Image Details
Caption: Figure 15.
Showing STEC (left panel) and IFRM (right panel) estimates using data from the closest three GNSS stations to the VLA for the VLA D2 observation. Only the “pie1” station (blue traces) has known receiver bias values. Use of the data from the other two stations results in improbable, or impossible, estimates of the STEC and IFRM.
© 2026. The Author(s). Published by the American Astronomical Society.