SDO HMI 2014-11-09 11:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.29 | 25.76 | 0.67 | 13.63 | -15.63 | 19.13 | -5.17 | 167.14 | 0.3450 | -64.4 | -172.3 | |
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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 | 1.12 | 0.00 | 0.58 | -11.51 | 28.29 | 3.99 | 194.76 | 0.2688 | 886.0 | 800.8 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -9.06 | 27.21 | 2.91 | 192.98 | 0.2240 | 823.0 | 603.2 | |
| 0.95 | 4.57 | 0.49 | 2.36 | -13.07 | 23.07 | -1.23 | 175.79 | 0.2871 | 1157.3 | 879.9 | |
| 0.34 | 1.81 | 0.18 | 0.94 | -13.41 | 22.73 | -1.57 | 174.76 | 0.2933 | 847.5 | 716.5 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -14.19 | 21.96 | -2.34 | 172.56 | 0.3077 | 791.0 | 647.2 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -14.28 | 21.77 | -2.53 | 172.02 | 0.3096 | 486.0 | 239.0 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -14.63 | 21.12 | -3.18 | 170.21 | 0.3170 | -656.0 | -538.4 | |
| 0.00 | 1.64 | 0.00 | 0.86 | -14.82 | 19.74 | -4.57 | 166.23 | 0.3248 | -966.0 | -832.2 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -17.46 | 16.51 | -7.79 | 160.08 | 0.3814 | -672.0 | -574.2 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -15.84 | 16.51 | -7.79 | 158.48 | 0.3569 | -913.0 | -680.1 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -16.13 | 16.41 | -7.89 | 158.52 | 0.3619 | -831.0 | -722.8 | |
| 0.00 | 5.00 | 0.00 | 2.71 | -18.55 | 15.35 | -8.95 | 158.50 | 0.4044 | -539.0 | -777.4 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -18.56 | 14.78 | -9.52 | 157.28 | 0.4079 | -546.0 | -460.2 | |
| 0.00 | 2.67 | 0.00 | 1.45 | -18.82 | 14.41 | -9.89 | 156.77 | 0.4140 | -818.0 | -690.1 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -17.60 | 14.20 | -10.10 | 155.03 | 0.3978 | -778.0 | -512.6 | |
| 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. | |