SDO HMI 2014-06-08 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.67 | 0.00 | 9.92 | 3.76 | 260.47 | 2.44 | 204.23 | 0.1659 | 382.3 | 215.9 | |
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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 | 1.45 | 0.00 | 0.75 | 6.04 | 274.25 | 16.22 | 290.09 | 0.2971 | -773.0 | -622.7 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 4.70 | 272.88 | 14.85 | 287.04 | 0.2684 | -774.0 | -617.2 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 4.49 | 272.31 | 14.28 | 286.87 | 0.2581 | -776.0 | -663.1 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 4.46 | 272.06 | 14.03 | 287.04 | 0.2539 | -943.0 | -853.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 4.60 | 261.33 | 3.30 | 323.07 | 0.0960 | 901.0 | 652.2 | |
| 0.00 | 1.00 | 0.00 | 0.49 | 3.87 | 260.50 | 2.47 | 325.92 | 0.0772 | 886.0 | 710.2 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 6.50 | 259.75 | 1.72 | 344.73 | 0.1139 | 947.0 | 748.2 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 5.98 | 258.22 | 0.19 | 358.11 | 0.1009 | 798.0 | 616.9 | |
| 0.00 | 1.54 | 0.00 | 0.76 | 0.37 | 257.30 | -0.73 | 78.08 | 0.0131 | 838.0 | 704.3 | |
| 0.00 | 2.35 | 0.00 | 1.17 | -0.20 | 254.77 | -3.26 | 97.36 | 0.0575 | 844.0 | 681.4 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 5.80 | 252.86 | -5.17 | 42.65 | 0.1329 | 876.0 | 650.5 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 9.24 | 252.45 | -5.58 | 31.46 | 0.1846 | 761.0 | 446.4 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -1.26 | 247.19 | -10.84 | 97.80 | 0.1906 | 901.0 | 743.1 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 1.42 | 243.23 | -14.80 | 85.29 | 0.2574 | 866.0 | 636.5 | |
| 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. | |