SDO HMI 2014-05-28 07:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.80 | 63.61 | 15.06 | 33.34 | -19.59 | 50.72 | 3.83 | 191.31 | 0.3255 | 159.5 | 437.3 | |
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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 | 1.35 | 0.00 | 0.71 | -18.92 | 53.24 | 6.35 | 198.91 | 0.3245 | 890.0 | 714.5 | |
| 0.99 | 2.98 | 0.52 | 1.56 | -18.95 | 52.47 | 5.58 | 196.72 | 0.3211 | 1031.1 | 800.7 | |
| 12.73 | 26.90 | 6.66 | 14.07 | -19.21 | 51.90 | 5.01 | 194.87 | 0.3226 | 1096.1 | 869.6 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -19.72 | 51.52 | 4.63 | 193.41 | 0.3293 | 638.0 | 545.8 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -19.21 | 51.25 | 4.36 | 193.03 | 0.3200 | 617.0 | 510.6 | |
| 0.00 | 0.54 | 0.00 | 0.29 | -20.78 | 50.87 | 3.98 | 190.92 | 0.3441 | 631.0 | 454.3 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -20.91 | 50.61 | 3.72 | 190.16 | 0.3454 | 849.0 | 729.7 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -20.43 | 50.60 | 3.71 | 190.40 | 0.3376 | 853.0 | 709.9 | |
| 0.00 | 2.26 | 0.00 | 1.19 | -20.81 | 50.45 | 3.56 | 189.77 | 0.3434 | 641.0 | 500.8 | |
| 8.40 | 21.66 | 4.39 | 11.33 | -19.69 | 49.58 | 2.69 | 187.91 | 0.3228 | -946.7 | -584.3 | |
| 1.35 | -10.00 | 0.71 | -10.00 | -19.37 | 49.55 | 2.66 | 187.95 | 0.3175 | -1170.7 | 999999 | |
| 5.33 | -10.00 | 2.78 | -10.00 | -19.53 | 49.42 | 2.53 | 187.51 | 0.3198 | -1140.5 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -21.62 | 49.03 | 2.14 | 185.65 | 0.3534 | 857.0 | 680.8 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -20.29 | 44.99 | -1.90 | 174.60 | 0.3312 | -856.0 | -678.9 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -22.33 | 42.63 | -4.26 | 169.24 | 0.3698 | -802.0 | -705.5 | |
| 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. | |