SDO HMI 2014-11-08 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.60 | 23.64 | 0.35 | 13.47 | 5.37 | 71.80 | 29.40 | 274.54 | 0.4912 | -74.7 | -143.7 | |
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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 | 4.92 | 0.00 | 2.91 | 5.54 | 75.75 | 33.34 | 274.53 | 0.5509 | -753.0 | -692.5 | |
| 0.60 | 3.19 | 0.35 | 1.87 | 5.31 | 74.88 | 32.47 | 274.14 | 0.5381 | -891.0 | -688.3 | |
| 0.00 | 0.78 | 0.00 | 0.45 | 4.43 | 74.48 | 32.07 | 272.50 | 0.5320 | -691.0 | -578.0 | |
| 0.00 | 1.12 | 0.00 | 0.65 | 4.15 | 73.87 | 31.46 | 271.97 | 0.5229 | -654.0 | -443.5 | |
| 0.00 | 2.07 | 0.00 | 1.20 | 5.09 | 73.49 | 31.09 | 273.78 | 0.5175 | -1015.0 | -830.6 | |
| 0.00 | 1.12 | 0.00 | 0.65 | 5.01 | 73.25 | 30.84 | 273.64 | 0.5138 | -778.0 | -717.5 | |
| 0.00 | 2.16 | 0.00 | 1.22 | 5.86 | 71.57 | 29.16 | 275.48 | 0.4890 | 854.0 | 653.1 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 4.45 | 71.15 | 28.75 | 272.58 | 0.4820 | -580.0 | -554.6 | |
| 0.00 | 1.55 | 0.00 | 0.85 | 5.63 | 67.33 | 24.92 | 275.49 | 0.4231 | 775.0 | 582.2 | |
| 0.00 | 0.52 | 0.00 | 0.28 | 5.53 | 66.83 | 24.42 | 275.31 | 0.4151 | 660.0 | 578.3 | |
| 0.00 | 3.11 | 0.00 | 1.69 | 5.75 | 66.54 | 24.14 | 275.88 | 0.4108 | 774.0 | 612.9 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 6.28 | 66.47 | 24.07 | 277.20 | 0.4103 | 859.0 | 742.2 | |
| 0.00 | 1.29 | 0.00 | 0.70 | 4.74 | 65.17 | 22.76 | 273.53 | 0.3880 | 754.0 | 578.9 | |
| 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. | |