SDO HMI 2014-11-10 11:00:27 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 | -24.00 | 7.67 | -3.45 | 173.97 | 0.4681 | 543.1 | 483.6 | |
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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 | 1.90 | 0.00 | 1.03 | -20.60 | 10.20 | -0.92 | 177.89 | 0.4084 | 871.0 | 643.1 | |
| 0.00 | 1.81 | 0.00 | 0.99 | -21.48 | 10.13 | -0.99 | 177.81 | 0.4225 | 913.0 | 737.9 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -22.60 | 10.09 | -1.03 | 177.83 | 0.4402 | 608.0 | 581.8 | |
| 0.00 | 2.59 | 0.00 | 1.42 | -22.60 | 9.80 | -1.32 | 177.22 | 0.4404 | 624.0 | 582.2 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -23.36 | 9.37 | -1.75 | 176.44 | 0.4527 | 157.0 | 339.4 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -23.66 | 9.23 | -1.88 | 176.21 | 0.4575 | 830.0 | 686.6 | |
| 0.00 | 1.90 | 0.00 | 1.06 | -24.40 | 9.13 | -1.99 | 176.11 | 0.4691 | 785.0 | 647.1 | |
| 0.00 | 3.36 | 0.00 | 1.89 | -24.70 | 8.99 | -2.13 | 175.90 | 0.4739 | 819.0 | 644.1 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -24.94 | 8.99 | -2.13 | 175.93 | 0.4775 | 458.0 | 471.2 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -24.06 | 8.61 | -2.51 | 175.05 | 0.4645 | 925.0 | 643.2 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -24.03 | 8.38 | -2.73 | 174.59 | 0.4643 | 919.0 | 774.4 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -26.62 | 357.40 | -13.72 | 156.96 | 0.5439 | -333.0 | -430.1 | |
| 0.00 | 1.64 | 0.00 | 1.01 | -29.58 | 355.26 | -15.85 | 156.34 | 0.5942 | -516.0 | -499.6 | |
| 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. | |