Connecting the Low to High Corona: Propagating Disturbances as Tracers of the Near-Sun Solar Wind

Abstract

We revisit a quiet 14-day period of solar minimum during January 2008 and track sub-streamer propagating disturbances (PDs) from low heights in STEREO/EUVI to the extended corona through STEREO/COR1 and into STEREO/COR2 along nonradial paths that trace the structure of the underlying streamers. Using our recently developed method for generating nonradial Height-Time profiles of outward PDs (OPDs) and inward PDs (IPDs), we obtained their velocities along the radial and position angle directions. Our analysis of 417 unique OPDs revealed two classes: slow and fast OPDs. Slow OPDs form preferentially at $\approx$1.6 $R_{\odot }$ closer to the streamer boundaries, with asymmetric occurrence rates, and show speeds of $16.4_{-8.4}^{+26.6}km/s$ at 1.5 $R_{\odot }$ and accelerate up to $200.1_{-57.9}^{+71.1}km/s$ at 7.5 $R_{\odot }$. Fast OPDs form preferentially at $\approx$ 1.6 $R_{\odot }$ and at $\approx$3.0 $R_{\odot }$ both at the streamer boundaries and slightly more often within them. They show speeds of $87.8_{-24.8}^{+59.1}km/s$ at 1.5 $R_{\odot }$ up to $197.8_{-46.7}^{+61.8}km/s$ at 7.5 $R_{\odot }$. IPDs are observed forming at $\approx$1.8 $R_{\odot }$ with speeds of tens of $km/s$, mostly concentrated in the aftermath of a CME eruption. We present an example in which we show that periodic brightness variations related to OPDs remained in the range of 98 to 128 min, down to $\approx$2.0 $R_{\odot }$, well within the field of view of COR1. The velocity profiles of slow OPDs for heliocentric height below 3.0 $R_{\odot }$ show good agreement with speeds more closely related to the bulk solar wind obtained via interplanetary scintillation.

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Cited by in corpus (1)

• Statistics of blob properties in two types of coronal streamers