Publication
Stratification of the 5-min oscillation through the solar photosphere
Not Available
-
-
PublicationStructure and Dynamics of the Sun's Interior Revealed by the Helioseismic and Magnetic ImagerHigh-resolution helioseismology observations with the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) provide a unique three...
-
PublicationStudies of the Solar Chromosphere from Millimeter to Sub-Millimeter Observations. I: Isophotometric MappingAbstract image available at: http://adsabs.harvard.edu/abs/1973SoPh...29...25B
-
PublicationStudies of the Solar Chromosphere from Millimetre and Sub-Millimetre Observations. II: Simple Models of the Lower ChromosphereAbstract image available at: http://adsabs.harvard.edu/abs/1973SoPh...31..319B
-
PublicationSUNRISE III: Overview of Observatory and InstrumentsIn July 2024, SUNRISE completed its third successful science flight. The SUNRISE III observatory had been upgraded significantly after the two previous...
-
PublicationTaiwan Oscillation NetworkThe Taiwan Oscillation Network (TON) is a ground-based network to measure solar intensity oscillations to study the internal structure of the Sun. K-line full...
-
PublicationThe density matrix approach to polarized radiative transferThe density matrix approach to polarized radiative transfer is reviewed, with particular emphasis on the physical assumptions that are at the basis of the...
-
PublicationThe Dynamics of the Solar Radiative ZoneThe dynamics of the solar radiative interior are still poorly constrained by comparison to the convective zone. This disparity is even more marked when we...
-
PublicationThe Filter Imager SuFI and the Image Stabilization and Light Distribution System ISLiD of the Sunrise Balloon-Borne Observatory: Instrument DescriptionWe describe the design of the Sunrise Filter Imager (SuFI) and the Image Stabilization and Light Distribution (ISLiD) unit onboard the Sunrise balloon borne...