SDO HMI 2014-03-02 04:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.77 | 91.34 | 11.91 | 54.66 | -7.82 | 151.53 | 34.33 | 266.73 | 0.5615 | 481.3 | 361.0 | |
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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 | 1.12 | 0.00 | 0.68 | -8.68 | 152.70 | 35.50 | 265.20 | 0.5783 | 62.0 | -19.3 | |
| 7.08 | 76.23 | 4.28 | 45.98 | -7.65 | 152.48 | 35.29 | 266.99 | 0.5755 | 806.5 | 455.5 | |
| 0.00 | 1.73 | 0.00 | 1.04 | -8.13 | 152.34 | 35.15 | 266.15 | 0.5734 | 549.0 | 455.0 | |
| 5.70 | -2.00 | 3.43 | -2.00 | -7.66 | 152.23 | 35.03 | 266.98 | 0.5719 | 1039.9 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.73 | -8.98 | 152.25 | 35.05 | 264.67 | 0.5720 | -329.0 | -314.9 | |
| 6.99 | -2.00 | 4.20 | -2.00 | -7.95 | 151.96 | 34.76 | 266.48 | 0.5680 | 957.1 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -7.63 | 150.52 | 33.32 | 267.12 | 0.5473 | 611.0 | 531.9 | |
| 0.00 | 2.59 | 0.00 | 1.47 | -8.54 | 146.68 | 29.49 | 265.45 | 0.4903 | 694.0 | 501.4 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -8.99 | 146.52 | 29.32 | 264.50 | 0.4879 | 839.0 | 680.0 | |
| 0.00 | 2.85 | 0.00 | 1.60 | -9.50 | 145.43 | 28.23 | 263.36 | 0.4716 | -785.0 | -481.1 | |
| 0.00 | 1.04 | 0.00 | 0.58 | -6.02 | 144.87 | 27.68 | 270.86 | 0.4639 | -661.0 | -543.9 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -6.01 | 144.57 | 27.37 | 270.93 | 0.4592 | -656.0 | -508.9 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -5.81 | 144.39 | 27.19 | 271.39 | 0.4567 | -817.0 | -638.6 | |
| 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. | |