SDO HMI 2014-05-24 20:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.50 | 23.77 | 3.11 | 16.21 | -18.82 | 133.20 | 40.56 | 243.73 | 0.6883 | -68.3 | 6.7 | |
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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 | 1.08 | 0.00 | 0.76 | -18.75 | 135.29 | 42.64 | 244.77 | 0.7115 | 437.0 | 361.2 | |
| 1.08 | 2.16 | 0.76 | 1.51 | -18.56 | 135.10 | 42.46 | 244.95 | 0.7087 | 694.2 | 558.8 | |
| 0.00 | 1.17 | 0.00 | 0.82 | -18.81 | 135.09 | 42.45 | 244.60 | 0.7095 | 690.0 | 579.2 | |
| 0.00 | 2.16 | 0.00 | 1.51 | -18.98 | 134.88 | 42.24 | 244.30 | 0.7078 | 754.0 | 630.1 | |
| 3.06 | 5.95 | 2.11 | 4.09 | -18.16 | 134.12 | 41.47 | 245.10 | 0.6961 | 627.3 | 485.8 | |
| 0.00 | 1.71 | 0.00 | 1.18 | -20.02 | 133.49 | 40.84 | 242.28 | 0.6964 | -576.0 | -509.2 | |
| 0.00 | 0.54 | 0.00 | 0.37 | -20.12 | 133.22 | 40.57 | 242.02 | 0.6938 | -661.0 | -522.8 | |
| 0.00 | 1.26 | 0.00 | 0.84 | -17.90 | 132.24 | 39.59 | 244.65 | 0.6733 | -479.0 | -354.6 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -17.72 | 132.19 | 39.54 | 244.89 | 0.6720 | -559.0 | -440.8 | |
| 0.00 | 1.71 | 0.00 | 1.14 | -17.59 | 132.07 | 39.42 | 245.02 | 0.6701 | -814.0 | -627.2 | |
| 0.36 | 1.80 | 0.24 | 1.20 | -17.98 | 131.68 | 39.03 | 244.29 | 0.6671 | -835.2 | -632.4 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -19.66 | 131.86 | 39.21 | 242.00 | 0.6765 | -632.0 | -478.6 | |
| 0.00 | 1.08 | 0.00 | 0.74 | -22.21 | 131.89 | 39.25 | 238.54 | 0.6889 | -604.0 | -425.6 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -21.37 | 124.79 | 32.14 | 235.32 | 0.6046 | 596.0 | 460.4 | |
| 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. | |