SDO HMI 2014-09-29 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.18 | 0.00 | 6.64 | -17.15 | 208.35 | -2.22 | 174.88 | 0.4168 | 140.1 | 109.0 | |
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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 | 0.53 | 0.00 | 0.30 | -20.83 | 216.02 | 5.45 | 190.84 | 0.4741 | 419.0 | 388.2 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -17.57 | 214.84 | 4.28 | 189.77 | 0.4207 | 815.0 | 606.0 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -18.30 | 214.54 | 3.98 | 188.82 | 0.4313 | 670.0 | 533.5 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -18.13 | 214.51 | 3.94 | 188.80 | 0.4286 | 656.0 | 529.6 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -25.95 | 210.91 | 0.34 | 180.57 | 0.5435 | 675.0 | 473.8 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -8.81 | 209.50 | -1.07 | 176.10 | 0.2714 | -804.0 | -638.5 | |
| 0.00 | 0.71 | 0.00 | 0.36 | -9.00 | 209.07 | -1.49 | 174.61 | 0.2751 | -736.0 | -542.4 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -19.11 | 208.68 | -1.89 | 175.92 | 0.4403 | 751.0 | 586.2 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -13.90 | 208.64 | -1.93 | 174.73 | 0.3570 | 846.0 | 570.7 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -17.86 | 203.24 | -7.32 | 163.77 | 0.4359 | 823.0 | 616.9 | |
| 0.00 | 1.50 | 0.00 | 0.82 | -16.69 | 202.41 | -8.16 | 161.13 | 0.4223 | -828.0 | -710.6 | |
| 0.00 | 0.53 | 0.00 | 0.29 | -14.72 | 201.61 | -8.96 | 157.63 | 0.3974 | -726.0 | -596.7 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -22.57 | 196.35 | -14.22 | 155.05 | 0.5399 | -740.0 | -566.0 | |
| 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. | |