SDO HMI 2014-05-26 15:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.99 | 0.00 | 10.66 | -20.04 | 48.46 | -20.50 | 134.98 | 0.4621 | 291.6 | 292.9 | |
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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 | 2.07 | 0.00 | 1.12 | -19.12 | 53.40 | -15.56 | 140.38 | 0.3992 | 766.0 | 559.0 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -14.92 | 53.07 | -15.89 | 131.71 | 0.3558 | 903.0 | 590.8 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -19.02 | 52.60 | -16.35 | 138.85 | 0.4063 | 800.0 | 600.0 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -18.51 | 52.46 | -16.50 | 137.71 | 0.4020 | 620.0 | 472.9 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -18.99 | 52.21 | -16.75 | 138.13 | 0.4101 | 737.0 | 596.7 | |
| 0.00 | 1.89 | 0.00 | 1.03 | -18.98 | 51.63 | -17.32 | 137.20 | 0.4162 | 904.0 | 793.0 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -20.26 | 51.01 | -17.94 | 138.38 | 0.4370 | 657.0 | 564.1 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -20.42 | 50.76 | -18.20 | 138.24 | 0.4414 | 742.0 | 635.5 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -21.12 | 49.53 | -19.43 | 137.58 | 0.4619 | 600.0 | 524.1 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -21.66 | 48.90 | -20.06 | 137.56 | 0.4743 | 624.0 | 477.2 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -20.22 | 43.34 | -25.62 | 128.76 | 0.5224 | 788.0 | 665.5 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -22.70 | 42.16 | -26.80 | 131.39 | 0.5565 | -634.0 | -488.3 | |
| 0.00 | 1.35 | 0.00 | 0.80 | -22.24 | 41.85 | -27.10 | 130.42 | 0.5561 | -719.0 | -615.5 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -20.88 | 41.95 | -27.01 | 128.45 | 0.5439 | -714.0 | -581.5 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -20.69 | 41.99 | -26.97 | 128.18 | 0.5419 | -702.0 | -517.8 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -22.63 | 41.44 | -27.52 | 130.60 | 0.5639 | -706.0 | -618.2 | |
| 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. | |