SDO HMI 2014-12-06 18:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.45 | 0.00 | 10.22 | 15.37 | 15.28 | -9.28 | 340.90 | 0.3137 | -355.3 | -307.1 | |
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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 | 0.77 | 0.00 | 0.40 | 15.92 | 28.05 | 3.49 | 347.83 | 0.2786 | 643.0 | 605.4 | |
| 0.00 | 1.79 | 0.00 | 0.91 | 12.22 | 21.83 | -2.74 | 12.64 | 0.2146 | -828.0 | -594.6 | |
| 0.00 | 1.71 | 0.00 | 0.88 | 17.10 | 21.18 | -3.38 | 10.98 | 0.2976 | -843.0 | -582.8 | |
| 0.00 | 0.85 | 0.00 | 0.43 | 12.89 | 21.22 | -3.35 | 14.54 | 0.2281 | -1002.0 | -858.5 | |
| 0.00 | 1.28 | 0.00 | 0.65 | 13.31 | 19.42 | -5.15 | 21.06 | 0.2444 | -1062.0 | -822.6 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.60 | 18.93 | -5.63 | 19.59 | 0.2833 | -789.0 | -644.8 | |
| 0.00 | 1.96 | 0.00 | 1.00 | 13.01 | 18.29 | -6.27 | 25.63 | 0.2472 | -850.0 | -576.3 | |
| 0.00 | 1.88 | 0.00 | 0.95 | 9.64 | 17.52 | -7.05 | 36.38 | 0.2049 | -963.0 | -827.7 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 13.25 | 17.28 | -7.29 | 28.65 | 0.2587 | -918.0 | -665.7 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 12.01 | 16.77 | -7.80 | 32.94 | 0.2453 | -739.0 | -727.9 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 15.54 | 13.29 | -11.27 | 35.43 | 0.3264 | -774.0 | -591.6 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 22.09 | 9.14 | -15.43 | 33.45 | 0.4491 | 717.0 | 594.3 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 18.69 | 9.19 | -15.38 | 38.35 | 0.4066 | 668.0 | 586.3 | |
| 0.00 | 0.60 | 0.00 | 0.36 | 24.15 | 359.27 | -25.30 | 43.81 | 0.5654 | 788.0 | 639.1 | |
| 0.00 | 1.62 | 0.00 | 0.95 | 20.01 | 358.80 | -25.77 | 50.28 | 0.5332 | 623.0 | 470.1 | |
| 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. | |