SDO HMI 2014-04-19 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 |
| 0.00 | 26.70 | 0.00 | 13.64 | -16.06 | 200.10 | -2.95 | 178.20 | 0.2243 | -479.2 | -339.3 | |
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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 | 2.48 | 0.00 | 1.25 | -13.27 | 208.79 | 5.75 | 214.96 | 0.1709 | 902.0 | 675.1 | |
| 0.00 | 2.13 | 0.00 | 1.07 | -13.73 | 208.03 | 4.98 | 209.79 | 0.1705 | 908.0 | 745.0 | |
| 0.00 | 1.68 | 0.00 | 0.85 | -13.55 | 207.84 | 4.79 | 209.39 | 0.1662 | 897.0 | 713.5 | |
| 0.00 | 3.81 | 0.00 | 1.90 | -10.49 | 206.53 | 3.48 | 213.26 | 0.1094 | -873.0 | -683.5 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -11.91 | 206.27 | 3.22 | 205.40 | 0.1287 | -958.0 | -797.1 | |
| 0.00 | 0.89 | 0.00 | 0.44 | -8.35 | 203.95 | 0.90 | 196.22 | 0.0562 | -809.0 | -648.5 | |
| 0.00 | 2.04 | 0.00 | 1.03 | -15.51 | 202.84 | -0.20 | 178.89 | 0.1785 | -818.0 | -613.0 | |
| 0.00 | 1.86 | 0.00 | 0.96 | -19.75 | 198.89 | -4.15 | 164.75 | 0.2604 | -671.0 | -508.6 | |
| 0.00 | 0.98 | 0.00 | 0.50 | -20.95 | 197.73 | -5.32 | 162.26 | 0.2854 | -782.0 | -701.7 | |
| 0.00 | 1.42 | 0.00 | 0.74 | -22.79 | 196.41 | -6.64 | 160.53 | 0.3213 | -776.0 | -636.5 | |
| 0.00 | 1.51 | 0.00 | 0.79 | -23.44 | 194.75 | -8.29 | 157.05 | 0.3409 | -915.0 | -707.0 | |
| 0.00 | 0.98 | 0.00 | 0.51 | -18.64 | 192.19 | -10.86 | 142.50 | 0.2945 | -760.0 | -615.8 | |
| 0.00 | 1.60 | 0.00 | 0.82 | -14.72 | 191.72 | -11.33 | 131.13 | 0.2533 | -874.0 | -633.7 | |
| 0.00 | 2.04 | 0.00 | 1.08 | -19.83 | 188.13 | -14.91 | 136.39 | 0.3525 | -823.0 | -704.3 | |
| 0.00 | 2.04 | 0.00 | 1.08 | -19.94 | 187.72 | -15.32 | 135.88 | 0.3584 | -836.0 | -645.3 | |
| 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. | |