SDO HMI 2014-07-13 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.44 | 129.90 | 80.19 | 373.88 | -6.48 | 237.12 | 79.61 | 262.68 | 0.9858 | -137.0 | -34.6 | |
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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 | 5.72 | 0.00 | 24.17 | -4.82 | 240.24 | 82.72 | 264.63 | 0.9933 | 135.0 | 161.5 | |
| 0.00 | 7.09 | 0.00 | 21.60 | -4.70 | 237.81 | 80.30 | 264.54 | 0.9876 | -244.0 | -102.3 | |
| 6.54 | 95.74 | 19.02 | 279.81 | -5.71 | 237.25 | 79.74 | 263.47 | 0.9863 | 326.2 | -54.0 | |
| 0.00 | 2.36 | 0.00 | 7.99 | -7.62 | 238.39 | 80.88 | 261.65 | 0.9898 | 210.0 | 288.2 | |
| 8.27 | -3.00 | 24.85 | -3.00 | -6.62 | 237.45 | 79.94 | 262.57 | 0.9871 | -330.3 | 999999 | |
| 0.00 | 1.73 | 0.00 | 4.67 | -6.48 | 236.34 | 78.82 | 262.61 | 0.9838 | -152.0 | -126.7 | |
| 5.54 | -3.00 | 16.14 | -3.00 | -7.76 | 237.02 | 79.51 | 261.37 | 0.9862 | -395.3 | 999999 | |
| 3.82 | -3.00 | 11.61 | -3.00 | -8.23 | 237.39 | 79.87 | 260.94 | 0.9873 | 41.0 | 999999 | |
| 0.00 | 1.00 | 0.00 | 2.45 | -4.93 | 235.42 | 77.90 | 264.09 | 0.9803 | 502.0 | 468.1 | |
| 0.00 | 1.18 | 0.00 | 2.87 | -5.08 | 235.33 | 77.82 | 263.93 | 0.9800 | 451.0 | 373.5 | |
| 4.27 | 8.90 | 8.57 | 18.03 | -5.02 | 232.76 | 75.24 | 263.74 | 0.9702 | -462.0 | -78.1 | |
| 0.00 | 2.82 | 0.00 | 5.62 | -4.73 | 232.66 | 75.15 | 264.03 | 0.9697 | -354.0 | -317.8 | |
| 0.00 | 3.09 | 0.00 | 6.14 | -5.87 | 232.58 | 75.06 | 262.85 | 0.9698 | -360.0 | -280.7 | |
| 0.00 | 0.27 | 0.00 | 0.53 | -5.60 | 232.24 | 74.72 | 263.10 | 0.9682 | -544.0 | -537.7 | |
| 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. | |