SDO HMI 2014-03-13 01:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.51 | 18.92 | 1.88 | 13.81 | -9.49 | 21.54 | 47.64 | 263.67 | 0.7344 | 42.7 | 152.7 | |
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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 | 0.87 | 0.00 | 0.66 | -9.31 | 23.73 | 49.82 | 263.90 | 0.7606 | 452.0 | 336.6 | |
| 0.95 | 3.12 | 0.72 | 2.37 | -9.05 | 23.58 | 49.68 | 264.25 | 0.7590 | 588.0 | 585.4 | |
| 1.13 | 2.43 | 0.85 | 1.84 | -9.54 | 23.58 | 49.68 | 263.61 | 0.7589 | 581.8 | 452.2 | |
| 0.00 | 1.48 | 0.00 | 1.11 | -9.59 | 23.31 | 49.41 | 263.55 | 0.7558 | 398.0 | 488.6 | |
| 0.00 | 2.43 | 0.00 | 1.80 | -9.52 | 22.51 | 48.60 | 263.67 | 0.7467 | 527.0 | 440.4 | |
| 0.00 | 1.13 | 0.00 | 0.83 | -7.97 | 21.70 | 47.80 | 265.79 | 0.7379 | -364.0 | -367.0 | |
| 0.00 | 1.13 | 0.00 | 0.82 | -9.77 | 21.38 | 47.47 | 263.35 | 0.7335 | -346.0 | -300.9 | |
| 0.00 | 1.21 | 0.00 | 0.88 | -9.64 | 21.13 | 47.22 | 263.53 | 0.7306 | -358.0 | -414.8 | |
| 0.43 | 1.21 | 0.31 | 0.88 | -9.62 | 21.04 | 47.13 | 263.56 | 0.7295 | -400.4 | -371.4 | |
| 0.00 | 0.87 | 0.00 | 0.62 | -9.25 | 20.84 | 46.93 | 264.08 | 0.7272 | -372.0 | -317.0 | |
| 0.00 | 0.61 | 0.00 | 0.43 | -9.74 | 19.30 | 45.40 | 263.42 | 0.7087 | 512.0 | 480.0 | |
| 0.00 | 1.30 | 0.00 | 0.90 | -9.85 | 18.81 | 44.90 | 263.28 | 0.7026 | 319.0 | 353.6 | |
| 0.00 | 1.13 | 0.00 | 0.67 | -11.50 | 7.97 | 34.07 | 260.10 | 0.5594 | -612.0 | -520.5 | |
| 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. | |