SDO HMI 2014-09-05 12:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.68 | 226.99 | 47.48 | 222.36 | -19.57 | 107.26 | -54.12 | 117.76 | 0.8646 | 535.5 | 214.6 | |
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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 | 1.07 | 0.00 | 1.05 | -23.14 | 109.03 | -52.35 | 122.32 | 0.8635 | -428.0 | -339.7 | |
| 0.36 | 5.45 | 0.36 | 5.46 | -22.23 | 107.62 | -53.76 | 120.75 | 0.8707 | 588.5 | 377.5 | |
| 0.00 | 0.98 | 0.00 | 0.98 | -22.10 | 107.53 | -53.85 | 120.58 | 0.8710 | 599.0 | 460.5 | |
| 0.00 | 1.88 | 0.00 | 1.81 | -19.73 | 108.00 | -53.37 | 118.23 | 0.8594 | 653.0 | 539.4 | |
| 6.07 | 114.62 | 6.03 | 113.91 | -20.56 | 107.14 | -54.23 | 118.77 | 0.8687 | 544.5 | 138.5 | |
| 19.65 | 79.33 | 18.73 | 75.29 | -18.67 | 107.97 | -53.41 | 117.06 | 0.8562 | 749.1 | 399.0 | |
| 16.97 | -5.00 | 16.84 | -5.00 | -19.97 | 106.95 | -54.43 | 118.07 | 0.8684 | 608.1 | 999999 | |
| 5.63 | 17.42 | 5.52 | 17.18 | -19.08 | 106.95 | -54.42 | 117.10 | 0.8655 | 541.3 | 53.3 | |
| 0.00 | 0.80 | 0.00 | 0.84 | -21.31 | 105.48 | -55.90 | 118.92 | 0.8833 | 491.0 | 442.4 | |
| 0.00 | 0.71 | 0.00 | 0.71 | -18.16 | 106.23 | -55.15 | 115.83 | 0.8683 | 321.0 | 254.4 | |
| 0.00 | 0.80 | 0.00 | 0.84 | -18.41 | 104.56 | -56.82 | 115.49 | 0.8817 | -169.0 | -118.1 | |
| 0.00 | 0.80 | 0.00 | 0.87 | -18.23 | 103.22 | -58.16 | 114.83 | 0.8909 | -378.0 | -307.7 | |
| 0.00 | 1.52 | 0.00 | 1.65 | -17.83 | 102.94 | -58.43 | 114.31 | 0.8919 | -427.0 | -470.9 | |
| 0.00 | 0.27 | 0.00 | 0.30 | -18.26 | 102.65 | -58.72 | 114.67 | 0.8950 | -228.0 | -272.0 | |
| 0.00 | 1.34 | 0.00 | 1.47 | -17.32 | 102.54 | -58.84 | 113.63 | 0.8936 | -459.0 | -401.5 | |
| 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. | |