SDO HMI 2014-01-07 00:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.95 | 0.00 | 9.70 | -17.98 | 77.69 | -32.76 | 116.71 | 0.5771 | 411.1 | 392.6 | |
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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 | 2.63 | 0.00 | 1.51 | -18.67 | 83.36 | -27.09 | 121.57 | 0.5085 | 826.0 | 627.7 | |
| 0.00 | 0.93 | 0.00 | 0.54 | -18.91 | 83.18 | -27.27 | 121.84 | 0.5124 | 922.0 | 753.1 | |
| 0.00 | 1.87 | 0.00 | 1.08 | -19.19 | 82.49 | -27.96 | 121.78 | 0.5230 | 557.0 | 432.0 | |
| 0.00 | 1.02 | 0.00 | 0.59 | -13.57 | 80.01 | -30.45 | 110.09 | 0.5266 | -786.0 | -719.0 | |
| 0.00 | 1.19 | 0.00 | 0.71 | -13.19 | 77.82 | -32.64 | 108.43 | 0.5556 | -655.0 | -526.4 | |
| 0.00 | 1.44 | 0.00 | 0.88 | -16.80 | 76.70 | -33.75 | 114.04 | 0.5846 | 616.0 | 457.1 | |
| 0.00 | 1.19 | 0.00 | 0.75 | -18.63 | 74.13 | -36.33 | 115.66 | 0.6251 | 714.0 | 624.8 | |
| 0.00 | 3.48 | 0.00 | 2.20 | -18.36 | 74.16 | -36.30 | 115.26 | 0.6235 | 665.0 | 549.4 | |
| 0.00 | 0.93 | 0.00 | 0.60 | -19.02 | 73.76 | -36.70 | 116.07 | 0.6313 | 631.0 | 542.1 | |
| 0.00 | 0.59 | 0.00 | 0.39 | -20.73 | 72.65 | -37.80 | 118.07 | 0.6520 | 607.0 | 538.9 | |
| 0.00 | 0.68 | 0.00 | 0.45 | -20.50 | 72.12 | -38.34 | 117.48 | 0.6572 | 425.0 | 380.2 | |
| 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. | |