SDO HMI 2014-09-13 10:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.09 | 37.21 | 9.34 | 48.72 | 13.71 | 348.09 | -68.74 | 78.09 | 0.9248 | -95.5 | 183.8 | |
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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 | 0.53 | 0.00 | 0.56 | 12.13 | 354.45 | -62.37 | 80.08 | 0.8813 | -470.0 | -498.3 | |
| 0.00 | 0.71 | 0.00 | 0.75 | 12.21 | 354.08 | -62.75 | 79.97 | 0.8843 | -486.0 | -436.0 | |
| 6.76 | 10.06 | 7.19 | 10.71 | 12.48 | 353.76 | -63.07 | 79.65 | 0.8868 | -396.8 | -138.4 | |
| 0.00 | 0.80 | 0.00 | 0.85 | 11.65 | 353.97 | -62.85 | 80.61 | 0.8853 | -322.0 | -286.3 | |
| 0.00 | 0.27 | 0.00 | 0.28 | 8.34 | 354.56 | -62.27 | 84.39 | 0.8820 | 106.0 | 135.3 | |
| 0.00 | 0.98 | 0.00 | 1.03 | 8.73 | 354.18 | -62.65 | 83.92 | 0.8848 | -384.0 | -368.3 | |
| 0.00 | 0.98 | 0.00 | 1.16 | 16.55 | 350.41 | -66.41 | 75.06 | 0.9110 | -152.0 | -156.0 | |
| 0.00 | 4.63 | 0.00 | 6.29 | 14.37 | 347.17 | -69.66 | 77.35 | 0.9325 | 392.0 | 410.3 | |
| 0.00 | 3.29 | 0.00 | 4.50 | 13.97 | 346.99 | -69.84 | 77.76 | 0.9337 | 531.0 | 468.5 | |
| 0.00 | 2.49 | 0.00 | 3.48 | 13.98 | 346.52 | -70.31 | 77.73 | 0.9365 | 427.0 | 362.8 | |
| 0.00 | 1.69 | 0.00 | 2.39 | 14.38 | 346.23 | -70.60 | 77.29 | 0.9381 | 303.0 | 289.5 | |
| 0.00 | 2.94 | 0.00 | 4.26 | 14.94 | 345.62 | -71.21 | 76.68 | 0.9415 | 95.0 | 96.2 | |
| 0.00 | 3.92 | 0.00 | 6.13 | 14.38 | 344.12 | -72.71 | 77.19 | 0.9499 | 328.0 | 250.0 | |
| 1.33 | 3.92 | 2.15 | 6.33 | 14.19 | 343.53 | -73.30 | 77.36 | 0.9530 | 207.6 | 121.4 | |
| 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. | |