SDO HMI 2014-05-27 07:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.16 | 0.00 | 11.83 | -19.55 | 49.62 | -10.51 | 152.92 | 0.3633 | 290.7 | 291.1 | |
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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 | 1.53 | 0.00 | 0.79 | -17.98 | 56.72 | -3.40 | 168.92 | 0.2947 | 766.0 | 477.1 | |
| 0.00 | 1.35 | 0.00 | 0.71 | -19.83 | 56.04 | -4.09 | 168.13 | 0.3271 | 923.0 | 683.9 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -16.20 | 53.39 | -6.73 | 156.45 | 0.2829 | 820.0 | 634.4 | |
| 0.00 | 1.80 | 0.00 | 0.93 | -14.63 | 53.38 | -6.74 | 153.89 | 0.2592 | 793.0 | 616.1 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -18.67 | 52.65 | -7.47 | 157.65 | 0.3253 | 776.0 | 629.5 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -19.05 | 52.47 | -7.65 | 157.64 | 0.3322 | 838.0 | 702.9 | |
| 0.00 | 1.99 | 0.00 | 1.04 | -18.73 | 52.26 | -7.86 | 156.69 | 0.3288 | 980.0 | 810.9 | |
| 0.00 | 1.80 | 0.00 | 0.95 | -19.27 | 51.19 | -8.93 | 154.67 | 0.3440 | 958.0 | 822.5 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -19.81 | 50.96 | -9.16 | 154.83 | 0.3536 | 810.0 | 647.7 | |
| 0.00 | 3.25 | 0.00 | 1.72 | -20.06 | 50.52 | -9.60 | 154.12 | 0.3604 | 791.0 | 624.5 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -21.89 | 42.61 | -17.51 | 141.70 | 0.4523 | -796.0 | -673.5 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -21.63 | 42.61 | -17.51 | 141.31 | 0.4493 | -914.0 | -746.7 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -22.08 | 42.10 | -18.02 | 141.22 | 0.4595 | -848.0 | -730.0 | |
| 0.00 | 1.35 | 0.00 | 0.76 | -22.44 | 41.81 | -18.31 | 141.31 | 0.4664 | -797.0 | -561.5 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -22.01 | 41.56 | -18.56 | 140.32 | 0.4640 | -740.0 | -494.9 | |
| 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. | |