SDO HMI 2014-11-07 14:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.16 | 16.14 | 1.19 | 8.70 | 5.68 | 71.95 | 22.93 | 276.07 | 0.3909 | -184.7 | -172.5 | |
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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 |
| 1.64 | 2.76 | 0.91 | 1.53 | 5.65 | 75.64 | 26.61 | 275.22 | 0.4494 | -924.3 | -810.8 | |
| 0.00 | 1.29 | 0.00 | 0.72 | 5.54 | 75.50 | 26.47 | 274.98 | 0.4472 | -928.0 | -745.8 | |
| 0.52 | 2.42 | 0.28 | 1.33 | 5.35 | 74.85 | 25.83 | 274.62 | 0.4370 | -959.7 | -791.4 | |
| 0.00 | 0.78 | 0.00 | 0.43 | 4.07 | 74.80 | 25.77 | 271.69 | 0.4358 | -566.0 | -430.0 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 5.43 | 73.05 | 24.02 | 275.02 | 0.4085 | -675.0 | -600.1 | |
| 0.00 | 1.64 | 0.00 | 0.88 | 6.02 | 72.10 | 23.07 | 276.66 | 0.3940 | -894.0 | -616.3 | |
| 0.00 | 0.26 | 0.00 | 0.14 | 4.36 | 69.46 | 20.44 | 272.54 | 0.3500 | 20.0 | 18.7 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 4.60 | 69.47 | 20.44 | 273.22 | 0.3502 | 18.0 | 26.2 | |
| 0.00 | 0.78 | 0.00 | 0.41 | 6.60 | 69.29 | 20.26 | 278.98 | 0.3498 | -21.0 | -32.7 | |
| 0.00 | 0.26 | 0.00 | 0.14 | 9.14 | 68.82 | 19.79 | 286.41 | 0.3500 | -8.0 | -12.0 | |
| 0.00 | 1.38 | 0.00 | 0.72 | 5.87 | 67.17 | 18.15 | 277.52 | 0.3139 | 772.0 | 715.2 | |
| 0.00 | 1.38 | 0.00 | 0.72 | 6.21 | 66.53 | 17.50 | 278.87 | 0.3039 | 1023.0 | 888.8 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 6.57 | 66.32 | 17.29 | 280.15 | 0.3013 | 892.0 | 774.5 | |
| 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. | |