SDO HMI 2014-11-11 00:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.66 | 0.00 | 12.66 | -23.62 | 8.55 | 4.60 | 189.34 | 0.4626 | 556.3 | 598.8 | |
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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 | 0.86 | 0.00 | 0.48 | -22.36 | 9.99 | 6.04 | 192.65 | 0.4460 | 818.0 | 637.4 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -23.18 | 9.80 | 5.85 | 191.85 | 0.4579 | 716.0 | 602.7 | |
| 0.00 | 2.84 | 0.00 | 1.57 | -22.35 | 9.63 | 5.68 | 191.93 | 0.4448 | 795.0 | 639.9 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -22.25 | 9.41 | 5.45 | 191.51 | 0.4425 | 725.0 | 638.8 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -22.02 | 9.40 | 5.44 | 191.61 | 0.4390 | 843.0 | 732.6 | |
| 0.00 | 1.46 | 0.00 | 0.83 | -24.88 | 9.12 | 5.17 | 189.80 | 0.4817 | 695.0 | 554.6 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -23.48 | 9.06 | 5.11 | 190.27 | 0.4602 | 805.0 | 663.5 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -24.21 | 8.99 | 5.04 | 189.83 | 0.4712 | 733.0 | 595.5 | |
| 0.00 | 1.81 | 0.00 | 1.01 | -23.71 | 8.94 | 4.99 | 189.94 | 0.4634 | 778.0 | 654.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -24.41 | 8.97 | 5.02 | 189.71 | 0.4742 | 766.0 | 639.6 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -22.15 | 8.89 | 4.93 | 190.49 | 0.4394 | 598.0 | 548.3 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -24.68 | 8.95 | 4.99 | 189.56 | 0.4782 | 821.0 | 616.6 | |
| 0.00 | 6.03 | 0.00 | 3.37 | -23.91 | 8.72 | 4.77 | 189.43 | 0.4659 | 605.0 | 775.3 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -26.56 | 2.74 | -1.21 | 177.83 | 0.5010 | -672.0 | -581.6 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -26.23 | 357.57 | -6.38 | 168.58 | 0.5053 | -682.0 | -507.5 | |
| 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. | |