SDO HMI 2014-11-11 04:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.16 | 0.00 | 13.00 | -23.73 | 8.84 | 7.08 | 194.00 | 0.4706 | 687.4 | 621.3 | |
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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 | 0.95 | 0.00 | 0.52 | -21.34 | 10.32 | 8.57 | 198.43 | 0.4408 | 693.0 | 501.2 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -22.35 | 9.96 | 8.21 | 196.97 | 0.4541 | 852.0 | 648.9 | |
| 0.00 | 3.53 | 0.00 | 1.98 | -23.21 | 9.72 | 7.96 | 195.93 | 0.4657 | 681.0 | 496.1 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -22.18 | 9.40 | 7.65 | 195.99 | 0.4491 | 888.0 | 758.4 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -23.40 | 9.01 | 7.26 | 194.47 | 0.4657 | 900.0 | 593.4 | |
| 0.00 | 1.46 | 0.00 | 0.82 | -23.70 | 9.00 | 7.24 | 194.27 | 0.4701 | 817.0 | 651.2 | |
| 0.00 | 3.88 | 0.00 | 2.20 | -24.87 | 9.03 | 7.27 | 193.68 | 0.4877 | 555.0 | 595.9 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -24.17 | 8.86 | 7.10 | 193.75 | 0.4766 | 768.0 | 589.8 | |
| 0.00 | 5.34 | 0.00 | 3.00 | -23.86 | 8.71 | 6.95 | 193.64 | 0.4715 | 699.0 | 771.5 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -24.26 | 8.57 | 6.81 | 193.16 | 0.4770 | 703.0 | 554.1 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -23.92 | 7.96 | 6.21 | 192.19 | 0.4699 | 837.0 | 667.5 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -24.35 | 7.36 | 5.60 | 190.85 | 0.4745 | 717.0 | 567.8 | |
| 0.00 | 0.34 | 0.00 | 0.20 | -26.09 | 357.67 | -4.08 | 172.58 | 0.4970 | -174.0 | -247.5 | |
| 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. | |