SDO HMI 2014-11-30 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.23 | 437.21 | 36.61 | 224.91 | 16.58 | 110.31 | -0.45 | 1.51 | 0.2704 | -1076.3 | -375.6 | |
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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 |
| 70.03 | 422.50 | 36.00 | 217.28 | 16.52 | 110.54 | -0.22 | 0.80 | 0.2688 | -1607.6 | -421.3 | |
| 0.94 | -1.00 | 0.48 | -1.00 | 16.99 | 110.02 | -0.75 | 2.60 | 0.2769 | -943.8 | 999999 | |
| 0.26 | -1.00 | 0.13 | -1.00 | 16.52 | 109.77 | -0.99 | 3.55 | 0.2693 | -1203.3 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 17.82 | 107.93 | -2.83 | 9.23 | 0.2944 | 947.0 | 810.8 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 17.60 | 106.63 | -4.13 | 13.52 | 0.2952 | 827.0 | 686.5 | |
| 0.00 | 4.28 | 0.00 | 2.21 | 17.54 | 106.48 | -4.29 | 14.06 | 0.2948 | 927.0 | 765.3 | |
| 0.00 | 1.88 | 0.00 | 0.97 | 16.46 | 104.86 | -5.90 | 20.30 | 0.2856 | 1002.0 | 795.2 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 18.81 | 104.72 | -6.04 | 18.04 | 0.3232 | 876.0 | 719.4 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 17.45 | 104.49 | -6.28 | 20.22 | 0.3032 | 754.0 | 615.7 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 18.97 | 103.52 | -7.24 | 21.13 | 0.3322 | 787.0 | 662.7 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.42 | 102.63 | -8.13 | 28.69 | 0.2853 | 665.0 | 441.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 18.50 | 102.22 | -8.55 | 25.10 | 0.3337 | 786.0 | 636.7 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 22.19 | 98.37 | -12.39 | 28.77 | 0.4146 | 741.0 | 627.8 | |
| 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. | |