Observations of pores and surrounding regions with CO 4.66 μm lines by BBSO/CYRA

Solar observations of carbon monoxide (CO) indicate the existence lower-temperature gas in lower solar chromosphere. We present an observation pores, and quiet-Sun, network magnetic field regions with CO 4.66 {\mu}m lines by Cryogenic Infrared Spectrograph (CYRA) at Big Bear Observatory. used strong around to understand properties thermal structures atmosphere different features various strengths. AIA 1700 {\AA} images, HMI continuum images magnetograms are also included observation. The data from 3D radiation magnetohydrodynamic (MHD) simulation Bifrost code employed for first time be compared RH synthesize line profiles regions. 3-2 R14 center intensity changes either enhanced or diminished increasing strength, which should caused heating effects flux tubes sizes. find several "cold bubbles" can classified into two types. One type is located quiet-Sun without fields. other type, has rarely been reported past, near surrounded Notably, some edge network. kinds cold bubbles relationship between bubble intensities strength both reproduced MHD codes. shows that there a plasma blob fields, causing observed seen image. Our illustrate plays vital role generation bubbles.