SDO HMI 2014-07-06 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.26 | 0.00 | 10.22 | 4.95 | 257.87 | 4.98 | 151.53 | 0.1485 | 768.2 | 636.1 | |
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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 | 1.09 | 0.00 | 0.63 | 4.70 | 283.98 | 31.09 | 273.44 | 0.5176 | -681.0 | -609.2 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 0.93 | 268.73 | 15.83 | 261.43 | 0.2771 | 791.0 | 643.0 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 3.09 | 267.08 | 14.18 | 269.10 | 0.2458 | 750.0 | 641.8 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 9.13 | 267.03 | 14.13 | 292.83 | 0.2627 | 839.0 | 716.3 | |
| 0.00 | 2.73 | 0.00 | 1.36 | 5.95 | 259.56 | 6.67 | 291.17 | 0.1244 | 871.0 | 634.2 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 0.95 | 259.31 | 6.41 | 249.16 | 0.1200 | 952.0 | 768.8 | |
| 0.00 | 0.55 | 0.00 | 0.27 | -2.55 | 257.35 | 4.45 | 216.80 | 0.1300 | 839.0 | 608.2 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -3.31 | 257.13 | 4.24 | 212.26 | 0.1389 | 734.0 | 551.7 | |
| 0.00 | 1.82 | 0.00 | 0.90 | 7.60 | 251.49 | -1.41 | 18.44 | 0.0774 | 932.0 | 789.0 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 7.78 | 251.43 | -1.47 | 18.44 | 0.0807 | 1016.0 | 788.5 | |
| 0.00 | 4.18 | 0.00 | 2.08 | 7.48 | 251.27 | -1.62 | 21.60 | 0.0766 | 1079.0 | 777.2 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 6.93 | 250.29 | -2.61 | 36.32 | 0.0765 | 761.0 | 569.3 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 3.51 | 248.65 | -4.25 | 88.56 | 0.0743 | 1104.0 | 930.3 | |
| 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. | |