SDO HMI 2014-10-03 14:00:32 UT
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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.26 | 92.69 | 11.80 | 49.49 | -12.38 | 160.84 | 10.18 | 207.70 | 0.3698 | -90.6 | -35.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-10-03 14:00:32 UT
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 | 1.93 | 0.00 | 1.18 | -21.83 | 173.07 | 22.41 | 217.10 | 0.5889 | 644.0 | 496.8 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -9.32 | 167.63 | 16.97 | 226.93 | 0.3960 | 820.0 | 685.3 | |
| 0.00 | 3.34 | 0.00 | 1.82 | -11.48 | 167.62 | 16.96 | 223.12 | 0.4201 | 586.0 | 651.1 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -11.77 | 167.64 | 16.98 | 222.68 | 0.4236 | 699.0 | 603.3 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -10.30 | 166.16 | 15.50 | 222.54 | 0.3905 | 630.0 | 536.5 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -13.87 | 166.05 | 15.39 | 216.70 | 0.4329 | 684.0 | 549.1 | |
| 0.53 | 1.76 | 0.28 | 0.94 | -10.32 | 163.67 | 13.01 | 217.57 | 0.3649 | -785.0 | -681.5 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -23.69 | 164.61 | 13.96 | 203.78 | 0.5499 | 650.0 | 512.5 | |
| 0.00 | 2.46 | 0.00 | 1.31 | -11.79 | 162.08 | 11.42 | 211.75 | 0.3698 | 1008.0 | 836.5 | |
| 0.00 | 2.81 | 0.00 | 1.50 | -12.29 | 162.03 | 11.38 | 210.94 | 0.3764 | 687.0 | 670.2 | |
| 2.64 | 20.67 | 1.41 | 11.00 | -12.04 | 161.90 | 11.24 | 211.00 | 0.3717 | 938.2 | 836.9 | |
| 5.80 | -11.00 | 3.09 | -11.00 | -11.84 | 161.51 | 10.86 | 210.41 | 0.3658 | 999.5 | 999999 | |
| 0.00 | 3.08 | 0.00 | 1.63 | -11.31 | 160.50 | 9.84 | 208.73 | 0.3502 | 764.0 | 565.8 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -11.68 | 160.08 | 9.42 | 207.19 | 0.3523 | 773.0 | 558.1 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -13.29 | 159.79 | 9.13 | 204.52 | 0.3739 | -497.0 | -460.8 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -13.38 | 159.48 | 8.82 | 203.69 | 0.3732 | -698.0 | -453.5 | |
| 3.96 | 9.59 | 2.08 | 5.04 | -10.93 | 159.06 | 8.41 | 205.57 | 0.3340 | -886.4 | -679.6 | |
| 0.88 | 22.69 | 0.47 | 12.03 | -12.80 | 158.90 | 8.24 | 202.91 | 0.3607 | -724.9 | -697.7 | |
| 0.35 | -17.00 | 0.18 | -17.00 | -11.12 | 158.82 | 8.16 | 204.69 | 0.3350 | -1089.8 | 999999 | |
| 4.49 | -18.00 | 2.38 | -18.00 | -12.51 | 158.83 | 8.17 | 203.06 | 0.3559 | -1014.3 | 999999 | |
| 2.64 | -18.00 | 1.40 | -18.00 | -12.32 | 158.73 | 8.07 | 203.02 | 0.3524 | -1100.0 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -12.00 | 158.72 | 8.07 | 203.36 | 0.3476 | -999.0 | -823.2 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -11.24 | 158.64 | 7.98 | 204.05 | 0.3356 | 418.0 | 232.4 | |
| 0.97 | 8.09 | 0.51 | 4.26 | -11.71 | 158.53 | 7.87 | 203.19 | 0.3420 | -1154.6 | -862.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -11.77 | 158.28 | 7.63 | 202.47 | 0.3413 | -657.0 | -562.5 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -13.77 | 158.28 | 7.62 | 200.37 | 0.3718 | -736.0 | -689.9 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -15.12 | 157.95 | 7.29 | 198.37 | 0.3905 | -564.0 | -593.5 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -14.02 | 157.48 | 6.82 | 198.16 | 0.3712 | -633.0 | -489.0 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -15.40 | 157.49 | 6.83 | 197.06 | 0.3926 | -661.0 | -551.2 | |
| 0.00 | 0.62 | 0.00 | 0.33 | -13.82 | 157.22 | 6.57 | 197.69 | 0.3669 | -831.0 | -684.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |