SDO HMI 2014-09-06 02:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.83 | 0.00 | 11.12 | 9.61 | 180.19 | 26.54 | 278.61 | 0.4444 | -176.3 | -39.8 | |
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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 | 2.05 | 0.00 | 1.24 | 7.03 | 188.54 | 34.89 | 271.88 | 0.5701 | -616.0 | -524.7 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 10.94 | 188.75 | 35.10 | 278.73 | 0.5734 | -633.0 | -552.5 | |
| 0.00 | 0.54 | 0.00 | 0.32 | 11.43 | 188.63 | 34.98 | 279.61 | 0.5721 | -562.0 | -424.2 | |
| 0.00 | 1.34 | 0.00 | 0.79 | 6.64 | 187.25 | 33.60 | 271.07 | 0.5519 | -681.0 | -460.3 | |
| 0.00 | 2.50 | 0.00 | 1.50 | 12.71 | 187.84 | 34.19 | 281.98 | 0.5626 | -676.0 | -543.1 | |
| 0.00 | 0.98 | 0.00 | 0.58 | 10.96 | 187.15 | 33.50 | 278.93 | 0.5506 | -732.0 | -653.3 | |
| 0.00 | 1.25 | 0.00 | 0.74 | 11.57 | 187.08 | 33.43 | 280.06 | 0.5503 | -681.0 | -581.2 | |
| 0.00 | 1.61 | 0.00 | 0.94 | 5.30 | 185.60 | 31.95 | 268.36 | 0.5292 | -618.0 | -461.0 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 11.47 | 173.83 | 20.17 | 283.50 | 0.3491 | 732.0 | 573.0 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 9.82 | 172.80 | 19.15 | 279.08 | 0.3287 | 656.0 | 513.7 | |
| 0.00 | 1.34 | 0.00 | 0.69 | 2.48 | 169.22 | 15.57 | 253.67 | 0.2807 | 786.0 | 742.5 | |
| 0.00 | 3.66 | 0.00 | 1.85 | 11.97 | 164.59 | 10.93 | 294.48 | 0.2048 | 909.0 | 839.9 | |
| 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. | |