SDO HMI 2014-05-19 06:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.54 | 250.55 | 20.87 | 147.04 | -24.45 | 190.76 | 24.26 | 224.38 | 0.5369 | 628.2 | 332.7 | |
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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 |
| 34.10 | 235.52 | 20.03 | 138.38 | -24.36 | 191.10 | 24.60 | 224.90 | 0.5393 | 1229.9 | 385.9 | |
| 0.72 | -1.00 | 0.42 | -1.00 | -24.11 | 190.47 | 23.96 | 224.58 | 0.5303 | 1011.6 | 999999 | |
| 0.27 | -1.00 | 0.16 | -1.00 | -24.11 | 190.25 | 23.75 | 224.33 | 0.5280 | 879.0 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -26.35 | 190.68 | 24.18 | 221.67 | 0.5541 | 286.0 | 310.7 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -24.28 | 189.74 | 23.24 | 223.50 | 0.5244 | 826.0 | 699.6 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -26.90 | 189.65 | 23.15 | 219.80 | 0.5498 | 652.0 | 472.4 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -24.52 | 186.87 | 20.37 | 219.66 | 0.4982 | -692.0 | -498.4 | |
| 0.00 | 1.80 | 0.00 | 1.03 | -25.98 | 186.23 | 19.73 | 216.82 | 0.5083 | -604.0 | -598.1 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -24.69 | 185.98 | 19.47 | 218.22 | 0.4915 | -811.0 | -671.1 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -25.78 | 185.59 | 19.09 | 216.21 | 0.5003 | -743.0 | -636.1 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -27.25 | 185.70 | 19.19 | 214.49 | 0.5182 | -619.0 | -522.5 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -26.98 | 185.62 | 19.11 | 214.71 | 0.5144 | -732.0 | -643.2 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -26.52 | 185.25 | 18.74 | 214.80 | 0.5058 | -760.0 | -613.2 | |
| 0.45 | 1.53 | 0.26 | 0.88 | -27.42 | 185.15 | 18.65 | 213.55 | 0.5156 | -938.0 | -825.8 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -27.06 | 184.26 | 17.76 | 212.76 | 0.5040 | -805.0 | -727.8 | |
| 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. | |