SDO HMI 2014-04-13 14:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.35 | 0.00 | 11.79 | -10.04 | 242.22 | -35.67 | 99.27 | 0.5839 | 615.8 | 499.6 | |
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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 | 0.26 | 0.00 | 0.16 | -10.01 | 244.61 | -33.29 | 99.54 | 0.5502 | 648.0 | 716.0 | |
| 0.00 | 1.68 | 0.00 | 0.99 | -10.34 | 244.53 | -33.36 | 100.13 | 0.5517 | 762.0 | 628.7 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -10.41 | 244.05 | -33.85 | 100.16 | 0.5587 | 602.0 | 515.7 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -9.79 | 243.86 | -34.03 | 99.04 | 0.5606 | 724.0 | 558.9 | |
| 0.00 | 0.71 | 0.00 | 0.42 | -10.30 | 243.73 | -34.17 | 99.92 | 0.5631 | 598.0 | 482.5 | |
| 0.00 | 1.15 | 0.00 | 0.69 | -9.69 | 243.69 | -34.20 | 98.83 | 0.5629 | 555.0 | 482.9 | |
| 0.00 | 2.03 | 0.00 | 1.23 | -9.72 | 242.65 | -35.25 | 98.76 | 0.5777 | -333.0 | -354.0 | |
| 0.00 | 2.74 | 0.00 | 1.68 | -9.48 | 241.70 | -36.20 | 98.26 | 0.5908 | 772.0 | 695.2 | |
| 0.00 | 2.03 | 0.00 | 1.25 | -10.59 | 241.40 | -36.50 | 100.08 | 0.5960 | 716.0 | 568.9 | |
| 0.00 | 1.15 | 0.00 | 0.71 | -9.35 | 241.52 | -36.37 | 98.02 | 0.5931 | 653.0 | 540.2 | |
| 0.00 | 1.77 | 0.00 | 1.09 | -9.74 | 241.36 | -36.53 | 98.65 | 0.5957 | 834.0 | 720.3 | |
| 0.00 | 1.24 | 0.00 | 0.76 | -9.91 | 241.26 | -36.63 | 98.93 | 0.5972 | 753.0 | 669.4 | |
| 0.00 | 1.68 | 0.00 | 1.05 | -11.57 | 240.56 | -37.33 | 101.58 | 0.6087 | 751.0 | 589.5 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -9.58 | 240.19 | -37.70 | 98.27 | 0.6116 | 586.0 | 414.4 | |
| 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. | |