A Compact, Ultra-High Resolution VIPA Spectrograph for Solar Spectroscopic Observations: Astrocomb Characterization and First Light

Abstract

We present a compact, high spectral resolution prototype spectrograph based on a Virtually Imaged Phased Array (VIPA), which is designed for solar spectral observations. This fiber-fed instrument has a size of only 53 $\times$ 20 $\times$ 18 cm${}^3$. Wavelength calibration using an astrocomb ($f_{\text{rep}}=25$ GHz) established an operational bandpass of 592.76--657.07 nm and revealed an asymmetric instrumental profile. A Fano-Lorentz product function provides a significantly better fit to this profile than a Gaussian. The measured spectral resolution ranges between 290,000 and 340,000 across the band. Initial on-sky validation at the New Vacuum Solar Telescope (NVST, Yunnan Observatories) successfully demonstrated the prototype's capabilities: clear detection of solar five-minute oscillations ($\pm 300{\text{m s}}^{-1}$) in the \ion {Fe}{1} 6280.57 Ã ~ line, resolution of magnetic broadening in sunspots using the \ion{Fe}{1} 6173.34 Ã ~ line, and the first ground-based definitive identification of the faint \ion{Si}{1} 6560.57 Ã ~ line within the H$\hat{I}\pm$ band. These results validate the VIPA as a promising platform for high spectral resolution solar spectroscopy. Its compact design and performance directly support future applications in multi-object solar studies, high spectral resolution observations for time-domain astronomy, including exoplanet detection, and potential space-borne instrumentation.