SDO HMI 2014-05-19 11:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.07 | 45.53 | 9.73 | 39.52 | -17.99 | 217.82 | 54.05 | 249.53 | 0.8238 | 270.7 | 159.8 | |
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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 |
| 8.37 | 22.04 | 7.46 | 19.58 | -18.51 | 218.78 | 55.01 | 249.10 | 0.8337 | 702.9 | 239.5 | |
| 0.00 | 2.79 | 0.00 | 2.47 | -18.10 | 218.59 | 54.82 | 249.55 | 0.8313 | 465.0 | 448.7 | |
| 0.72 | 2.61 | 0.62 | 2.25 | -17.08 | 217.64 | 53.87 | 250.58 | 0.8208 | 577.0 | 508.4 | |
| 0.00 | 1.62 | 0.00 | 1.39 | -16.87 | 217.39 | 53.62 | 250.79 | 0.8181 | 526.0 | 453.3 | |
| 0.00 | 0.99 | 0.00 | 0.84 | -16.94 | 216.94 | 53.17 | 250.61 | 0.8139 | 688.0 | 605.3 | |
| 0.00 | 1.44 | 0.00 | 1.25 | -18.76 | 217.62 | 53.86 | 248.56 | 0.8236 | -541.0 | -423.9 | |
| 0.00 | 1.35 | 0.00 | 1.14 | -16.89 | 216.65 | 52.88 | 250.62 | 0.8111 | 346.0 | 290.9 | |
| 0.00 | 0.81 | 0.00 | 0.68 | -16.67 | 216.56 | 52.80 | 250.86 | 0.8098 | 171.0 | 167.8 | |
| 0.00 | 1.44 | 0.00 | 1.24 | -18.58 | 217.22 | 53.45 | 248.68 | 0.8195 | -362.0 | -395.1 | |
| 0.00 | 2.52 | 0.00 | 2.14 | -18.25 | 216.85 | 53.08 | 249.01 | 0.8154 | 425.0 | 392.5 | |
| 0.00 | 1.08 | 0.00 | 0.89 | -15.66 | 215.77 | 52.00 | 251.95 | 0.8002 | -572.0 | -513.3 | |
| 0.00 | 1.53 | 0.00 | 1.29 | -18.26 | 216.48 | 52.71 | 248.92 | 0.8119 | -152.0 | -52.4 | |
| 1.08 | 2.16 | 0.91 | 1.82 | -18.42 | 216.24 | 52.47 | 248.66 | 0.8099 | -444.3 | -414.4 | |
| 0.00 | 0.81 | 0.00 | 0.63 | -12.15 | 214.09 | 50.32 | 256.06 | 0.7775 | -180.0 | -189.6 | |
| 0.90 | 2.34 | 0.74 | 1.91 | -17.24 | 215.23 | 51.46 | 249.88 | 0.7978 | -539.3 | -394.2 | |
| 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. | |