SDO HMI 2014-09-07 06:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.02 | 34.29 | 14.74 | 39.47 | -20.68 | 79.05 | -59.20 | 117.10 | 0.9036 | 49.5 | 55.6 | |
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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 |
| 1.34 | 3.13 | 1.39 | 3.24 | -20.51 | 82.41 | -55.84 | 118.11 | 0.8806 | 620.5 | 461.0 | |
| 0.89 | 2.14 | 0.94 | 2.25 | -20.20 | 81.89 | -56.36 | 117.58 | 0.8835 | 531.2 | 400.2 | |
| 0.71 | 1.61 | 0.76 | 1.70 | -20.42 | 81.70 | -56.55 | 117.75 | 0.8854 | 347.6 | 288.4 | |
| 0.00 | 1.07 | 0.00 | 1.17 | -21.30 | 81.07 | -57.18 | 118.44 | 0.8923 | 482.0 | 434.8 | |
| 0.00 | 0.80 | 0.00 | 0.80 | -17.65 | 82.85 | -55.40 | 115.20 | 0.8688 | 426.0 | 424.4 | |
| 0.71 | 2.50 | 0.80 | 2.81 | -21.54 | 80.12 | -58.13 | 118.35 | 0.8994 | 472.8 | 461.9 | |
| 0.00 | 1.16 | 0.00 | 1.32 | -21.69 | 79.71 | -58.54 | 118.36 | 0.9025 | 156.0 | 134.5 | |
| 3.30 | 5.36 | 3.72 | 6.03 | -21.16 | 79.93 | -58.32 | 117.88 | 0.8997 | 333.2 | 113.7 | |
| 0.00 | 0.27 | 0.00 | 0.31 | -20.20 | 78.90 | -59.35 | 116.52 | 0.9041 | -521.0 | -484.3 | |
| 6.07 | 13.39 | 7.13 | 15.69 | -20.05 | 78.23 | -60.02 | 116.13 | 0.9082 | -427.1 | -308.1 | |
| 0.00 | 2.86 | 0.00 | 4.15 | -22.42 | 73.39 | -64.86 | 117.08 | 0.9414 | 235.0 | 70.6 | |
| 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. | |