SDO HMI 2014-06-06 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.43 | 267.95 | 23.17 | 136.61 | -4.24 | 302.39 | 12.95 | 251.84 | 0.2366 | 932.8 | 428.9 | |
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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 | 3.53 | 0.00 | 1.82 | -5.02 | 304.37 | 14.94 | 251.41 | 0.2722 | 1080.0 | 766.6 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -6.54 | 303.56 | 14.13 | 245.03 | 0.2687 | 717.0 | 594.5 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -5.41 | 303.50 | 14.07 | 248.92 | 0.2605 | 918.0 | 804.1 | |
| 37.65 | 221.80 | 19.20 | 113.13 | -4.01 | 302.63 | 13.19 | 253.18 | 0.2389 | 1353.4 | 444.2 | |
| 7.78 | 14.93 | 3.97 | 7.62 | -5.47 | 302.12 | 12.69 | 246.67 | 0.2391 | 1098.1 | 675.6 | |
| 0.00 | 3.98 | 0.00 | 2.03 | -5.75 | 301.62 | 12.19 | 244.76 | 0.2333 | 619.0 | 653.8 | |
| 0.00 | 7.78 | 0.00 | 3.95 | -4.55 | 301.35 | 11.92 | 249.16 | 0.2213 | 572.0 | 507.2 | |
| 0.00 | 1.81 | 0.00 | 0.92 | -4.71 | 300.89 | 11.45 | 247.74 | 0.2148 | 763.0 | 554.4 | |
| 0.00 | 2.17 | 0.00 | 1.10 | -5.44 | 300.18 | 10.75 | 243.22 | 0.2089 | -459.0 | -378.7 | |
| 0.00 | 1.90 | 0.00 | 0.96 | -3.91 | 299.70 | 10.26 | 249.30 | 0.1909 | 892.0 | 780.6 | |
| 0.00 | 1.00 | 0.00 | 0.50 | -2.94 | 299.44 | 10.01 | 253.87 | 0.1814 | -619.0 | -471.4 | |
| 0.00 | 0.45 | 0.00 | 0.23 | -7.15 | 298.60 | 9.16 | 232.01 | 0.2014 | -335.0 | -461.2 | |
| 0.00 | 4.52 | 0.00 | 2.28 | -7.55 | 297.68 | 8.24 | 227.48 | 0.1937 | -868.0 | -540.4 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -3.02 | 295.81 | 6.37 | 245.01 | 0.1229 | -819.0 | -639.9 | |
| 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. | |