SDO HMI 2014-11-09 14:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.32 | 0.00 | 11.82 | -15.81 | 18.83 | -3.83 | 171.06 | 0.3455 | -241.6 | -44.5 | |
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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 | 2.15 | 0.00 | 1.11 | -11.34 | 28.34 | 5.68 | 200.79 | 0.2748 | 904.0 | 744.0 | |
| 0.00 | 3.53 | 0.00 | 1.83 | -13.08 | 23.16 | 0.50 | 181.70 | 0.2865 | 1224.0 | 973.6 | |
| 0.00 | 2.15 | 0.00 | 1.12 | -13.42 | 22.76 | 0.10 | 180.34 | 0.2921 | 941.0 | 675.2 | |
| 0.00 | 1.98 | 0.00 | 1.03 | -14.16 | 22.12 | -0.54 | 178.27 | 0.3047 | 871.0 | 747.0 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -15.84 | 16.51 | -6.14 | 162.70 | 0.3478 | -868.0 | -661.5 | |
| 0.00 | 3.71 | 0.00 | 2.00 | -18.54 | 15.32 | -7.34 | 162.08 | 0.3955 | -1019.0 | -853.0 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -18.74 | 14.99 | -7.67 | 161.51 | 0.4000 | -909.0 | -780.6 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -18.96 | 14.98 | -7.68 | 161.67 | 0.4035 | -743.0 | -626.6 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -19.16 | 14.94 | -7.72 | 161.74 | 0.4066 | -551.0 | -390.3 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -18.96 | 14.76 | -7.90 | 161.18 | 0.4047 | -685.0 | -568.3 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -18.71 | 14.42 | -8.24 | 160.22 | 0.4026 | -816.0 | -681.1 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -17.66 | 14.35 | -8.31 | 159.07 | 0.3872 | -813.0 | -657.4 | |
| 0.00 | 1.64 | 0.00 | 0.87 | -15.48 | 13.60 | -9.05 | 154.94 | 0.3596 | -677.0 | -541.7 | |
| 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. | |