The quasihysteresis effect in T-T plots of radio spurs between 38, 408 and 1420 MHz.

Astronomy and Astrophysics – Astronomy

Scientific paper

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North Polar Spur: Radio Radiation, North Polar Spur: Methods Of Reduction

Scientific paper

The T-T plots of the North Polar Spur, the Spur in Aquarius, Pegasus and Taurus, using data at 38, 408 and 1420 MHz of the same resolution of 7°25×8°25, reduced to the case of scaled areas, are presented. The T-T graphs for all spurs have shown clear splitting of branches supporting the reality of the quasihysteresis effect. An investigation on the influence of quoted errors on splitting was done. It was shown that the splitting may have astronomical causes. In an attempt to explain this effect the earlier introduced 4V (four vector) model was applied.

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