SDO HMI 2014-12-05 23:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.29 | 0.00 | 11.10 | 15.06 | 15.47 | -19.51 | 51.36 | 0.4138 | -460.2 | -335.6 | |
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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 | 1.11 | 0.00 | 0.58 | 16.65 | 24.86 | -10.13 | 30.86 | 0.3298 | -792.0 | -642.1 | |
| 0.00 | 1.88 | 0.00 | 0.98 | 14.30 | 21.86 | -13.12 | 42.25 | 0.3287 | -891.0 | -683.3 | |
| 0.00 | 2.30 | 0.00 | 1.19 | 7.59 | 20.06 | -14.92 | 63.48 | 0.2865 | -829.0 | -591.5 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 13.90 | 18.77 | -16.22 | 49.01 | 0.3607 | -1023.0 | -853.1 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 18.39 | 18.35 | -16.63 | 41.13 | 0.4145 | -709.0 | -551.9 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 18.58 | 17.82 | -17.17 | 41.70 | 0.4224 | -636.0 | -569.3 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 10.31 | 17.48 | -17.50 | 59.50 | 0.3449 | -772.0 | -554.4 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 9.83 | 17.47 | -17.51 | 60.74 | 0.3413 | -784.0 | -676.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 13.27 | 16.87 | -18.11 | 53.38 | 0.3786 | -946.0 | -742.9 | |
| 0.00 | 3.41 | 0.00 | 1.90 | 16.78 | 13.21 | -21.77 | 51.33 | 0.4567 | -637.0 | -425.5 | |
| 0.00 | 2.64 | 0.00 | 1.53 | 19.48 | 9.64 | -25.35 | 50.80 | 0.5229 | 778.0 | 613.0 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 22.54 | 4.57 | -30.41 | 50.95 | 0.6044 | 624.0 | 510.1 | |
| 0.00 | 0.85 | 0.00 | 0.53 | 16.03 | 0.73 | -34.25 | 63.29 | 0.6078 | 634.0 | 526.8 | |
| 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. | |