SDO HMI 2014-09-19 13:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.79 | 0.00 | 9.88 | 8.81 | 333.37 | -2.60 | 143.11 | 0.1240 | 14.7 | 108.4 | |
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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 | 1.24 | 0.00 | 0.62 | 9.11 | 344.45 | 8.48 | 283.94 | 0.1507 | 145.0 | 172.7 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 9.27 | 343.59 | 7.62 | 286.50 | 0.1371 | -776.0 | -540.1 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 11.65 | 342.35 | 6.38 | 306.24 | 0.1356 | -833.0 | -619.2 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 1.97 | 339.76 | 3.79 | 216.48 | 0.1116 | -833.0 | -618.6 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 10.47 | 339.56 | 3.59 | 313.71 | 0.0855 | -815.0 | -604.5 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 8.50 | 337.46 | 1.49 | 313.20 | 0.0355 | -893.0 | -741.8 | |
| 0.00 | 1.42 | 0.00 | 0.70 | 9.95 | 334.08 | -1.89 | 33.34 | 0.0595 | -754.0 | -537.2 | |
| 0.00 | 1.51 | 0.00 | 0.75 | 14.11 | 332.81 | -3.16 | 23.67 | 0.1338 | -803.0 | -643.9 | |
| 0.00 | 2.04 | 0.00 | 1.01 | 6.08 | 331.73 | -4.24 | 103.54 | 0.0761 | 940.0 | 731.0 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 8.88 | 329.10 | -6.87 | 74.98 | 0.1229 | 737.0 | 596.5 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 7.69 | 328.08 | -7.89 | 85.28 | 0.1372 | 821.0 | 714.2 | |
| 0.00 | 2.75 | 0.00 | 1.38 | 7.72 | 327.83 | -8.14 | 85.20 | 0.1414 | 804.0 | 713.0 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 7.71 | 327.06 | -8.91 | 85.61 | 0.1546 | 865.0 | 692.3 | |
| 0.00 | 1.60 | 0.00 | 0.80 | 8.24 | 326.74 | -9.23 | 82.37 | 0.1608 | 840.0 | 689.8 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 14.32 | 324.21 | -11.76 | 57.05 | 0.2363 | 775.0 | 587.3 | |
| 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. | |