SDO HMI 2014-09-22 02:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.44 | 15.25 | 0.23 | 8.89 | -17.83 | 283.67 | -18.73 | 144.60 | 0.5184 | 680.3 | 526.2 | |
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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 |
| 0.44 | 1.42 | 0.23 | 0.73 | -9.47 | 299.45 | -2.95 | 169.88 | 0.2903 | 921.6 | 769.5 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -13.79 | 291.08 | -11.32 | 151.69 | 0.4035 | 731.0 | 594.7 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -13.41 | 290.85 | -11.55 | 150.72 | 0.4000 | 623.0 | 449.3 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -8.99 | 285.79 | -16.61 | 133.89 | 0.3935 | 705.0 | 562.3 | |
| 0.00 | 1.51 | 0.00 | 0.89 | -19.32 | 282.71 | -19.69 | 144.01 | 0.5431 | 572.0 | 473.5 | |
| 0.00 | 1.42 | 0.00 | 0.85 | -21.51 | 282.17 | -20.23 | 145.69 | 0.5729 | 720.0 | 522.3 | |
| 0.00 | 1.68 | 0.00 | 1.04 | -23.36 | 281.18 | -21.22 | 146.33 | 0.6016 | 600.0 | 489.9 | |
| 0.00 | 1.33 | 0.00 | 0.83 | -23.90 | 280.10 | -22.30 | 145.57 | 0.6159 | 583.0 | 508.8 | |
| 0.00 | 1.86 | 0.00 | 1.17 | -24.05 | 279.86 | -22.55 | 145.44 | 0.6195 | 560.0 | 497.3 | |
| 0.00 | 0.89 | 0.00 | 0.50 | -11.71 | 280.95 | -21.45 | 131.21 | 0.4780 | 692.0 | 594.0 | |
| 0.00 | 1.24 | 0.00 | 0.74 | -18.26 | 279.65 | -22.75 | 138.75 | 0.5592 | 660.0 | 468.6 | |
| 0.00 | 1.24 | 0.00 | 0.70 | -10.08 | 279.32 | -23.08 | 126.47 | 0.4819 | 740.0 | 528.9 | |
| 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. | |