The QuickPUNCH Project: Polarimeter to Unify the Heliosphere and Corona (PUNCH) Observations for Space Weather Operations and Research

Daniel
Seaton
Southwest Research Institute
Matthew J. West, ESA ESTEC
J. Marcus Hughes, SwRI
Craig E. DeForest, SwRI
Sarah E. Gibson, NCAR
Derek Lamb, SwRI
Chris Lowder, SwRI
Ritesh Patel, SwRI
Jillian Redfern, SwRI
Samuel Van Kooten, SwRI
Adedoja Adeyeye, NOAA NCCF
Michael Burek, CIRES/NOAA SWPC
Gabriel Dima, CIRES/NOAA NCEI
Jeff Johnson, CIRES/NOAA SWPC
Timothy Meisenhelder, NOAA NCCF
Mark Middlebusher, NOAA NCCF
George Millward, CIRES/NOAA SWPC
Donald Schmit, CIRES/NOAA NCEI
Nai-Yu Wang, NOAA SWO
Poster
PUNCH is a coronagraphic and heliospheric imaging NASA Small Explorer comprising of four spacecraft: three Wide Field Imagers (WFI) and one Near Field Imager (NFI), which generates polarization-resolved observations of the corona and heliosphere between 6–180 solar radii. In addition to its science mission, PUNCH makes low-latency observations of the corona and heliosphere that can support space weather forecasting operations: the QuickPUNCH project, whose initial goal is to develop and demonstrate the required data products, pipeline, and low-latency capabilities.

We describe the space weather applications for QuickPUNCH observations, including tracking coronal mass ejections (CMEs) and solar wind outflow. We discuss the specific low-latency QuickPUNCH data products for space weather, PUNCH’s more general science products, and end-user data access. We provide an overview of research-to-operations opportunities provided by these data, including the uses of polarized coronal measurements for space weather, tracing of CMEs in 3D, and the use of PUNCH data as a constraint for numerical forecasting models. We conclude with a look at recent PUNCH science data and their potential to revolutionize forecasting by tracking CMEs in 3-D as they traverse the inner solar system.
Poster session day
Poster location
32