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 |
| 82.06 | 466.39 | 41.16 | 233.87 | -1.45 | 153.96 | 3.30 | 202.03 | 0.1536 | 767.3 | 430.0 | |
|
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 |
| 0.26 | 347.50 | 0.13 | 174.37 | -1.37 | 155.24 | 4.58 | 210.04 | 0.1603 | 1176.0 | 452.7 | |
| 54.97 | -1.00 | 27.58 | -1.00 | -1.54 | 154.79 | 4.13 | 207.02 | 0.1593 | 1411.1 | 999999 | |
| 4.13 | -1.00 | 2.07 | -1.00 | -1.44 | 153.71 | 3.05 | 200.85 | 0.1501 | 1098.9 | 999999 | |
| 6.60 | -1.00 | 3.31 | -1.00 | -1.74 | 153.50 | 2.84 | 198.87 | 0.1538 | 1022.9 | 999999 | |
| 0.97 | 2.20 | 0.49 | 1.11 | -2.84 | 153.44 | 2.78 | 196.48 | 0.1715 | 909.5 | 734.5 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -2.26 | 153.38 | 2.72 | 197.14 | 0.1616 | 916.0 | 772.6 | |
| 0.00 | 1.67 | 0.00 | 0.84 | -2.47 | 153.32 | 2.66 | 196.41 | 0.1649 | 685.0 | 643.8 | |
| 0.00 | 1.14 | 0.00 | 0.57 | -2.68 | 153.14 | 2.48 | 195.02 | 0.1675 | 817.0 | 639.9 | |
| 5.54 | 41.60 | 2.77 | 20.82 | -1.14 | 153.11 | 2.45 | 197.64 | 0.1417 | 1214.0 | 490.5 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -1.74 | 153.11 | 2.45 | 196.43 | 0.1517 | 624.0 | 482.8 | |
| 2.11 | -9.00 | 1.06 | -9.00 | -0.92 | 152.99 | 2.33 | 197.27 | 0.1375 | 1024.9 | 999999 | |
| 0.53 | 1.58 | 0.27 | 0.80 | -2.62 | 152.93 | 2.27 | 193.88 | 0.1656 | 877.3 | 736.3 | |
| 2.37 | 33.77 | 1.19 | 16.86 | -0.38 | 152.48 | 1.82 | 194.67 | 0.1260 | 1203.9 | 752.4 | |
| 0.53 | -13.00 | 0.26 | -13.00 | -0.32 | 152.30 | 1.64 | 193.38 | 0.1242 | 906.5 | 999999 | |
| 0.00 | 2.99 | 0.00 | 1.50 | -2.31 | 152.06 | 1.40 | 188.95 | 0.1574 | 1134.0 | 932.6 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 0.11 | 152.06 | 1.40 | 192.21 | 0.1161 | 908.0 | 721.3 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -2.74 | 151.97 | 1.31 | 188.01 | 0.1644 | -534.0 | -436.1 | |
| 0.00 | 1.67 | 0.00 | 0.84 | -2.34 | 151.70 | 1.04 | 186.65 | 0.1571 | 821.0 | 538.7 | |
| 0.62 | 2.11 | 0.31 | 1.06 | -2.83 | 151.67 | 1.01 | 186.13 | 0.1654 | -846.4 | -699.2 | |
| 0.00 | 1.14 | 0.00 | 0.57 | -2.37 | 151.49 | 0.83 | 185.30 | 0.1572 | 817.0 | 591.3 | |
| 0.70 | 2.20 | 0.35 | 1.10 | 0.02 | 151.19 | 0.53 | 184.62 | 0.1154 | -826.1 | -635.0 | |
| 0.00 | 1.93 | 0.00 | 0.96 | 0.29 | 151.01 | 0.35 | 183.19 | 0.1104 | -790.0 | -672.9 | |
| 0.00 | 1.58 | 0.00 | 0.79 | 0.14 | 150.92 | 0.26 | 182.32 | 0.1130 | -826.0 | -716.6 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 0.29 | 150.74 | 0.08 | 180.74 | 0.1103 | -1032.0 | -827.3 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -2.28 | 150.08 | -0.58 | 176.23 | 0.1553 | -827.0 | -622.0 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -0.07 | 149.93 | -0.73 | 173.74 | 0.1172 | -998.0 | -768.4 | |
| 0.00 | 1.58 | 0.00 | 0.79 | -1.52 | 149.66 | -1.00 | 172.95 | 0.1428 | -901.0 | -705.6 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -2.13 | 149.48 | -1.18 | 172.26 | 0.1537 | -889.0 | -678.7 | |
| 2.73 | 4.66 | 1.37 | 2.34 | -3.04 | 148.96 | -1.69 | 169.99 | 0.1706 | -1058.0 | -792.9 | |
| 0.00 | 3.25 | 0.00 | 1.63 | -1.46 | 148.82 | -1.84 | 167.09 | 0.1443 | -923.0 | -778.8 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -1.22 | 148.73 | -1.93 | 166.08 | 0.1406 | -831.0 | -664.7 | |
| 0.00 | 3.34 | 0.00 | 1.68 | -3.44 | 148.12 | -2.54 | 165.76 | 0.1804 | 868.0 | 671.6 | |
| 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. | |