SDO HMI 2014-07-18 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.35 | 52.55 | 6.92 | 27.27 | 7.04 | 112.53 | 17.34 | 278.87 | 0.3006 | 2.0 | -28.7 | |
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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 |
| 1.18 | 7.26 | 0.62 | 3.79 | 6.88 | 113.75 | 18.56 | 277.90 | 0.3204 | -928.0 | -819.7 | |
| 2.18 | 4.54 | 1.14 | 2.37 | 7.64 | 113.62 | 18.43 | 280.34 | 0.3199 | -876.7 | -705.5 | |
| 0.64 | -1.00 | 0.33 | -1.00 | 7.01 | 113.56 | 18.37 | 278.36 | 0.3175 | -1089.1 | 999999 | |
| 0.00 | 5.72 | 0.00 | 2.98 | 7.34 | 113.44 | 18.25 | 279.47 | 0.3163 | -660.0 | -511.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 7.17 | 113.21 | 18.02 | 279.01 | 0.3121 | -113.0 | -141.7 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 6.83 | 113.16 | 17.97 | 277.95 | 0.3107 | -741.0 | -647.5 | |
| 0.00 | 2.18 | 0.00 | 1.13 | 6.93 | 112.78 | 17.59 | 278.42 | 0.3046 | 130.0 | 161.8 | |
| 0.00 | 3.54 | 0.00 | 1.84 | 7.89 | 112.40 | 17.21 | 281.74 | 0.3007 | -950.0 | -758.6 | |
| 0.00 | 2.54 | 0.00 | 1.32 | 6.79 | 112.23 | 17.04 | 278.17 | 0.2952 | 549.0 | 401.6 | |
| 4.72 | 24.41 | 2.44 | 12.61 | 6.80 | 111.88 | 16.69 | 278.33 | 0.2894 | 969.4 | 685.5 | |
| 1.36 | -10.00 | 0.70 | -10.00 | 7.02 | 111.76 | 16.57 | 279.13 | 0.2879 | 866.1 | 999999 | |
| 3.27 | -10.00 | 1.69 | -10.00 | 6.72 | 111.52 | 16.33 | 278.19 | 0.2834 | 1103.1 | 999999 | |
| 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. | |