SDO HMI 2014-03-25 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.95 | 0.00 | 15.56 | -13.83 | 129.92 | -39.76 | 103.45 | 0.6389 | 512.3 | 474.5 | |
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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 | 1.05 | 0.00 | 0.60 | -19.80 | 142.70 | -26.99 | 118.97 | 0.4900 | 620.0 | 446.9 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -8.40 | 137.11 | -32.58 | 94.91 | 0.5368 | 650.0 | 592.7 | |
| 0.00 | 1.84 | 0.00 | 1.08 | -5.52 | 136.62 | -33.07 | 89.59 | 0.5453 | 669.0 | 493.0 | |
| 0.00 | 0.87 | 0.00 | 0.55 | -16.46 | 132.43 | -37.25 | 108.15 | 0.6132 | 133.0 | 195.8 | |
| 0.00 | 1.31 | 0.00 | 0.80 | -11.19 | 133.34 | -36.35 | 99.61 | 0.5919 | 546.0 | 486.3 | |
| 0.00 | 3.67 | 0.00 | 2.30 | -14.75 | 132.02 | -37.67 | 105.29 | 0.6149 | 529.0 | 598.2 | |
| 0.00 | 1.31 | 0.00 | 0.81 | -9.25 | 132.84 | -36.84 | 96.32 | 0.5977 | 620.0 | 541.5 | |
| 0.00 | 3.15 | 0.00 | 1.99 | -15.48 | 131.59 | -38.10 | 106.37 | 0.6220 | 611.0 | 558.7 | |
| 0.00 | 0.61 | 0.00 | 0.39 | -15.15 | 131.62 | -38.07 | 105.84 | 0.6209 | 672.0 | 553.0 | |
| 0.00 | 2.45 | 0.00 | 1.55 | -15.25 | 131.32 | -38.36 | 105.93 | 0.6250 | 529.0 | 505.8 | |
| 0.00 | 1.75 | 0.00 | 1.11 | -12.69 | 131.12 | -38.56 | 101.80 | 0.6236 | 729.0 | 623.9 | |
| 0.00 | 1.05 | 0.00 | 0.68 | -13.27 | 129.58 | -40.11 | 102.51 | 0.6446 | 672.0 | 597.0 | |
| 0.00 | 1.31 | 0.00 | 0.91 | -15.26 | 125.14 | -44.55 | 104.84 | 0.7025 | 480.0 | 384.2 | |
| 0.00 | 1.05 | 0.00 | 0.91 | -25.40 | 114.89 | -54.80 | 116.24 | 0.8251 | -248.0 | -151.6 | |
| 0.00 | 1.05 | 0.00 | 0.82 | -9.51 | 118.46 | -51.23 | 96.71 | 0.7765 | 520.0 | 465.7 | |
| 0.00 | 0.87 | 0.00 | 0.70 | -9.41 | 117.69 | -51.99 | 96.60 | 0.7848 | 465.0 | 366.5 | |
| 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. | |