SDO HMI 2014-09-29 04:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.42 | 109.42 | 24.00 | 107.88 | -9.70 | 266.46 | 57.54 | 254.31 | 0.8630 | 180.2 | 158.5 | |
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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 |
| 10.50 | 61.41 | 11.56 | 67.50 | -8.16 | 270.57 | 61.65 | 257.28 | 0.8949 | 601.2 | 230.8 | |
| 0.00 | 1.24 | 0.00 | 1.09 | -10.48 | 262.09 | 53.18 | 252.34 | 0.8282 | 215.0 | 230.6 | |
| 0.00 | 3.44 | 0.00 | 3.00 | -10.75 | 261.70 | 52.78 | 251.89 | 0.8253 | 482.0 | 401.1 | |
| 1.68 | 15.44 | 1.45 | 13.36 | -11.43 | 261.27 | 52.35 | 250.96 | 0.8231 | 636.0 | 518.3 | |
| 4.68 | -4.00 | 4.03 | -4.00 | -11.34 | 260.94 | 52.02 | 250.95 | 0.8198 | 747.3 | 999999 | |
| 0.00 | 1.59 | 0.00 | 1.36 | -11.19 | 260.76 | 51.84 | 251.06 | 0.8176 | 688.0 | 555.3 | |
| 0.00 | 1.06 | 0.00 | 0.89 | -11.09 | 260.04 | 51.12 | 250.92 | 0.8105 | 123.0 | 162.2 | |
| 0.00 | 0.62 | 0.00 | 0.51 | -12.23 | 259.06 | 50.14 | 249.22 | 0.8046 | -314.0 | -304.0 | |
| 0.97 | 7.41 | 0.80 | 6.12 | -11.96 | 258.94 | 50.02 | 249.49 | 0.8026 | -612.1 | -414.6 | |
| 0.00 | 1.94 | 0.00 | 1.60 | -12.18 | 258.90 | 49.98 | 249.22 | 0.8029 | -529.0 | -377.9 | |
| 2.03 | 4.15 | 1.70 | 3.48 | -13.53 | 259.18 | 50.26 | 247.73 | 0.8100 | -591.6 | -418.6 | |
| 0.00 | 1.06 | 0.00 | 0.89 | -13.73 | 258.89 | 49.97 | 247.39 | 0.8080 | -637.0 | -507.9 | |
| 0.00 | 1.15 | 0.00 | 0.93 | -14.27 | 257.24 | 48.32 | 246.06 | 0.7942 | -520.0 | -492.3 | |
| 5.56 | 8.91 | 4.46 | 7.15 | -14.41 | 256.63 | 47.71 | 245.64 | 0.7888 | -701.5 | -534.3 | |
| 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. | |