IVM Magnetograms

Each magnetogram is a 168 kbyte GIF image. Celestial north is at the top; east is at the left. The magnetogram is displayed as four panels:

Continuum brightness
This is in arbitrary units, but on a linear scale.
Line-of-sight component of magnetic field
Projection of magnetic field vector onto the line between the solar feature and the observer. The units are Gauss. The color changes linearly with the cube root of the field strength, to better show both strong and weak features. Thus if the top of the scale is 1000 = 10^3, the midpoint is 5^3 or 125.
Transverse component of magnetic field
Magnitude of the projection of the field vector onto the plane perpendicular to the line of sight. The units are Gauss; cube-root scaling is used here too.
Direction of transverse component
The orientation of the transverse component is indicated by the pixel color, as in the key wheel at the lower left. Note that there is a 180-degree ambiguity in the direction: the polarization data does not tell us whether the field vector points to the right or to the left.


AR0035_20020726.1712_ivm
AR0035_20020726.1712_ivm
AR0037_20020726.1650_ivm
AR0037_20020726.1650_ivm
AR0038_20020726.1634_ivm
AR0038_20020726.1634_ivm
AR0039_20020726.1656_ivm
AR0039_20020726.1656_ivm
AR0040_20020726.1707_ivm
AR0040_20020726.1707_ivm
AR0041_20020726.1644_ivm
AR0041_20020726.1644_ivm
AR0042_20020726.1701_ivm
AR0042_20020726.1701_ivm
AR0043_20020726.1629_ivm
AR0043_20020726.1629_ivm
AR0045_20020726.1639_ivm
AR0045_20020726.1639_ivm

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