SDO HMI 2014-09-26 11:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.39 | 0.00 | 12.20 | 8.77 | 285.76 | 41.08 | 274.57 | 0.6492 | -135.0 | -180.0 | |
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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 | 1.59 | 0.00 | 1.18 | 5.17 | 293.10 | 48.42 | 270.77 | 0.7474 | -623.0 | -568.3 | |
| 0.00 | 1.15 | 0.00 | 0.85 | 5.25 | 292.92 | 48.25 | 270.85 | 0.7453 | -634.0 | -532.5 | |
| 0.00 | 1.77 | 0.00 | 1.25 | 13.12 | 290.35 | 45.68 | 281.63 | 0.7137 | -653.0 | -542.4 | |
| 0.00 | 2.92 | 0.00 | 2.00 | 10.89 | 288.96 | 44.28 | 278.54 | 0.6956 | -773.0 | -648.2 | |
| 0.00 | 3.00 | 0.00 | 2.05 | 6.83 | 288.34 | 43.66 | 272.64 | 0.6885 | 666.0 | 521.0 | |
| 0.00 | 0.71 | 0.00 | 0.49 | 12.72 | 289.29 | 44.62 | 281.15 | 0.7006 | -603.0 | -533.0 | |
| 0.00 | 1.15 | 0.00 | 0.78 | 11.65 | 288.21 | 43.53 | 279.68 | 0.6866 | -694.0 | -560.2 | |
| 0.00 | 1.68 | 0.00 | 1.13 | 11.96 | 287.72 | 43.04 | 280.17 | 0.6807 | -851.0 | -673.8 | |
| 0.00 | 0.88 | 0.00 | 0.55 | 4.39 | 282.14 | 37.46 | 268.18 | 0.6090 | 344.0 | 419.3 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 10.70 | 278.70 | 34.02 | 278.92 | 0.5587 | 600.0 | 467.8 | |
| 0.00 | 1.24 | 0.00 | 0.66 | 7.16 | 266.54 | 21.87 | 272.03 | 0.3714 | 825.0 | 585.9 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 2.52 | 255.76 | 11.08 | 248.85 | 0.2069 | 776.0 | 614.1 | |
| 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. | |