SDO HMI 2014-05-28 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.18 | 34.55 | 8.43 | 21.52 | -10.92 | 83.92 | 35.94 | 252.94 | 0.6046 | 375.1 | 200.5 | |
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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 |
| 13.18 | 16.61 | 8.43 | 10.62 | -9.77 | 86.47 | 38.49 | 255.88 | 0.6347 | 857.3 | 514.9 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -9.88 | 84.88 | 36.90 | 255.24 | 0.6139 | 660.0 | 615.0 | |
| 0.00 | 1.08 | 0.00 | 0.68 | -10.41 | 84.68 | 36.70 | 254.33 | 0.6127 | 586.0 | 424.3 | |
| 0.00 | 1.99 | 0.00 | 1.25 | -11.98 | 84.64 | 36.66 | 251.81 | 0.6170 | 580.0 | 418.2 | |
| 0.00 | 1.26 | 0.00 | 0.79 | -10.07 | 84.25 | 36.27 | 254.73 | 0.6060 | 611.0 | 579.1 | |
| 0.00 | 0.90 | 0.00 | 0.56 | -10.32 | 83.87 | 35.88 | 254.19 | 0.6015 | 661.0 | 498.0 | |
| 0.00 | 1.44 | 0.00 | 0.89 | -11.96 | 83.29 | 35.31 | 251.30 | 0.5992 | 649.0 | 511.2 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -11.56 | 83.12 | 35.14 | 251.88 | 0.5955 | 741.0 | 618.3 | |
| 0.00 | 2.62 | 0.00 | 1.59 | -12.19 | 81.97 | 33.98 | 250.35 | 0.5823 | 691.0 | 548.5 | |
| 0.00 | 0.63 | 0.00 | 0.38 | -10.48 | 80.55 | 32.57 | 252.66 | 0.5567 | -612.0 | -501.4 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -10.23 | 80.41 | 32.43 | 253.03 | 0.5539 | -573.0 | -500.5 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -9.81 | 79.82 | 31.84 | 253.53 | 0.5441 | -669.0 | -563.0 | |
| 0.00 | 2.44 | 0.00 | 1.44 | -15.00 | 78.06 | 30.08 | 243.42 | 0.5434 | -709.0 | -544.1 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -14.49 | 75.27 | 27.28 | 242.29 | 0.5032 | -655.0 | -475.7 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -14.13 | 73.99 | 26.00 | 241.94 | 0.4838 | -775.0 | -649.0 | |
| 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. | |