SDO HMI 2014-09-30 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.99 | 0.00 | 8.52 | -19.38 | 199.35 | 1.98 | 187.30 | 0.4765 | -130.1 | -100.6 | |
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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 | 2.12 | 0.00 | 1.12 | -8.55 | 211.36 | 13.99 | 222.49 | 0.3554 | -885.0 | -689.2 | |
| 0.00 | 1.76 | 0.00 | 0.96 | -14.32 | 210.88 | 13.51 | 212.39 | 0.4244 | 775.0 | 610.5 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -24.97 | 211.18 | 13.80 | 202.46 | 0.5683 | 786.0 | 587.8 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -15.91 | 208.81 | 11.44 | 206.44 | 0.4302 | 578.0 | 509.8 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -21.16 | 207.59 | 10.22 | 199.51 | 0.4974 | 681.0 | 569.9 | |
| 0.00 | 0.44 | 0.00 | 0.26 | -24.53 | 205.07 | 7.70 | 193.23 | 0.5351 | 534.0 | 572.8 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -13.35 | 200.61 | 3.24 | 189.09 | 0.3499 | -9.0 | -8.0 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -22.55 | 199.44 | 2.07 | 183.90 | 0.4930 | -728.0 | -560.6 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -7.07 | 192.99 | -4.38 | 162.40 | 0.2519 | -862.0 | -718.5 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -13.30 | 191.44 | -5.93 | 163.65 | 0.3588 | -862.0 | -583.8 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -23.77 | 190.52 | -6.85 | 167.85 | 0.5212 | -728.0 | -524.9 | |
| 0.00 | 1.15 | 0.00 | 0.73 | -30.92 | 185.50 | -11.87 | 163.85 | 0.6367 | -45.0 | -89.4 | |
| 0.00 | 1.15 | 0.00 | 0.72 | -29.03 | 184.60 | -12.77 | 161.65 | 0.6160 | -422.0 | -327.4 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -27.36 | 180.65 | -16.73 | 155.34 | 0.6149 | -634.0 | -508.0 | |
| 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. | |