SDO HMI 2014-04-15 01:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.12 | 269.51 | 23.04 | 140.85 | 12.27 | 262.79 | 4.18 | 346.74 | 0.3206 | -708.6 | -358.3 | |
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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 | 1.59 | 0.00 | 0.83 | 12.10 | 265.67 | 7.06 | 338.44 | 0.3283 | 904.0 | 721.8 | |
| 11.58 | 251.92 | 6.05 | 131.49 | 12.09 | 263.72 | 5.11 | 344.02 | 0.3176 | -1387.7 | -423.6 | |
| 10.26 | -2.00 | 5.36 | -2.00 | 12.31 | 263.70 | 5.08 | 344.29 | 0.3210 | -1179.4 | 999999 | |
| 22.28 | -2.00 | 11.63 | -2.00 | 12.05 | 263.29 | 4.68 | 345.28 | 0.3152 | -1369.2 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.72 | 18.25 | 258.78 | 0.16 | 359.62 | 0.4067 | -654.0 | -489.2 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 17.80 | 255.52 | -3.09 | 7.36 | 0.4027 | -685.0 | -571.3 | |
| 0.00 | 1.24 | 0.00 | 0.66 | 15.73 | 254.65 | -3.97 | 10.37 | 0.3717 | 720.0 | 518.1 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 12.47 | 253.99 | -4.63 | 14.23 | 0.3218 | 784.0 | 560.2 | |
| 0.00 | 2.30 | 0.00 | 1.20 | 12.79 | 253.98 | -4.63 | 14.00 | 0.3269 | 687.0 | 558.7 | |
| 0.00 | 1.50 | 0.00 | 0.79 | 13.71 | 253.78 | -4.83 | 13.89 | 0.3425 | 779.0 | 645.9 | |
| 0.00 | 0.71 | 0.00 | 0.38 | 15.98 | 252.13 | -6.49 | 16.45 | 0.3851 | 775.0 | 702.1 | |
| 0.00 | 2.83 | 0.00 | 1.54 | 16.55 | 248.91 | -9.71 | 23.24 | 0.4112 | 573.0 | 372.0 | |
| 0.00 | 2.12 | 0.00 | 1.13 | 12.90 | 246.93 | -11.68 | 31.99 | 0.3741 | 669.0 | 522.0 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 12.06 | 246.41 | -12.21 | 34.42 | 0.3674 | 626.0 | 466.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 12.00 | 246.16 | -12.46 | 35.06 | 0.3690 | 635.0 | 510.6 | |
| 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. | |