SDO HMI 2014-09-30 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.93 | 0.00 | 9.82 | -21.40 | 200.67 | 6.04 | 193.45 | 0.5040 | -185.4 | -167.7 | |
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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 | 2.38 | 0.00 | 1.38 | -17.60 | 214.33 | 19.70 | 218.37 | 0.5198 | 307.0 | 335.9 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -7.27 | 209.52 | 14.89 | 226.90 | 0.3506 | -792.0 | -505.2 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -15.88 | 208.79 | 14.16 | 211.66 | 0.4502 | 756.0 | 598.3 | |
| 0.00 | 1.06 | 0.00 | 0.61 | -21.16 | 207.65 | 13.02 | 204.29 | 0.5128 | 697.0 | 509.2 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -25.29 | 207.62 | 12.99 | 201.06 | 0.5679 | 543.0 | 475.2 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -24.48 | 205.11 | 10.48 | 197.76 | 0.5449 | 596.0 | 511.9 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -22.53 | 199.54 | 4.91 | 189.18 | 0.4973 | -698.0 | -529.8 | |
| 0.00 | 2.03 | 0.00 | 1.13 | -20.31 | 198.69 | 4.07 | 188.32 | 0.4615 | -644.0 | -588.6 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -7.17 | 192.91 | -1.72 | 172.97 | 0.2436 | -899.0 | -804.7 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -13.17 | 191.55 | -3.08 | 171.27 | 0.3463 | -533.0 | -500.0 | |
| 0.00 | 2.56 | 0.00 | 1.64 | -32.58 | 190.90 | -3.73 | 175.05 | 0.6384 | -515.0 | -489.5 | |
| 0.00 | 0.35 | 0.00 | 0.23 | -32.77 | 187.58 | -7.04 | 170.79 | 0.6464 | -594.0 | -608.2 | |
| 0.00 | 0.97 | 0.00 | 0.65 | -34.34 | 186.20 | -8.42 | 169.56 | 0.6697 | -634.0 | -491.0 | |
| 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. | |