The goal for the SAMEX magnetograph's optical system is to accurately measure the polarization state of sunlight in a narrow spectral bandwidth over the field of view of an active region to make an accurate determination of the magnetic field in that region. The instrumental polarization is characterized. The optics and coatings were designed to minimize this spurious polarization introduced by foreoptics. The method developed to calculate the instrumental polarization of the SAMEX optics is described
A major goal of proposed future space observatories, such as the Habitable World Observatory, is to ...
8 pags., 4 figs., 2 tabs. -- EUV and X-ray Optics: Synergy between Laboratory and Space V. -- SPIE O...
Aims. The paper aims are to simulate steady-state distributions of electrons beams precipitating in ...
The 10(exp -5) polarization specification for the Balloon-borne Vector Magnetograph (BVM) can be met...
Context. The impact polarization of optical chromospheric lines in solar flares is still b...
Observations of the four Stokes parameters of a 430 MHz flare from the UV Ceti-type star AD Leonis a...
The degree of linear polarization in solar flares has not yet been precisely determined despite mult...
The activity of the sun can be studied through the measurement of its magnetic field. The measuremen...
We exhibit the effects of Faraday rotation on the direction of the transverse component of the magne...
The coronal magnetic field creates the structure of the corona and is the source of heat and energy ...
Simulation: Vector Vortex Coronagraph Vector vortex retarders (VVR) are halfwave retarders with a s...
The pioneering observational work in solar flare X-ray polarimetry was done in a series of satellite...
The Hanle effect is the modification of the linear polarization parameters of a spectral line due to...
The analysis of the polarization characteristics displayed by optical systems can be divided into tw...
The progressive phases of three solar flares have beenobserv ed with THEMIS in July 2000, using the ...
A major goal of proposed future space observatories, such as the Habitable World Observatory, is to ...
8 pags., 4 figs., 2 tabs. -- EUV and X-ray Optics: Synergy between Laboratory and Space V. -- SPIE O...
Aims. The paper aims are to simulate steady-state distributions of electrons beams precipitating in ...
The 10(exp -5) polarization specification for the Balloon-borne Vector Magnetograph (BVM) can be met...
Context. The impact polarization of optical chromospheric lines in solar flares is still b...
Observations of the four Stokes parameters of a 430 MHz flare from the UV Ceti-type star AD Leonis a...
The degree of linear polarization in solar flares has not yet been precisely determined despite mult...
The activity of the sun can be studied through the measurement of its magnetic field. The measuremen...
We exhibit the effects of Faraday rotation on the direction of the transverse component of the magne...
The coronal magnetic field creates the structure of the corona and is the source of heat and energy ...
Simulation: Vector Vortex Coronagraph Vector vortex retarders (VVR) are halfwave retarders with a s...
The pioneering observational work in solar flare X-ray polarimetry was done in a series of satellite...
The Hanle effect is the modification of the linear polarization parameters of a spectral line due to...
The analysis of the polarization characteristics displayed by optical systems can be divided into tw...
The progressive phases of three solar flares have beenobserv ed with THEMIS in July 2000, using the ...
A major goal of proposed future space observatories, such as the Habitable World Observatory, is to ...
8 pags., 4 figs., 2 tabs. -- EUV and X-ray Optics: Synergy between Laboratory and Space V. -- SPIE O...
Aims. The paper aims are to simulate steady-state distributions of electrons beams precipitating in ...