SDO HMI 2014-07-07 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.35 | 0.00 | 13.31 | -13.47 | 257.58 | 18.47 | 226.68 | 0.4248 | 718.4 | 637.8 | |
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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 |
| 0.00 | 1.18 | 0.00 | 0.65 | -12.58 | 260.52 | 21.41 | 232.51 | 0.4508 | 650.0 | 556.8 | |
| 0.00 | 0.55 | 0.00 | 0.30 | -13.71 | 259.78 | 20.67 | 229.55 | 0.4525 | 540.0 | 496.5 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -14.38 | 259.74 | 20.63 | 228.35 | 0.4586 | 546.0 | 443.3 | |
| 0.00 | 1.91 | 0.00 | 1.06 | -13.45 | 259.62 | 20.51 | 229.79 | 0.4481 | 860.0 | 663.0 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -13.69 | 259.11 | 20.00 | 228.66 | 0.4444 | 542.0 | 570.0 | |
| 0.00 | 3.63 | 0.00 | 2.00 | -13.37 | 258.88 | 19.77 | 228.90 | 0.4384 | 819.0 | 679.2 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -14.16 | 258.75 | 19.64 | 227.34 | 0.4450 | 678.0 | 569.6 | |
| 0.00 | 2.00 | 0.00 | 1.10 | -13.94 | 258.70 | 19.58 | 227.64 | 0.4420 | 725.0 | 499.8 | |
| 0.00 | 3.36 | 0.00 | 1.81 | -11.82 | 256.49 | 17.38 | 228.14 | 0.3942 | 901.0 | 718.7 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -13.19 | 256.59 | 17.47 | 225.74 | 0.4099 | 815.0 | 638.5 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -13.35 | 256.53 | 17.42 | 225.37 | 0.4110 | 679.0 | 561.7 | |
| 0.00 | 4.91 | 0.00 | 2.68 | -14.84 | 255.95 | 16.84 | 221.87 | 0.4214 | 871.0 | 742.9 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -11.78 | 252.48 | 13.37 | 220.79 | 0.3480 | 713.0 | 552.6 | |
| 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. | |