SDO HMI 2014-05-27 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.35 | 0.00 | 12.39 | -19.77 | 49.28 | -8.65 | 157.26 | 0.3529 | 363.9 | 208.3 | |
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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 | 1.08 | 0.00 | 0.57 | -19.65 | 56.05 | -1.89 | 174.40 | 0.3190 | 701.0 | 481.3 | |
| 0.00 | 1.80 | 0.00 | 0.93 | -16.22 | 53.58 | -4.35 | 164.29 | 0.2700 | 866.0 | 644.6 | |
| 0.00 | 1.08 | 0.00 | 0.56 | -18.66 | 52.81 | -5.12 | 164.25 | 0.3127 | 771.0 | 597.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -19.04 | 52.48 | -5.45 | 163.64 | 0.3203 | 741.0 | 671.6 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -18.78 | 52.33 | -5.60 | 162.96 | 0.3169 | 786.0 | 686.5 | |
| 0.00 | 2.89 | 0.00 | 1.51 | -19.16 | 51.50 | -6.43 | 161.06 | 0.3271 | 915.0 | 800.8 | |
| 0.00 | 1.89 | 0.00 | 1.00 | -19.83 | 51.05 | -6.88 | 160.57 | 0.3399 | 826.0 | 637.4 | |
| 0.00 | 1.26 | 0.00 | 0.66 | -17.57 | 51.05 | -6.88 | 157.93 | 0.3051 | 855.0 | 595.5 | |
| 0.00 | 1.35 | 0.00 | 0.71 | -20.15 | 50.45 | -7.48 | 159.37 | 0.3482 | 782.0 | 688.7 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -19.06 | 50.28 | -7.65 | 157.67 | 0.3327 | 678.0 | 536.3 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -20.25 | 49.83 | -8.10 | 157.92 | 0.3534 | 701.0 | 548.9 | |
| 0.00 | 2.35 | 0.00 | 1.24 | -19.51 | 49.51 | -8.42 | 156.26 | 0.3444 | -807.0 | -705.8 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -21.79 | 42.79 | -15.14 | 145.42 | 0.4292 | -856.0 | -718.1 | |
| 0.00 | 2.17 | 0.00 | 1.19 | -22.21 | 42.02 | -15.91 | 144.74 | 0.4413 | -809.0 | -613.0 | |
| 0.00 | 2.26 | 0.00 | 1.25 | -22.37 | 41.83 | -16.10 | 144.66 | 0.4450 | -691.0 | -578.3 | |
| 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. | |