SDO HMI 2014-05-19 15:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.32 | 135.53 | 27.81 | 178.83 | -13.32 | 229.34 | 67.77 | 256.39 | 0.9268 | 308.3 | 110.5 | |
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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 |
| 10.97 | 117.98 | 15.15 | 161.33 | -12.63 | 230.53 | 68.96 | 257.30 | 0.9351 | 496.2 | 143.5 | |
| 9.35 | -1.00 | 12.66 | -1.00 | -13.23 | 230.02 | 68.45 | 256.63 | 0.9322 | 539.3 | 999999 | |
| 0.00 | 1.53 | 0.00 | 1.98 | -12.55 | 229.04 | 67.48 | 257.31 | 0.9258 | 646.0 | 584.1 | |
| 0.00 | 1.08 | 0.00 | 1.38 | -13.37 | 228.68 | 67.11 | 256.40 | 0.9238 | 329.0 | 292.9 | |
| 0.00 | 1.08 | 0.00 | 1.24 | -15.03 | 225.63 | 64.06 | 254.35 | 0.9037 | -289.0 | -256.7 | |
| 0.00 | 1.62 | 0.00 | 1.87 | -15.81 | 225.86 | 64.29 | 253.51 | 0.9059 | -142.0 | -118.0 | |
| 0.00 | 1.17 | 0.00 | 1.30 | -14.44 | 224.74 | 63.18 | 254.93 | 0.8968 | -361.0 | -274.6 | |
| 0.00 | 1.35 | 0.00 | 1.28 | -12.98 | 219.61 | 58.05 | 256.08 | 0.8539 | -374.0 | -345.1 | |
| 0.00 | 2.16 | 0.00 | 2.24 | -18.53 | 222.14 | 60.57 | 250.04 | 0.8805 | -90.0 | -121.3 | |
| 0.00 | 3.33 | 0.00 | 3.02 | -21.81 | 216.60 | 55.03 | 245.22 | 0.8401 | -435.0 | -334.2 | |
| 0.00 | 1.17 | 0.00 | 0.93 | -16.28 | 212.15 | 50.59 | 250.87 | 0.7872 | -655.0 | -534.6 | |
| 0.00 | 1.17 | 0.00 | 0.95 | -19.64 | 212.22 | 50.65 | 246.72 | 0.7951 | -459.0 | -327.8 | |
| 0.00 | 1.89 | 0.00 | 1.31 | -24.45 | 201.19 | 39.63 | 236.30 | 0.7002 | -548.0 | -470.3 | |
| 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. | |