SDO HMI 2014-05-14 09:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.47 | 262.95 | 32.57 | 174.44 | -23.81 | 193.86 | -37.14 | 123.72 | 0.6658 | 660.6 | 249.1 | |
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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 |
| 4.49 | 250.46 | 2.94 | 165.12 | -23.76 | 194.73 | -36.27 | 124.14 | 0.6564 | 1098.0 | 298.8 | |
| 12.03 | -1.00 | 7.88 | -1.00 | -23.59 | 194.58 | -36.42 | 123.82 | 0.6571 | 1134.3 | 999999 | |
| 32.95 | -1.00 | 21.75 | -1.00 | -23.71 | 194.08 | -36.91 | 123.69 | 0.6632 | 953.4 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.48 | -23.26 | 192.14 | -38.86 | 122.00 | 0.6820 | 547.0 | 453.2 | |
| 0.00 | 1.26 | 0.00 | 0.92 | -25.80 | 188.07 | -42.92 | 123.32 | 0.7361 | -717.0 | -593.4 | |
| 0.00 | 0.63 | 0.00 | 0.45 | -23.54 | 188.32 | -42.68 | 120.53 | 0.7239 | -433.0 | -331.0 | |
| 0.00 | 0.90 | 0.00 | 0.67 | -25.94 | 187.13 | -43.87 | 123.07 | 0.7460 | -558.0 | -481.7 | |
| 0.00 | 1.97 | 0.00 | 1.48 | -26.29 | 186.72 | -44.27 | 123.33 | 0.7514 | -725.0 | -636.5 | |
| 0.00 | 1.35 | 0.00 | 1.01 | -26.02 | 186.52 | -44.47 | 122.90 | 0.7522 | -727.0 | -661.3 | |
| 0.00 | 1.44 | 0.00 | 1.08 | -26.14 | 186.18 | -44.82 | 122.91 | 0.7560 | -496.0 | -435.5 | |
| 0.00 | 0.90 | 0.00 | 0.68 | -26.06 | 185.79 | -45.21 | 122.64 | 0.7594 | -535.0 | -411.2 | |
| 0.00 | 2.51 | 0.00 | 1.92 | -26.28 | 185.58 | -45.42 | 122.84 | 0.7623 | -508.0 | -411.5 | |
| 0.00 | 0.81 | 0.00 | 0.63 | -27.86 | 184.64 | -46.36 | 124.37 | 0.7774 | -627.0 | -530.7 | |
| 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. | |