SDO HMI 2014-04-01 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.09 | 0.00 | 10.38 | -17.20 | 123.24 | 42.60 | 250.92 | 0.6768 | -86.8 | -22.1 | |
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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 | 1.23 | 0.00 | 1.03 | -16.44 | 134.62 | 53.98 | 254.38 | 0.8077 | 317.0 | 290.2 | |
| 0.00 | 0.61 | 0.00 | 0.51 | -16.64 | 134.49 | 53.85 | 254.12 | 0.8066 | 514.0 | 420.4 | |
| 0.00 | 1.23 | 0.00 | 1.02 | -17.33 | 134.30 | 53.66 | 253.24 | 0.8053 | 403.0 | 301.4 | |
| 0.00 | 0.61 | 0.00 | 0.49 | -15.88 | 132.94 | 52.30 | 254.94 | 0.7904 | 573.0 | 492.4 | |
| 0.00 | 1.76 | 0.00 | 1.41 | -15.87 | 132.73 | 52.09 | 254.93 | 0.7882 | 631.0 | 474.9 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -15.99 | 132.42 | 51.78 | 254.75 | 0.7851 | 576.0 | 611.7 | |
| 0.00 | 1.67 | 0.00 | 1.13 | -19.11 | 123.17 | 42.52 | 248.94 | 0.6867 | 53.0 | 145.4 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -13.41 | 115.08 | 34.44 | 255.82 | 0.5695 | -655.0 | -486.2 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -18.84 | 114.78 | 34.14 | 246.44 | 0.5816 | -653.0 | -559.7 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -18.54 | 114.52 | 33.88 | 246.82 | 0.5771 | -662.0 | -519.4 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -19.69 | 114.02 | 33.38 | 244.68 | 0.5753 | -524.0 | -434.9 | |
| 0.00 | 1.32 | 0.00 | 0.79 | -20.81 | 113.34 | 32.70 | 242.45 | 0.5717 | -676.0 | -513.0 | |
| 0.00 | 1.40 | 0.00 | 0.78 | -10.53 | 108.20 | 27.55 | 259.74 | 0.4641 | -603.0 | -424.2 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -23.62 | 108.30 | 27.66 | 234.30 | 0.5258 | -509.0 | -512.6 | |
| 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. | |