High - resolution observations are presented based on direct imaging, two - dimensional spectropolarimetry with Fabry - Pérot interferometers, and scanning long - slit spectrographs to introduce some of the science cases for high - resolution solar physics: (1) statistical properties of flows in and around pores and sunspots, (2) chromospheric dynamics associated with newly emerging flux, and (3) flare diagnostics from near - infrared spectropolarime
High - resolution observations are presented based on direct imaging, two - dimensional spectropolarimetry with Fabry - Pérot interferometers, and scanning long - slit spectrographs to introduce some of the science cases for
high - resolution solar physics: (1) statistical properties of flows in and around pores and sunspots, (2) chromospheric dynamics associated with newly emerging flux, and (3) flare diagnostics from near - infrared spectropolarime
high - resolution solar physics: (1) statistical properties of flows in and around pores and sunspots, (2) chromospheric dynamics
associated with newly emerging
flux, and (3) flare diagnostics from near - infrared spectropolarimetry.
The
highest values of the uncertainties
associated with the interpolation / extrapolation into unsampled grid boxes are found in subpolar latitudes of both hemispheres for the turbulent
fluxes, where they can be comparable with the sampling errors.
The US CLIVAR
High Latitude Surface
Flux Working Group was formed in January 2008, with the particular goal of addressing some of the challenges
associated with air - sea and air - ice - ocean exchanges in Arctic, Antarctic, and Southern Ocean regions.