SDO HMI 2014-04-11 17:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.68 | 0.00 | 12.05 | -19.70 | 324.85 | 22.21 | 233.15 | 0.4466 | 185.7 | 108.6 | |
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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 | 1.50 | 0.00 | 0.87 | -15.36 | 332.78 | 30.13 | 249.80 | 0.5179 | 680.0 | 551.2 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -17.30 | 332.56 | 29.92 | 246.09 | 0.5230 | 545.0 | 572.1 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -17.04 | 332.33 | 29.69 | 246.45 | 0.5187 | 428.0 | 482.3 | |
| 0.00 | 2.03 | 0.00 | 1.16 | -17.38 | 330.88 | 28.24 | 244.94 | 0.5005 | 696.0 | 529.0 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -18.47 | 330.64 | 28.00 | 242.73 | 0.5029 | 768.0 | 602.3 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -19.30 | 330.18 | 27.53 | 240.87 | 0.5014 | 846.0 | 621.8 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -17.44 | 329.54 | 26.90 | 243.94 | 0.4824 | 854.0 | 635.9 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -16.88 | 329.10 | 26.46 | 244.75 | 0.4733 | 669.0 | 526.1 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -18.54 | 327.64 | 24.99 | 240.32 | 0.4630 | 574.0 | 423.9 | |
| 0.00 | 1.50 | 0.00 | 0.82 | -18.72 | 325.27 | 22.63 | 237.76 | 0.4326 | 703.0 | 559.7 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -24.14 | 316.60 | 13.96 | 214.85 | 0.3869 | -775.0 | -626.4 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -21.38 | 316.12 | 13.48 | 218.79 | 0.3479 | -760.0 | -520.8 | |
| 0.00 | 2.82 | 0.00 | 1.49 | -21.92 | 315.90 | 13.26 | 217.35 | 0.3523 | -866.0 | -704.6 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -24.25 | 316.04 | 13.39 | 213.62 | 0.3831 | -920.0 | -762.7 | |
| 0.00 | 1.76 | 0.00 | 0.94 | -25.01 | 314.49 | 11.85 | 209.43 | 0.3802 | -656.0 | -609.5 | |
| 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. | |