 | 78.32 | 0.5872 | 737.0 | 607.2 | |
| 0.00 | 0.91 | 0.00 | 0.62 | -0.61 | 252.25 | -43.67 | 94.06 | 0.6945 | 425.0 | 393.1 | |
| 0.00 | 1.00 | 0.00 | 0.72 | 6.17 | 249.63 | -46.29 | 84.37 | 0.7244 | 554.0 | 463.4 | |
| 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. | |