SDO HMI 2014-11-15 13:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.88 | 75.73 | 40.96 | 118.54 | 13.87 | 15.69 | 71.58 | 283.71 | 0.9490 | -301.3 | -28.0 | |
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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 |
| 5.50 | 21.23 | 9.26 | 36.03 | 13.27 | 17.18 | 73.08 | 283.03 | 0.9571 | -229.7 | 7.5 | |
| 0.00 | 1.12 | 0.00 | 1.74 | 12.82 | 15.72 | 71.62 | 282.59 | 0.9495 | -441.0 | -384.8 | |
| 0.00 | 0.26 | 0.00 | 0.40 | 12.50 | 15.41 | 71.30 | 282.26 | 0.9478 | -313.0 | -330.3 | |
| 1.38 | 33.18 | 2.19 | 52.36 | 13.93 | 16.05 | 71.94 | 283.75 | 0.9514 | 119.8 | 52.2 | |
| 5.67 | 10.14 | 8.74 | 15.59 | 13.35 | 15.51 | 71.41 | 283.15 | 0.9485 | -502.8 | -398.0 | |
| 12.90 | -4.00 | 20.23 | -4.00 | 14.25 | 15.80 | 71.69 | 284.09 | 0.9501 | -367.8 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.64 | 14.14 | 14.85 | 70.74 | 284.01 | 0.9450 | -306.0 | -334.2 | |
| 0.00 | 0.26 | 0.00 | 0.38 | 14.87 | 14.27 | 70.17 | 284.81 | 0.9419 | -382.0 | -343.0 | |
| 0.00 | 1.63 | 0.00 | 2.35 | 15.22 | 13.99 | 69.89 | 285.19 | 0.9404 | -476.0 | -338.1 | |
| 0.43 | 1.29 | 0.54 | 1.61 | 14.18 | 10.69 | 66.59 | 284.24 | 0.9196 | 219.6 | 187.1 | |
| 0.00 | 2.32 | 0.00 | 2.84 | 13.98 | 10.20 | 66.09 | 284.06 | 0.9162 | 460.0 | 410.1 | |
| 0.00 | 1.12 | 0.00 | 1.42 | 15.82 | 11.02 | 66.92 | 286.00 | 0.9225 | -460.0 | -385.2 | |
| 0.00 | 0.95 | 0.00 | 1.17 | 15.53 | 10.45 | 66.34 | 285.73 | 0.9185 | -340.0 | -366.7 | |
| 0.00 | 0.77 | 0.00 | 0.90 | 13.95 | 8.84 | 64.74 | 284.11 | 0.9068 | 312.0 | 231.0 | |
| 0.00 | 1.03 | 0.00 | 1.11 | 18.04 | 6.07 | 61.96 | 288.91 | 0.8890 | 172.0 | 114.3 | |
| 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. | |