SDO HMI 2014-07-13 19:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.24 | 427.18 | 113.24 | 660.36 | -7.76 | 221.99 | 70.54 | 260.36 | 0.9489 | 631.4 | 191.4 | |
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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 | 1.82 | 0.00 | 2.98 | -5.17 | 223.32 | 71.88 | 263.22 | 0.9545 | 311.0 | 283.4 | |
| 1.09 | 2.63 | 1.62 | 3.91 | -4.67 | 221.48 | 70.04 | 263.54 | 0.9442 | -153.3 | -83.4 | |
| 69.43 | 385.98 | 109.23 | 604.63 | -7.79 | 222.26 | 70.81 | 260.37 | 0.9505 | 715.6 | 209.3 | |
| 0.00 | 9.17 | 0.00 | 12.57 | -6.15 | 219.59 | 68.14 | 261.75 | 0.9340 | -497.0 | -422.8 | |
| 0.00 | 1.54 | 0.00 | 2.08 | -5.56 | 219.19 | 67.75 | 262.32 | 0.9311 | -312.0 | -285.2 | |
| 0.00 | 12.25 | 0.00 | 16.31 | -6.80 | 218.78 | 67.34 | 260.95 | 0.9295 | 645.0 | 310.2 | |
| 1.72 | 6.53 | 2.39 | 9.06 | -9.52 | 219.41 | 67.97 | 258.15 | 0.9356 | 221.9 | 130.6 | |
| 0.00 | 1.27 | 0.00 | 1.72 | -9.26 | 218.89 | 67.45 | 258.34 | 0.9323 | -23.0 | -65.6 | |
| 0.00 | 0.73 | 0.00 | 0.99 | -9.89 | 218.90 | 67.46 | 257.68 | 0.9329 | 160.0 | 100.0 | |
| 0.00 | 1.18 | 0.00 | 1.53 | -9.04 | 217.93 | 66.49 | 258.43 | 0.9260 | -311.0 | -291.4 | |
| 0.00 | 0.54 | 0.00 | 0.60 | -9.13 | 213.70 | 62.26 | 257.63 | 0.8965 | -446.0 | -371.5 | |
| 0.00 | 1.54 | 0.00 | 1.77 | -12.70 | 214.08 | 62.64 | 253.79 | 0.9041 | 354.0 | 339.7 | |
| 0.00 | 1.18 | 0.00 | 1.34 | -12.36 | 213.73 | 62.29 | 254.08 | 0.9010 | 540.0 | 506.3 | |
| 0.00 | 0.82 | 0.00 | 0.87 | -11.87 | 212.09 | 60.65 | 254.27 | 0.8880 | -424.0 | -299.0 | |
| 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. | |