SDO HMI 2014-09-30 04:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.81 | 0.00 | 6.62 | -17.83 | 202.86 | 7.13 | 194.46 | 0.4562 | -105.8 | 19.2 | |
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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 | 2.12 | 0.00 | 1.22 | -17.96 | 214.13 | 18.40 | 216.05 | 0.5124 | 602.0 | 545.6 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -18.12 | 214.01 | 18.29 | 215.68 | 0.5133 | 722.0 | 658.1 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -14.29 | 210.87 | 15.14 | 215.46 | 0.4382 | 426.0 | 532.0 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -15.81 | 208.72 | 13.00 | 209.60 | 0.4401 | 792.0 | 633.6 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -24.48 | 205.09 | 9.37 | 195.98 | 0.5403 | 547.0 | 465.1 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -14.80 | 200.82 | 5.10 | 193.17 | 0.3788 | -762.0 | -658.6 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -19.04 | 197.08 | 1.36 | 182.95 | 0.4377 | -828.0 | -623.3 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -7.10 | 192.92 | -2.81 | 168.54 | 0.2456 | -807.0 | -674.9 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -32.19 | 191.08 | -4.64 | 173.78 | 0.6345 | -575.0 | -477.6 | |
| 0.00 | 1.50 | 0.00 | 0.79 | -13.24 | 191.50 | -4.23 | 168.14 | 0.3508 | -790.0 | -582.6 | |
| 0.00 | 0.71 | 0.00 | 0.46 | -32.70 | 187.68 | -8.05 | 169.49 | 0.6479 | -491.0 | -458.8 | |
| 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. | |