SDO HMI 2014-03-07 14:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.73 | 268.93 | 71.62 | 290.53 | -13.51 | 109.40 | 63.55 | 258.52 | 0.8886 | 333.2 | 210.3 | |
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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 |
| 11.51 | 27.60 | 16.49 | 39.53 | -15.59 | 116.83 | 70.98 | 256.00 | 0.9400 | 444.1 | 264.8 | |
| 0.00 | 0.95 | 0.00 | 1.20 | -11.08 | 113.54 | 67.69 | 261.00 | 0.9209 | 249.0 | 257.5 | |
| 3.81 | 5.88 | 4.59 | 7.09 | -11.42 | 112.51 | 66.66 | 260.70 | 0.9137 | 514.2 | 393.5 | |
| 0.69 | 3.29 | 0.89 | 4.26 | -15.97 | 114.40 | 68.55 | 255.67 | 0.9252 | -137.2 | 73.3 | |
| 0.00 | 1.30 | 0.00 | 1.65 | -17.16 | 114.02 | 68.16 | 254.39 | 0.9226 | 274.0 | 237.9 | |
| 0.00 | 1.30 | 0.00 | 1.60 | -16.76 | 113.14 | 67.29 | 254.83 | 0.9169 | 265.0 | 265.8 | |
| 0.00 | 1.04 | 0.00 | 1.18 | -15.46 | 111.04 | 65.18 | 256.29 | 0.9023 | -445.0 | -365.4 | |
| 11.94 | 22.50 | 14.59 | 27.46 | -18.39 | 112.99 | 67.14 | 253.05 | 0.9158 | -453.7 | -139.7 | |
| 3.98 | 17.91 | 4.20 | 18.91 | -12.84 | 108.76 | 62.90 | 259.27 | 0.8854 | -396.2 | -18.9 | |
| 0.00 | 0.95 | 0.00 | 1.02 | -15.67 | 109.15 | 63.30 | 256.07 | 0.8881 | 268.0 | 276.7 | |
| 30.80 | 182.40 | 30.86 | 182.77 | -12.30 | 107.02 | 61.17 | 259.93 | 0.8713 | 834.6 | 268.1 | |
| 0.00 | 1.21 | 0.00 | 1.22 | -14.98 | 107.31 | 61.46 | 256.85 | 0.8735 | -307.0 | -287.7 | |
| 0.00 | 1.30 | 0.00 | 1.31 | -15.54 | 107.27 | 61.41 | 256.21 | 0.8731 | -436.0 | -362.5 | |
| 0.00 | 0.61 | 0.00 | 0.59 | -13.13 | 105.85 | 60.00 | 259.00 | 0.8612 | 330.0 | 246.1 | |
| 0.00 | 0.69 | 0.00 | 0.74 | -19.41 | 109.19 | 63.34 | 251.85 | 0.8890 | -366.0 | -320.2 | |
| 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. | |