SDO HMI 2014-12-06 01:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.01 | 0.00 | 11.30 | -14.51 | 36.10 | 2.22 | 188.06 | 0.2613 | -535.1 | -501.3 | |
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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 | 1.28 | 0.00 | 0.67 | -16.97 | 40.68 | 6.80 | 200.92 | 0.3187 | 818.0 | 635.3 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -19.40 | 40.08 | 6.20 | 196.85 | 0.3532 | 748.0 | 595.8 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -12.59 | 39.82 | 5.94 | 204.40 | 0.2455 | 815.0 | 563.3 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -12.86 | 36.97 | 3.09 | 193.02 | 0.2342 | -820.0 | -651.8 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -13.07 | 36.88 | 3.00 | 192.46 | 0.2374 | -739.0 | -571.0 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -15.14 | 35.71 | 1.83 | 186.62 | 0.2688 | -742.0 | -543.1 | |
| 0.00 | 3.24 | 0.00 | 1.66 | -14.90 | 35.65 | 1.77 | 186.50 | 0.2646 | -908.0 | -822.9 | |
| 0.00 | 1.79 | 0.00 | 0.91 | -13.65 | 35.61 | 1.73 | 186.95 | 0.2434 | -870.0 | -624.3 | |
| 0.00 | 1.79 | 0.00 | 0.91 | -13.13 | 35.49 | 1.61 | 186.71 | 0.2344 | -970.0 | -755.9 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -14.47 | 35.37 | 1.49 | 185.65 | 0.2569 | -945.0 | -759.7 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -15.36 | 35.04 | 1.16 | 184.14 | 0.2713 | -799.0 | -676.9 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -15.05 | 34.86 | 0.97 | 183.56 | 0.2660 | -1015.0 | -879.2 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -14.83 | 34.64 | 0.76 | 182.82 | 0.2621 | -956.0 | -809.4 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -15.11 | 34.58 | 0.70 | 182.54 | 0.2667 | -745.0 | -683.1 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -13.03 | 30.82 | -3.06 | 167.25 | 0.2370 | -899.0 | -797.9 | |
| 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. | |