SDO HMI 2014-09-22 01:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.27 | 0.00 | 10.60 | 13.88 | 351.21 | 48.26 | 282.67 | 0.7409 | 19.3 | -66.2 | |
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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 | 0.80 | 0.00 | 0.67 | 11.68 | 357.54 | 54.59 | 279.33 | 0.8110 | -371.0 | -328.2 | |
| 0.00 | 0.62 | 0.00 | 0.52 | 11.38 | 357.19 | 54.24 | 278.95 | 0.8075 | -376.0 | -440.3 | |
| 0.00 | 1.68 | 0.00 | 1.39 | 11.91 | 356.81 | 53.86 | 279.60 | 0.8037 | -216.0 | -299.5 | |
| 0.00 | 0.80 | 0.00 | 0.65 | 13.97 | 355.84 | 52.89 | 282.20 | 0.7940 | -347.0 | -247.7 | |
| 0.00 | 1.95 | 0.00 | 1.56 | 13.92 | 355.36 | 52.41 | 282.17 | 0.7891 | -562.0 | -445.6 | |
| 0.00 | 0.44 | 0.00 | 0.35 | 14.97 | 354.70 | 51.75 | 283.54 | 0.7826 | -304.0 | -346.0 | |
| 0.00 | 2.39 | 0.00 | 1.80 | 13.85 | 352.23 | 49.28 | 282.23 | 0.7553 | -501.0 | -456.7 | |
| 0.00 | 0.89 | 0.00 | 0.64 | 12.99 | 349.90 | 46.95 | 281.21 | 0.7282 | 334.0 | 299.1 | |
| 0.00 | 0.89 | 0.00 | 0.59 | 15.71 | 344.57 | 41.62 | 285.73 | 0.6666 | 630.0 | 523.3 | |
| 0.00 | 2.48 | 0.00 | 1.61 | 16.11 | 342.97 | 40.02 | 286.65 | 0.6471 | 766.0 | 662.0 | |
| 0.00 | 0.89 | 0.00 | 0.56 | 13.37 | 341.17 | 38.22 | 282.68 | 0.6192 | 617.0 | 487.3 | |
| 0.00 | 0.44 | 0.00 | 0.26 | 18.52 | 335.60 | 32.65 | 292.98 | 0.5578 | 562.0 | 497.8 | |
| 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. | |