SDO HMI 2014-12-09 04:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.36 | 0.00 | 7.08 | 13.63 | 19.19 | 26.48 | 299.60 | 0.5003 | -514.7 | -421.4 | |
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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 | 1.02 | 0.00 | 0.64 | 16.89 | 26.51 | 33.80 | 298.78 | 0.6097 | -625.0 | -468.8 | |
| 0.00 | 1.19 | 0.00 | 0.72 | 12.91 | 25.73 | 33.02 | 292.99 | 0.5793 | -606.0 | -518.7 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 13.49 | 25.31 | 32.60 | 294.17 | 0.5766 | -147.0 | -160.5 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 4.79 | 23.13 | 30.42 | 279.63 | 0.5139 | -769.0 | -614.2 | |
| 0.00 | 0.43 | 0.00 | 0.25 | 15.13 | 23.53 | 30.82 | 298.00 | 0.5624 | -620.0 | -533.6 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 12.72 | 21.56 | 28.86 | 295.28 | 0.5227 | -713.0 | -614.3 | |
| 0.00 | 0.68 | 0.00 | 0.39 | 15.37 | 17.77 | 25.06 | 303.19 | 0.4901 | -659.0 | -549.0 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 11.30 | 17.15 | 24.44 | 296.03 | 0.4534 | -811.0 | -665.8 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 14.61 | 14.11 | 21.41 | 305.76 | 0.4371 | -195.0 | -293.2 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 14.73 | 13.63 | 20.93 | 306.58 | 0.4321 | -804.0 | -632.9 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 15.31 | 12.78 | 20.07 | 308.81 | 0.4266 | -722.0 | -485.9 | |
| 0.00 | 0.34 | 0.00 | 0.19 | 15.03 | 12.72 | 20.01 | 308.36 | 0.4233 | -735.0 | -693.0 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 18.09 | 10.00 | 17.30 | 317.89 | 0.4233 | 715.0 | 543.9 | |
| 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. | |