SDO HMI 2014-07-08 15:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.87 | 0.00 | 10.36 | -16.25 | 234.24 | 14.41 | 214.64 | 0.4274 | -13.6 | 5.1 | |
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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 | 0.91 | 0.00 | 0.53 | -18.39 | 243.72 | 23.89 | 226.07 | 0.5356 | 363.0 | 355.6 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -16.01 | 242.54 | 22.70 | 228.19 | 0.4997 | 440.0 | 426.1 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -14.25 | 237.88 | 18.04 | 224.59 | 0.4294 | 789.0 | 618.2 | |
| 0.00 | 2.36 | 0.00 | 1.30 | -15.08 | 237.32 | 17.48 | 222.34 | 0.4324 | 999.0 | 770.3 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -14.10 | 236.78 | 16.94 | 223.07 | 0.4156 | 762.0 | 533.4 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -15.48 | 236.59 | 16.76 | 220.51 | 0.4295 | 730.0 | 530.8 | |
| 0.00 | 1.45 | 0.00 | 0.79 | -14.56 | 235.76 | 15.93 | 220.56 | 0.4102 | 811.0 | 570.3 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -17.56 | 233.29 | 13.46 | 211.64 | 0.4249 | -822.0 | -751.5 | |
| 0.00 | 2.45 | 0.00 | 1.34 | -17.55 | 232.64 | 12.80 | 210.39 | 0.4194 | -931.0 | -749.3 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -16.86 | 232.43 | 12.59 | 210.87 | 0.4084 | -819.0 | -617.4 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -17.09 | 232.18 | 12.35 | 210.09 | 0.4094 | -946.0 | -805.9 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -13.73 | 226.83 | 6.99 | 201.62 | 0.3223 | -897.0 | -712.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -23.71 | 213.56 | -6.27 | 167.72 | 0.4720 | -656.0 | -496.1 | |
| 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. | |