SDO HMI 2014-11-04 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.42 | 0.00 | 9.12 | -21.35 | 77.86 | -7.41 | 165.06 | 0.4494 | 672.7 | 564.3 | |
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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 | 0.60 | 0.00 | 0.32 | -17.14 | 82.45 | -2.82 | 172.57 | 0.3656 | 615.0 | 524.3 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -21.92 | 81.27 | -4.00 | 171.57 | 0.4438 | 743.0 | 480.3 | |
| 0.00 | 1.73 | 0.00 | 0.95 | -20.96 | 80.75 | -4.52 | 170.11 | 0.4303 | 746.0 | 625.4 | |
| 0.00 | 2.59 | 0.00 | 1.42 | -20.54 | 80.64 | -4.63 | 169.68 | 0.4240 | 933.0 | 678.0 | |
| 0.00 | 1.73 | 0.00 | 0.95 | -20.87 | 80.50 | -4.77 | 169.53 | 0.4295 | 710.0 | 627.0 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -20.02 | 79.64 | -5.63 | 167.23 | 0.4192 | 850.0 | 743.8 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -22.54 | 77.14 | -8.13 | 163.69 | 0.4671 | 787.0 | 630.0 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -20.50 | 77.03 | -8.24 | 162.04 | 0.4373 | 850.0 | 729.1 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -20.57 | 76.51 | -8.76 | 161.05 | 0.4410 | 821.0 | 640.8 | |
| 0.00 | 1.38 | 0.00 | 0.76 | -20.37 | 76.30 | -8.97 | 160.47 | 0.4392 | 938.0 | 774.0 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -26.39 | 70.33 | -14.94 | 155.39 | 0.5566 | 712.0 | 655.4 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -24.11 | 65.19 | -20.08 | 146.17 | 0.5651 | -633.0 | -543.8 | |
| 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. | |