SDO HMI 2014-11-04 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.11 | 38.87 | 6.24 | 20.36 | 5.57 | 71.08 | -18.60 | 84.20 | 0.3198 | -142.5 | -13.1 | |
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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 |
| 3.98 | 20.74 | 2.05 | 10.68 | 5.80 | 74.01 | -15.67 | 82.89 | 0.2720 | -1259.4 | -740.3 | |
| 4.93 | -1.00 | 2.54 | -1.00 | 5.95 | 73.88 | -15.80 | 82.41 | 0.2744 | -1004.1 | 999999 | |
| 3.20 | -1.00 | 1.65 | -1.00 | 5.71 | 73.86 | -15.82 | 83.28 | 0.2744 | -1132.9 | 999999 | |
| 0.00 | 3.28 | 0.00 | 1.69 | 5.20 | 73.56 | -16.12 | 85.22 | 0.2787 | -703.0 | -683.1 | |
| 0.00 | 2.07 | 0.00 | 1.07 | 5.76 | 73.52 | -16.16 | 83.21 | 0.2802 | -646.0 | -549.5 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 5.71 | 67.02 | -22.66 | 84.83 | 0.3866 | 859.0 | 692.2 | |
| 0.00 | 3.02 | 0.00 | 1.63 | 4.71 | 66.18 | -23.50 | 87.47 | 0.3995 | 830.0 | 781.4 | |
| 0.00 | 3.89 | 0.00 | 2.10 | 4.58 | 66.02 | -23.66 | 87.78 | 0.4021 | 752.0 | 771.3 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 4.75 | 65.69 | -23.99 | 87.37 | 0.4074 | 686.0 | 532.5 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 4.89 | 65.45 | -24.23 | 87.03 | 0.4112 | 603.0 | 483.9 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 6.60 | 64.89 | -24.80 | 82.98 | 0.4216 | 653.0 | 574.1 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 6.21 | 64.54 | -25.14 | 83.97 | 0.4265 | 905.0 | 708.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 6.23 | 64.34 | -25.34 | 83.95 | 0.4296 | 749.0 | 618.5 | |
| 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. | |