SDO HMI 2014-12-05 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.26 | 0.00 | 10.20 | 13.70 | 18.89 | -23.80 | 59.29 | 0.4606 | -629.9 | -495.1 | |
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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 | 1.45 | 0.00 | 0.78 | 18.26 | 26.90 | -15.79 | 40.01 | 0.4036 | -694.0 | -555.1 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 15.18 | 24.44 | -18.25 | 49.70 | 0.3980 | -746.0 | -585.2 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 15.15 | 24.06 | -18.63 | 50.33 | 0.4024 | -822.0 | -662.0 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 14.75 | 21.78 | -20.90 | 54.17 | 0.4274 | -815.0 | -579.3 | |
| 0.00 | 2.05 | 0.00 | 1.11 | 7.85 | 20.28 | -22.41 | 70.86 | 0.4015 | -728.0 | -681.0 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 15.45 | 19.26 | -23.43 | 55.74 | 0.4657 | -600.0 | -455.5 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 13.74 | 18.49 | -24.20 | 59.75 | 0.4629 | -812.0 | -725.9 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 13.25 | 17.80 | -24.89 | 61.33 | 0.4688 | -775.0 | -572.5 | |
| 0.00 | 0.68 | 0.00 | 0.38 | 13.47 | 17.55 | -25.14 | 61.15 | 0.4737 | -646.0 | -601.2 | |
| 0.00 | 0.68 | 0.00 | 0.38 | 8.89 | 17.47 | -25.22 | 70.48 | 0.4486 | -718.0 | -620.9 | |
| 0.00 | 2.90 | 0.00 | 1.61 | 9.97 | 17.35 | -25.34 | 68.29 | 0.4556 | -819.0 | -457.7 | |
| 0.00 | 1.37 | 0.00 | 0.81 | 20.19 | 15.41 | -27.28 | 51.67 | 0.5506 | -661.0 | -524.5 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 12.19 | 14.40 | -28.29 | 66.03 | 0.5091 | -698.0 | -553.7 | |
| 0.00 | 1.02 | 0.00 | 0.64 | 19.24 | 9.15 | -33.54 | 58.09 | 0.6168 | 715.0 | 590.2 | |
| 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. | |