SDO HMI 2014-11-08 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.60 | 18.47 | 0.34 | 10.56 | -14.39 | 18.60 | -23.80 | 127.90 | 0.4968 | -55.2 | -330.3 | |
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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 | 1.04 | 0.00 | 0.55 | -12.15 | 27.54 | -14.87 | 137.15 | 0.3705 | 808.0 | 676.2 | |
| 0.00 | 1.55 | 0.00 | 0.82 | -5.31 | 24.06 | -18.35 | 115.97 | 0.3502 | -14.0 | 1.2 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -13.76 | 21.42 | -20.99 | 130.32 | 0.4582 | 846.0 | 709.5 | |
| 0.60 | 1.64 | 0.34 | 0.92 | -13.74 | 20.70 | -21.71 | 129.36 | 0.4666 | 823.6 | 617.9 | |
| 0.00 | 4.06 | 0.00 | 2.28 | -13.91 | 20.19 | -22.22 | 129.00 | 0.4743 | -836.0 | -524.5 | |
| 0.00 | 1.04 | 0.00 | 0.58 | -14.57 | 20.05 | -22.36 | 129.93 | 0.4821 | 524.0 | 381.8 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -16.97 | 16.07 | -26.33 | 129.20 | 0.5496 | -700.0 | -493.5 | |
| 0.00 | 4.57 | 0.00 | 2.70 | -16.21 | 15.94 | -26.46 | 127.94 | 0.5447 | -643.0 | -771.7 | |
| 0.00 | 1.55 | 0.00 | 0.92 | -16.51 | 15.52 | -26.89 | 127.96 | 0.5521 | -612.0 | -574.6 | |
| 0.00 | 0.60 | 0.00 | 0.36 | -17.73 | 14.90 | -27.50 | 129.14 | 0.5693 | -551.0 | -482.0 | |
| 0.00 | 0.95 | 0.00 | 0.58 | -15.92 | 12.01 | -30.40 | 123.89 | 0.5883 | -552.0 | -481.7 | |
| 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. | |