Interplanetary magnetic correlation and low-frequency spectrum over many solar rotations

Fluctuations and structure across a wide range of spatial and temporal scales are frequently studied in the solar wind. The properties of the low-frequency fluctuations are of relevance to turbulent energy injection into the plasma and the transport of high-energy cosmic rays. Correlation analysis of decade-long intervals of interplanetary data permits study of fluctuations at time scales much longer than suitably defined correlation times, and therefore at frequencies well below those associated with the Kolmogorov inertial range of in situ turbulence. At the frequencies of interest, we study the familiar occurrence of the [Formula: see text] spectral signature. We also study point spectral features due to solar rotation and their relation with the [Formula: see text] signal. We report properties at timescales ranging from minutes up to years, using data selected by wind speed, phase of solar cycle, and cartesian components of the magnetic field. A surprising finding is that the power in solar rotation harmonics is consistent with an extension of the [Formula: see text] spectrum, down to frequencies as low as around [Formula: see text]. The presence of a broadband [Formula: see text] spectrum across different wind types supports the interpretation that [Formula: see text] signals may be related to or even originate from the solar dynamo.