SDO HMI 2014-11-05 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.55 | 35.15 | 5.24 | 17.63 | 5.94 | 70.09 | -7.50 | 68.99 | 0.1376 | -43.7 | 202.5 | |
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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 | 0.95 | 0.00 | 0.47 | 9.26 | 75.60 | -1.99 | 20.23 | 0.0994 | -678.0 | -551.5 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 6.07 | 74.60 | -2.99 | 54.25 | 0.0643 | -166.0 | -220.5 | |
| 3.46 | 14.34 | 1.72 | 7.12 | 5.83 | 74.57 | -3.02 | 57.64 | 0.0624 | -1227.3 | -825.3 | |
| 7.09 | -3.00 | 3.52 | -3.00 | 5.74 | 74.42 | -3.17 | 60.08 | 0.0638 | -1150.5 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.43 | 5.37 | 70.77 | -6.82 | 77.83 | 0.1216 | -919.0 | -774.7 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 6.27 | 68.67 | -8.92 | 74.88 | 0.1603 | -1004.0 | -795.2 | |
| 0.00 | 1.90 | 0.00 | 0.96 | 5.47 | 66.32 | -11.27 | 81.75 | 0.1975 | 904.0 | 684.6 | |
| 0.00 | 1.21 | 0.00 | 0.61 | 5.27 | 66.29 | -11.30 | 82.82 | 0.1975 | 1047.0 | 839.1 | |
| 0.00 | 1.38 | 0.00 | 0.70 | 4.58 | 66.09 | -11.50 | 86.36 | 0.2000 | 977.0 | 701.9 | |
| 0.00 | 4.93 | 0.00 | 2.49 | 6.51 | 65.78 | -11.81 | 77.15 | 0.2095 | 927.0 | 667.4 | |
| 0.00 | 2.07 | 0.00 | 1.05 | 6.21 | 65.79 | -11.80 | 78.55 | 0.2084 | 968.0 | 637.9 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 5.05 | 65.81 | -11.78 | 84.12 | 0.2054 | 940.0 | 746.0 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 6.62 | 65.35 | -12.24 | 77.04 | 0.2171 | 691.0 | 526.3 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 5.82 | 65.15 | -12.44 | 80.86 | 0.2180 | 869.0 | 607.5 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 5.55 | 64.94 | -12.64 | 82.21 | 0.2209 | 807.0 | 636.8 | |
| 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. | |