SDO HMI 2014-11-29 15:00:25 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 |
| 134.50 | 635.35 | 90.98 | 430.28 | 3.94 | 161.25 | 42.77 | 274.73 | 0.6813 | -221.8 | -102.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-29 15:00:25 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 |
| 2.56 | 405.17 | 1.82 | 283.56 | 3.16 | 164.16 | 45.68 | 273.35 | 0.7180 | -317.7 | -317.6 | |
| 1.71 | -1.00 | 1.21 | -1.00 | 3.42 | 164.05 | 45.57 | 273.73 | 0.7167 | -224.4 | 999999 | |
| 48.12 | -1.00 | 33.86 | -1.00 | 3.07 | 163.73 | 45.25 | 273.25 | 0.7127 | -1084.2 | 999999 | |
| 12.39 | -1.00 | 8.65 | -1.00 | 3.70 | 163.26 | 44.79 | 274.16 | 0.7072 | -1121.6 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.95 | 1.01 | 162.77 | 44.30 | 270.34 | 0.7006 | -647.0 | -470.1 | |
| 8.29 | -1.00 | 5.71 | -1.00 | 3.89 | 162.48 | 44.01 | 274.47 | 0.6976 | -943.6 | 999999 | |
| 3.08 | -1.00 | 2.11 | -1.00 | 4.25 | 162.26 | 43.79 | 275.00 | 0.6951 | -904.8 | 999999 | |
| 2.05 | -1.00 | 1.40 | -1.00 | 4.61 | 161.80 | 43.32 | 275.56 | 0.6894 | -565.9 | 999999 | |
| 5.98 | -1.00 | 4.07 | -1.00 | 4.38 | 161.65 | 43.18 | 275.23 | 0.6875 | -887.4 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.44 | 3.58 | 161.03 | 42.56 | 274.11 | 0.6791 | -733.0 | -679.7 | |
| 0.00 | 1.11 | 0.00 | 0.75 | 4.62 | 161.02 | 42.55 | 275.64 | 0.6797 | -416.0 | -381.2 | |
| 0.00 | 1.28 | 0.00 | 0.86 | 4.21 | 160.83 | 42.36 | 275.05 | 0.6769 | 207.0 | 112.8 | |
| 0.00 | 1.03 | 0.00 | 0.69 | 4.68 | 160.83 | 42.35 | 275.75 | 0.6772 | -417.0 | -367.5 | |
| 0.00 | 1.11 | 0.00 | 0.75 | 4.33 | 160.80 | 42.33 | 275.23 | 0.6766 | -291.0 | -273.6 | |
| 0.00 | 3.59 | 0.00 | 2.40 | 4.72 | 160.67 | 42.19 | 275.81 | 0.6752 | -776.0 | -578.4 | |
| 0.00 | 1.28 | 0.00 | 0.85 | 3.56 | 160.27 | 41.80 | 274.13 | 0.6693 | 183.0 | 134.4 | |
| 0.00 | 1.54 | 0.00 | 1.02 | 4.54 | 160.25 | 41.78 | 275.60 | 0.6697 | -521.0 | -460.2 | |
| 3.59 | 12.31 | 2.38 | 8.16 | 3.24 | 160.05 | 41.58 | 273.66 | 0.6663 | 789.4 | 245.7 | |
| 0.00 | 0.77 | 0.00 | 0.51 | 4.07 | 160.06 | 41.59 | 274.90 | 0.6669 | 247.0 | 142.6 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 3.78 | 159.96 | 41.49 | 274.47 | 0.6654 | 540.0 | 478.9 | |
| 0.85 | 3.42 | 0.56 | 2.26 | 5.35 | 159.80 | 41.33 | 276.85 | 0.6645 | 637.0 | 434.6 | |
| 0.00 | 0.94 | 0.00 | 0.62 | 5.17 | 159.71 | 41.23 | 276.60 | 0.6631 | -393.0 | -289.5 | |
| 8.55 | 12.99 | 5.62 | 8.55 | 4.52 | 159.54 | 41.06 | 275.63 | 0.6604 | 808.2 | 531.6 | |
| 0.00 | 0.60 | 0.00 | 0.39 | 5.44 | 159.37 | 40.90 | 277.05 | 0.6591 | -646.0 | -518.7 | |
| 0.00 | 1.54 | 0.00 | 1.01 | 5.48 | 159.14 | 40.67 | 277.13 | 0.6560 | -746.0 | -676.1 | |
| 3.50 | 7.09 | 2.29 | 4.63 | 4.77 | 158.97 | 40.49 | 276.06 | 0.6531 | 829.9 | 534.5 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 3.23 | 158.37 | 39.89 | 273.74 | 0.6440 | 547.0 | 496.9 | |
| 3.50 | 10.77 | 2.26 | 6.94 | 4.98 | 158.24 | 39.77 | 276.47 | 0.6437 | -872.9 | -657.8 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 5.46 | 157.89 | 39.42 | 277.27 | 0.6395 | -444.0 | -471.9 | |
| 0.00 | 4.36 | 0.00 | 2.79 | 3.57 | 157.61 | 39.14 | 274.32 | 0.6341 | 570.0 | 428.3 | |
| 0.00 | 1.28 | 0.00 | 0.82 | 3.16 | 157.52 | 39.04 | 273.67 | 0.6325 | 606.0 | 500.3 | |
| 0.00 | 0.51 | 0.00 | 0.33 | 3.75 | 157.20 | 38.73 | 274.64 | 0.6286 | 586.0 | 505.0 | |
| 1.45 | 14.28 | 0.92 | 9.04 | 3.16 | 157.10 | 38.62 | 273.70 | 0.6268 | 747.1 | 702.8 | |
| 0.51 | 9.06 | 0.32 | 5.74 | 3.87 | 156.94 | 38.47 | 274.85 | 0.6252 | 796.3 | 597.2 | |
| 0.00 | 0.77 | 0.00 | 0.49 | 6.19 | 157.03 | 38.56 | 278.53 | 0.6289 | 348.0 | 245.2 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 5.39 | 156.85 | 38.38 | 277.29 | 0.6255 | -90.0 | -69.2 | |
| 0.77 | 98.81 | 0.49 | 62.16 | 5.86 | 156.85 | 38.38 | 278.05 | 0.6261 | 453.3 | 345.0 | |
| 0.00 | 0.85 | 0.00 | 0.54 | 3.64 | 156.52 | 38.04 | 274.52 | 0.6192 | 686.0 | 667.5 | |
| 0.00 | 1.03 | 0.00 | 0.64 | 3.56 | 156.25 | 37.77 | 274.40 | 0.6154 | 655.0 | 634.8 | |
| 0.00 | 2.31 | 0.00 | 1.45 | 4.77 | 156.24 | 37.77 | 276.38 | 0.6164 | 774.0 | 668.9 | |
| 7.52 | -37.00 | 4.72 | -37.00 | 5.49 | 156.18 | 37.71 | 277.54 | 0.6164 | 1001.5 | 999999 | |
| 14.87 | -37.00 | 9.34 | -37.00 | 6.02 | 156.19 | 37.71 | 278.41 | 0.6172 | 864.6 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.91 | 3.65 | 155.91 | 37.44 | 274.58 | 0.6109 | 281.0 | 393.5 | |
| 3.08 | -37.00 | 1.93 | -37.00 | 5.61 | 156.00 | 37.53 | 277.77 | 0.6141 | 1081.4 | 999999 | |
| 0.00 | 3.50 | 0.00 | 2.18 | 3.89 | 155.52 | 37.04 | 275.01 | 0.6056 | 1073.0 | 841.6 | |
| 0.00 | 1.62 | 0.00 | 1.01 | 5.67 | 155.52 | 37.05 | 277.95 | 0.6076 | 914.0 | 740.7 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 4.13 | 155.38 | 36.91 | 275.42 | 0.6039 | 821.0 | 666.9 | |
| 0.00 | 3.33 | 0.00 | 2.07 | 6.15 | 155.22 | 36.75 | 278.79 | 0.6042 | 726.0 | 695.1 | |
| 0.51 | 2.48 | 0.32 | 1.53 | 5.50 | 154.84 | 36.36 | 277.78 | 0.5979 | 828.3 | 712.6 | |
| 0.00 | 2.65 | 0.00 | 1.63 | 5.77 | 154.79 | 36.31 | 278.24 | 0.5976 | 822.0 | 673.5 | |
| 1.62 | 8.12 | 1.00 | 4.99 | 5.45 | 154.54 | 36.06 | 277.73 | 0.5937 | 1024.8 | 808.7 | |
| 0.00 | 2.22 | 0.00 | 1.34 | 4.39 | 153.45 | 34.97 | 276.09 | 0.5770 | 653.0 | 460.8 | |
| 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. | |