SDO HMI 2014-09-26 03:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.24 | 25.88 | 0.79 | 17.22 | 7.01 | 206.87 | -42.18 | 87.26 | 0.6692 | -48.2 | 92.7 | |
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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 | 0.97 | 0.00 | 0.61 | 6.35 | 210.44 | -38.62 | 88.53 | 0.6228 | -701.0 | -607.6 | |
| 0.00 | 0.35 | 0.00 | 0.22 | 6.67 | 210.25 | -38.80 | 88.00 | 0.6251 | -632.0 | -526.5 | |
| 0.00 | 1.24 | 0.00 | 0.79 | 6.08 | 209.72 | -39.34 | 88.88 | 0.6327 | -614.0 | -417.4 | |
| 0.00 | 1.94 | 0.00 | 1.24 | 7.00 | 209.44 | -39.62 | 87.42 | 0.6359 | -816.0 | -580.6 | |
| 1.24 | 2.30 | 0.79 | 1.47 | 6.43 | 209.45 | -39.60 | 88.32 | 0.6360 | -611.2 | -497.8 | |
| 0.00 | 0.97 | 0.00 | 0.63 | 5.72 | 208.96 | -40.10 | 89.37 | 0.6432 | -689.0 | -588.6 | |
| 0.00 | 0.97 | 0.00 | 0.63 | 6.85 | 208.26 | -40.80 | 87.57 | 0.6516 | -461.0 | -413.7 | |
| 0.00 | 3.00 | 0.00 | 1.97 | 6.98 | 207.97 | -41.09 | 87.35 | 0.6554 | -619.0 | -442.2 | |
| 0.00 | 1.15 | 0.00 | 0.78 | 6.68 | 205.82 | -43.23 | 87.64 | 0.6832 | 650.0 | 591.8 | |
| 0.00 | 0.71 | 0.00 | 0.48 | 8.92 | 205.41 | -43.65 | 84.35 | 0.6875 | 537.0 | 423.6 | |
| 0.00 | 5.83 | 0.00 | 3.97 | 7.02 | 205.49 | -43.57 | 87.12 | 0.6872 | 795.0 | 684.7 | |
| 0.00 | 0.88 | 0.00 | 0.60 | 7.40 | 205.36 | -43.69 | 86.56 | 0.6886 | 474.0 | 348.9 | |
| 0.00 | 1.33 | 0.00 | 0.91 | 8.69 | 204.89 | -44.17 | 84.66 | 0.6940 | 477.0 | 410.1 | |
| 0.00 | 2.56 | 0.00 | 1.76 | 7.53 | 204.71 | -44.35 | 86.33 | 0.6967 | 180.0 | 248.9 | |
| 0.00 | 0.88 | 0.00 | 0.61 | 7.69 | 204.48 | -44.58 | 86.09 | 0.6995 | 597.0 | 457.5 | |
| 0.00 | 0.80 | 0.00 | 0.55 | 5.52 | 204.21 | -44.85 | 89.16 | 0.7044 | 543.0 | 408.3 | |
| 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. | |