SDO HMI 2014-04-14 06:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.14 | 288.42 | 27.82 | 151.26 | 12.25 | 262.98 | -6.09 | 18.19 | 0.3277 | -1106.4 | -365.8 | |
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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 |
| 5.75 | 274.02 | 3.01 | 143.25 | 12.37 | 263.80 | -5.28 | 16.18 | 0.3237 | -1237.0 | -394.6 | |
| 25.55 | -1.00 | 13.36 | -1.00 | 12.12 | 263.71 | -5.36 | 16.66 | 0.3201 | -1495.6 | 999999 | |
| 0.27 | -1.00 | 0.14 | -1.00 | 11.81 | 263.65 | -5.42 | 17.12 | 0.3154 | -1529.3 | 999999 | |
| 19.63 | -1.00 | 10.26 | -1.00 | 12.03 | 263.31 | -5.76 | 17.92 | 0.3206 | -1401.7 | 999999 | |
| 0.88 | -1.00 | 0.46 | -1.00 | 12.10 | 262.85 | -6.23 | 19.19 | 0.3242 | -681.4 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 18.52 | 262.56 | -6.51 | 14.72 | 0.4250 | -906.0 | -736.9 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 11.40 | 260.85 | -8.22 | 25.59 | 0.3261 | -658.0 | -533.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 14.44 | 259.65 | -9.42 | 24.82 | 0.3792 | -689.0 | -502.3 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 18.30 | 258.18 | -10.90 | 23.91 | 0.4446 | -656.0 | -567.4 | |
| 0.00 | 1.50 | 0.00 | 0.84 | 18.10 | 255.40 | -13.67 | 29.28 | 0.4611 | -877.0 | -747.9 | |
| 1.06 | 2.21 | 0.59 | 1.23 | 17.09 | 254.99 | -14.08 | 31.17 | 0.4510 | 823.3 | 605.0 | |
| 0.00 | 1.59 | 0.00 | 0.88 | 16.09 | 253.87 | -15.20 | 34.43 | 0.4474 | 874.0 | 777.3 | |
| 0.00 | 1.33 | 0.00 | 0.75 | 11.68 | 245.13 | -23.95 | 53.88 | 0.4940 | 708.0 | 585.2 | |
| 0.00 | 3.27 | 0.00 | 1.88 | 11.28 | 243.51 | -25.57 | 56.30 | 0.5107 | 697.0 | 640.8 | |
| 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. | |