SDO HMI 2014-10-06 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.33 | 0.00 | 12.04 | 13.63 | 59.72 | -48.04 | 77.39 | 0.7426 | -149.3 | -208.4 | |
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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 | 1.14 | 0.00 | 0.80 | 14.10 | 62.85 | -44.92 | 76.44 | 0.7068 | -737.0 | -584.1 | |
| 0.00 | 1.49 | 0.00 | 1.08 | 15.08 | 60.84 | -46.92 | 75.33 | 0.7314 | -570.0 | -445.8 | |
| 0.00 | 1.14 | 0.00 | 0.82 | 12.66 | 61.07 | -46.69 | 78.63 | 0.7266 | -347.0 | -301.7 | |
| 0.00 | 1.32 | 0.00 | 0.95 | 13.75 | 60.62 | -47.15 | 77.18 | 0.7327 | -433.0 | -386.8 | |
| 0.00 | 1.49 | 0.00 | 1.08 | 13.31 | 60.50 | -47.26 | 77.78 | 0.7336 | -350.0 | -424.3 | |
| 0.00 | 1.40 | 0.00 | 1.03 | 14.47 | 60.10 | -47.67 | 76.25 | 0.7392 | -655.0 | -534.7 | |
| 0.00 | 1.32 | 0.00 | 0.97 | 14.96 | 59.77 | -47.99 | 75.62 | 0.7434 | -523.0 | -415.2 | |
| 0.00 | 1.58 | 0.00 | 1.16 | 13.61 | 60.06 | -47.71 | 77.41 | 0.7390 | -479.0 | -432.5 | |
| 0.00 | 0.97 | 0.00 | 0.71 | 13.21 | 60.07 | -47.70 | 77.95 | 0.7386 | -535.0 | -409.8 | |
| 0.00 | 0.70 | 0.00 | 0.52 | 13.41 | 59.88 | -47.89 | 77.69 | 0.7409 | -280.0 | -219.1 | |
| 0.00 | 0.79 | 0.00 | 0.60 | 12.74 | 58.32 | -49.44 | 78.70 | 0.7580 | 553.0 | 444.7 | |
| 0.00 | 0.53 | 0.00 | 0.40 | 11.88 | 57.88 | -49.89 | 79.86 | 0.7626 | 595.0 | 576.5 | |
| 0.00 | 1.23 | 0.00 | 0.95 | 12.40 | 57.21 | -50.55 | 79.20 | 0.7701 | 580.0 | 489.8 | |
| 0.00 | 0.70 | 0.00 | 0.55 | 13.41 | 56.19 | -51.57 | 77.95 | 0.7815 | 458.0 | 413.0 | |
| 0.00 | 0.53 | 0.00 | 0.42 | 13.39 | 55.55 | -52.22 | 78.01 | 0.7883 | 484.0 | 424.5 | |
| 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. | |