SDO HMI 2014-11-28 22:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.32 | 27.53 | 5.33 | 15.61 | 17.22 | 152.40 | 24.61 | 305.00 | 0.4874 | 239.4 | 11.3 | |
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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 | 1.71 | 0.00 | 0.99 | 17.95 | 154.19 | 26.41 | 304.47 | 0.5153 | 739.0 | 472.8 | |
| 7.18 | 9.75 | 4.13 | 5.61 | 17.64 | 154.04 | 26.25 | 304.09 | 0.5111 | 983.3 | 654.4 | |
| 0.77 | 1.80 | 0.43 | 1.01 | 15.63 | 152.28 | 24.49 | 302.18 | 0.4737 | 663.2 | 584.8 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 15.45 | 152.09 | 24.30 | 302.03 | 0.4699 | 928.0 | 824.9 | |
| 0.00 | 1.97 | 0.00 | 1.11 | 16.83 | 152.20 | 24.42 | 304.44 | 0.4818 | 528.0 | 499.3 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 15.57 | 151.90 | 24.12 | 302.44 | 0.4683 | 701.0 | 569.9 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 17.57 | 151.39 | 23.61 | 306.62 | 0.4777 | -570.0 | -501.9 | |
| 0.00 | 1.71 | 0.00 | 0.96 | 17.55 | 150.71 | 22.93 | 307.33 | 0.4691 | -558.0 | -503.3 | |
| 0.00 | 1.62 | 0.00 | 0.90 | 16.26 | 150.41 | 22.63 | 305.31 | 0.4545 | -947.0 | -831.1 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 17.40 | 150.52 | 22.74 | 307.27 | 0.4654 | -726.0 | -641.5 | |
| 1.37 | 2.65 | 0.77 | 1.49 | 18.11 | 150.45 | 22.67 | 308.61 | 0.4707 | -866.2 | -718.3 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 17.12 | 150.32 | 22.53 | 307.00 | 0.4606 | -768.0 | -626.9 | |
| 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. | |