SDO HMI 2014-01-13 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.02 | 0.00 | 11.12 | 16.40 | 24.71 | 0.37 | 358.95 | 0.3587 | 450.4 | 279.0 | |
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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 | 2.04 | 0.00 | 1.08 | 15.81 | 29.15 | 4.81 | 346.84 | 0.3557 | -1011.0 | -754.7 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 16.18 | 28.94 | 4.60 | 347.62 | 0.3610 | -734.0 | -617.9 | |
| 0.00 | 2.98 | 0.00 | 1.57 | 15.67 | 26.47 | 2.13 | 354.03 | 0.3463 | -883.0 | -762.9 | |
| 0.00 | 1.53 | 0.00 | 0.81 | 17.00 | 25.87 | 1.53 | 355.98 | 0.3670 | 862.0 | 737.9 | |
| 0.00 | 2.72 | 0.00 | 1.45 | 17.31 | 25.69 | 1.35 | 356.51 | 0.3720 | 777.0 | 718.4 | |
| 0.00 | 2.04 | 0.00 | 1.08 | 16.24 | 24.64 | 0.30 | 359.19 | 0.3538 | 741.0 | 605.1 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 15.58 | 23.60 | -0.74 | 2.10 | 0.3431 | 829.0 | 702.4 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 15.80 | 23.17 | -1.17 | 3.27 | 0.3471 | 817.0 | 670.2 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 16.65 | 22.67 | -1.67 | 4.45 | 0.3616 | 846.0 | 670.7 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 15.93 | 22.58 | -1.76 | 4.85 | 0.3499 | 904.0 | 658.8 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 16.09 | 22.37 | -1.97 | 5.40 | 0.3528 | 901.0 | 696.7 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 17.73 | 22.07 | -2.27 | 5.72 | 0.3800 | 731.0 | 575.4 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 15.90 | 21.85 | -2.49 | 6.88 | 0.3506 | 797.0 | 640.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 17.23 | 20.75 | -3.59 | 9.23 | 0.3747 | 729.0 | 525.1 | |
| 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. | |