SDO HMI 2014-01-13 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.49 | 57.28 | 36.14 | 100.44 | 8.36 | 103.44 | 72.55 | 280.12 | 0.9567 | 233.1 | 63.2 | |
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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 | 0.68 | 0.00 | 2.07 | 6.52 | 110.96 | 80.06 | 277.34 | 0.9875 | -196.0 | -162.9 | |
| 0.00 | 0.85 | 0.00 | 2.53 | 6.41 | 110.71 | 79.82 | 277.26 | 0.9868 | -274.0 | -264.0 | |
| 2.55 | 6.46 | 7.70 | 19.72 | 6.90 | 110.87 | 79.98 | 277.74 | 0.9873 | 200.3 | 71.3 | |
| 0.00 | 0.85 | 0.00 | 2.60 | 7.23 | 110.94 | 80.05 | 278.07 | 0.9876 | -81.0 | -74.2 | |
| 1.95 | 2.89 | 3.97 | 5.87 | 6.61 | 106.17 | 75.27 | 277.93 | 0.9711 | -220.1 | -173.8 | |
| 0.00 | 1.02 | 0.00 | 2.10 | 7.00 | 106.23 | 75.34 | 278.33 | 0.9716 | -237.0 | -205.8 | |
| 0.00 | 0.68 | 0.00 | 1.38 | 6.84 | 106.03 | 75.14 | 278.18 | 0.9707 | -318.0 | -297.0 | |
| 0.00 | 0.85 | 0.00 | 1.53 | 6.52 | 104.23 | 73.34 | 278.06 | 0.9626 | -273.0 | -212.9 | |
| 0.00 | 2.46 | 0.00 | 3.62 | 7.86 | 100.30 | 69.41 | 279.95 | 0.9430 | 168.0 | 174.2 | |
| 2.80 | 35.44 | 4.21 | 51.99 | 9.47 | 100.54 | 69.65 | 281.61 | 0.9456 | 73.3 | 145.5 | |
| 2.04 | -10.00 | 3.00 | -10.00 | 9.27 | 100.19 | 69.30 | 281.45 | 0.9435 | 372.2 | 999999 | |
| 7.99 | -10.00 | 11.52 | -10.00 | 9.38 | 99.65 | 68.75 | 281.65 | 0.9404 | 592.4 | 999999 | |
| 4.16 | 5.10 | 5.74 | 7.03 | 9.31 | 98.72 | 67.83 | 281.72 | 0.9349 | 408.8 | 331.6 | |
| 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. | |