SDO HMI 2014-10-09 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.43 | 0.00 | 12.62 | -21.25 | 74.98 | 2.93 | 186.18 | 0.4735 | 279.2 | 191.6 | |
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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 | 0.79 | 0.00 | 0.45 | -21.30 | 82.43 | 10.39 | 200.03 | 0.4925 | 617.0 | 492.8 | |
| 0.00 | 0.61 | 0.00 | 0.35 | -21.17 | 81.31 | 9.27 | 198.12 | 0.4851 | 710.0 | 623.0 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -21.53 | 80.59 | 8.54 | 196.55 | 0.4870 | 644.0 | 487.6 | |
| 0.00 | 2.28 | 0.00 | 1.28 | -21.05 | 80.49 | 8.45 | 196.69 | 0.4797 | 644.0 | 510.8 | |
| 0.00 | 1.31 | 0.00 | 0.73 | -19.46 | 79.35 | 7.31 | 195.48 | 0.4512 | 671.0 | 618.1 | |
| 0.00 | 4.03 | 0.00 | 2.27 | -21.30 | 79.21 | 7.17 | 194.13 | 0.4781 | 661.0 | 524.0 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -17.00 | 77.90 | 5.85 | 193.89 | 0.4079 | 786.0 | 638.9 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -17.03 | 77.64 | 5.60 | 193.30 | 0.4074 | 814.0 | 753.4 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -18.61 | 74.40 | 2.36 | 185.29 | 0.4239 | 817.0 | 675.4 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -20.07 | 74.29 | 2.25 | 184.75 | 0.4467 | 744.0 | 593.2 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -22.98 | 73.62 | 1.57 | 182.96 | 0.4910 | 570.0 | 419.2 | |
| 0.00 | 1.67 | 0.00 | 0.93 | -21.61 | 69.80 | -2.24 | 175.55 | 0.4707 | -459.0 | -433.2 | |
| 0.00 | 1.40 | 0.00 | 0.79 | -21.59 | 68.64 | -3.40 | 173.26 | 0.4720 | -787.0 | -550.4 | |
| 0.00 | 1.67 | 0.00 | 0.99 | -26.85 | 67.68 | -4.36 | 172.91 | 0.5521 | -598.0 | -508.8 | |
| 0.00 | 1.31 | 0.00 | 0.75 | -23.58 | 67.74 | -4.31 | 172.12 | 0.5039 | -590.0 | -491.3 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -20.52 | 66.55 | -5.49 | 168.73 | 0.4607 | -776.0 | -600.4 | |
| 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. | |