SDO HMI 2014-11-07 09:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.43 | 12.35 | 0.23 | 6.66 | -12.04 | 35.35 | -16.42 | 133.91 | 0.3899 | -58.1 | 81.5 | |
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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 |
| 0.43 | 2.24 | 0.23 | 1.20 | -13.01 | 37.43 | -14.33 | 139.86 | 0.3757 | 1047.2 | 879.1 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -11.76 | 36.66 | -15.11 | 136.06 | 0.3693 | -899.0 | -744.1 | |
| 0.00 | 1.73 | 0.00 | 0.94 | -14.74 | 36.43 | -15.33 | 140.89 | 0.4071 | 840.0 | 669.0 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -12.84 | 36.50 | -15.27 | 137.77 | 0.3836 | 783.0 | 719.9 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -10.04 | 36.66 | -15.11 | 132.56 | 0.3500 | -5.0 | -0.5 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -13.18 | 35.11 | -16.65 | 135.91 | 0.4027 | -818.0 | -618.3 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -7.19 | 34.47 | -17.29 | 122.29 | 0.3504 | 9.0 | 4.2 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -5.19 | 33.38 | -18.38 | 115.76 | 0.3503 | -7.0 | -3.8 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -14.72 | 32.64 | -19.13 | 134.63 | 0.4473 | -662.0 | -497.9 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -15.11 | 32.17 | -19.59 | 134.59 | 0.4565 | -735.0 | -635.9 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -15.42 | 32.08 | -19.69 | 134.96 | 0.4609 | -446.0 | -607.2 | |
| 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. | |