SDO HMI 2014-12-06 02:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.18 | 0.00 | 11.41 | -14.68 | 35.47 | 2.14 | 187.42 | 0.2636 | -580.2 | -564.0 | |
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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 | 0.60 | 0.00 | 0.32 | -18.13 | 41.68 | 8.35 | 203.64 | 0.3458 | 768.0 | 668.1 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -16.95 | 40.66 | 7.33 | 202.43 | 0.3214 | 864.0 | 664.2 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -15.15 | 35.66 | 2.32 | 188.38 | 0.2699 | -796.0 | -624.6 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -13.65 | 35.58 | 2.25 | 189.01 | 0.2447 | -904.0 | -695.2 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -13.17 | 35.55 | 2.21 | 189.20 | 0.2364 | -942.0 | -809.8 | |
| 0.00 | 5.72 | 0.00 | 2.94 | -14.84 | 35.56 | 2.23 | 188.21 | 0.2645 | -1009.0 | -719.6 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -15.27 | 35.32 | 1.99 | 187.12 | 0.2712 | -662.0 | -520.7 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -13.23 | 35.09 | 1.76 | 187.30 | 0.2363 | -742.0 | -578.1 | |
| 0.00 | 1.96 | 0.00 | 1.01 | -15.30 | 35.07 | 1.74 | 186.24 | 0.2712 | -605.0 | -587.2 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -15.00 | 34.89 | 1.56 | 185.70 | 0.2657 | -974.0 | -808.9 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -14.87 | 34.64 | 1.31 | 184.84 | 0.2633 | -946.0 | -818.1 | |
| 0.00 | 0.68 | 0.00 | 0.35 | -16.35 | 34.62 | 1.29 | 184.32 | 0.2880 | -516.0 | -500.2 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -12.95 | 34.39 | 1.06 | 184.51 | 0.2304 | -722.0 | -616.8 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -13.04 | 30.85 | -2.49 | 169.59 | 0.2350 | -937.0 | -780.8 | |
| 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. | |