SDO HMI 2014-11-22 22:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.13 | 0.00 | 14.12 | -12.32 | 225.50 | 18.63 | 231.60 | 0.3986 | -99.6 | -213.0 | |
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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 | 0.94 | 0.00 | 0.53 | -10.48 | 232.08 | 25.22 | 243.18 | 0.4714 | -595.0 | -495.0 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -13.48 | 229.12 | 22.25 | 234.42 | 0.4546 | 619.0 | 458.4 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -11.61 | 228.59 | 21.72 | 237.40 | 0.4322 | 555.0 | 384.1 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -13.04 | 228.52 | 21.65 | 234.53 | 0.4432 | 545.0 | 464.9 | |
| 0.00 | 2.31 | 0.00 | 1.27 | -12.86 | 228.21 | 21.34 | 234.50 | 0.4376 | 948.0 | 766.0 | |
| 0.00 | 1.46 | 0.00 | 0.80 | -12.67 | 228.13 | 21.26 | 234.76 | 0.4350 | 826.0 | 747.9 | |
| 0.00 | 1.37 | 0.00 | 0.76 | -13.56 | 228.04 | 21.18 | 232.97 | 0.4417 | 802.0 | 703.4 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -13.55 | 227.81 | 20.95 | 232.68 | 0.4389 | 794.0 | 587.4 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -12.98 | 223.78 | 16.91 | 227.91 | 0.3836 | -742.0 | -580.5 | |
| 0.00 | 5.66 | 0.00 | 3.01 | -11.64 | 223.44 | 16.57 | 230.13 | 0.3655 | -827.0 | -747.3 | |
| 0.00 | 1.11 | 0.00 | 0.60 | -13.96 | 223.53 | 16.66 | 225.59 | 0.3912 | -792.0 | -629.1 | |
| 0.00 | 1.97 | 0.00 | 1.05 | -11.42 | 223.27 | 16.40 | 230.31 | 0.3612 | -880.0 | -758.6 | |
| 0.00 | 1.71 | 0.00 | 0.91 | -12.73 | 223.13 | 16.26 | 227.32 | 0.3732 | -861.0 | -713.9 | |
| 0.00 | 3.09 | 0.00 | 1.64 | -12.18 | 223.03 | 16.16 | 228.28 | 0.3661 | -958.0 | -729.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -10.75 | 222.95 | 16.08 | 231.26 | 0.3504 | -928.0 | -677.8 | |
| 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. | |