SDO HMI 2014-12-01 13:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.84 | 443.59 | 36.52 | 238.53 | 16.68 | 110.00 | 16.79 | 314.75 | 0.3911 | -929.4 | -326.1 | |
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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 |
| 66.30 | 420.44 | 35.69 | 226.29 | 16.64 | 110.27 | 17.06 | 314.15 | 0.3934 | -1555.8 | -391.2 | |
| 1.54 | -1.00 | 0.83 | -1.00 | 16.98 | 109.63 | 16.41 | 315.86 | 0.3898 | -1018.1 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 16.49 | 108.11 | 14.90 | 317.64 | 0.3674 | 569.0 | 475.0 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 17.98 | 107.50 | 14.28 | 321.51 | 0.3786 | 716.0 | 540.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 16.96 | 107.22 | 14.01 | 320.21 | 0.3634 | 790.0 | 592.7 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 17.36 | 106.78 | 13.56 | 321.83 | 0.3638 | 797.0 | 603.1 | |
| 0.00 | 4.61 | 0.00 | 2.46 | 17.79 | 106.78 | 13.56 | 322.59 | 0.3692 | 877.0 | 792.9 | |
| 0.00 | 0.51 | 0.00 | 0.27 | 18.29 | 106.72 | 13.51 | 323.55 | 0.3749 | 727.0 | 609.3 | |
| 0.00 | 2.65 | 0.00 | 1.40 | 17.09 | 105.27 | 12.05 | 324.54 | 0.3455 | 839.0 | 723.0 | |
| 0.00 | 2.65 | 0.00 | 1.40 | 17.18 | 104.80 | 11.58 | 325.75 | 0.3423 | 914.0 | 721.3 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 17.18 | 104.64 | 11.42 | 326.11 | 0.3408 | 962.0 | 766.8 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 16.08 | 104.23 | 11.01 | 325.10 | 0.3222 | 839.0 | 692.3 | |
| 0.00 | 3.16 | 0.00 | 1.66 | 17.40 | 104.24 | 11.03 | 327.39 | 0.3402 | 771.0 | 657.8 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 15.66 | 102.33 | 9.12 | 329.20 | 0.2993 | 755.0 | 547.8 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 19.39 | 101.74 | 8.52 | 336.30 | 0.3492 | 791.0 | 634.3 | |
| 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. | |