Martin C E Huber - Academia.edu (original) (raw)
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Papers by Martin C E Huber
Journal of the Optical Society of America, 1974
Lecture Notes in Physics, 1995
The Ultraviolet Coronagraph Spectrometer (UVCS) is an instrument onboard the Solar and Heliospher... more The Ultraviolet Coronagraph Spectrometer (UVCS) is an instrument onboard the Solar and Heliospheric (SOHO) spacecraft, a joint ESA/NASA mission to be launched in 1995. The UVCS will provide ultraviolet spectroscopic measurements to determine the primary plasma parameters of the solar corona (temperatures, densities, velocities), from its base to as high as 10 R. We review briefly, here, its science objectives
Journal for the History of Astronomy
SPIE Proceedings, 1992
The HiRES High-Resolution EUV Spectroheliometer is a sounding rocket instrument yielding very hig... more The HiRES High-Resolution EUV Spectroheliometer is a sounding rocket instrument yielding very high spatial, spectral, and temporal resolution images of the solar outer atmosphere, on the basis of a 45-cm Gregorian telescope feeding a normal-incidence stigmatic EUV ...
Instrumentation in Astronomy VI, 1986
ABSTRACT
Observing Photons in Space, 2013
The Astrophysical Journal, 1974
ABSTRACT
The Astrophysical Journal, 1987
ABSTRACT
Physica Scripta, 1980
The classical methods for measuring transition probabilities, viz. the determination of lifetimes... more The classical methods for measuring transition probabilities, viz. the determination of lifetimes and branching ratios, and the absorption, hook, and emission techniques are briefly reviewed. The main advantages and difficulties of each method, as well as the accuracies reached, are described. Improved evaluation methods for hook spectrograms are summarized and the advances made with combinations of classical methods for determining and assessing oscillator strengths are described. The hitherto rarely exploited potential of magneto-rotation measurements for deriving accurate oscillator strengths and the promise of optogalvanic spectroscopy are mentioned. Applications of non-linear optical methods for f-value determinations are also discussed.
Metrologia, 1993
... On board the ESA/NASA space mission SOHO (Solar and Heliospheric Observatory) there will be s... more ... On board the ESA/NASA space mission SOHO (Solar and Heliospheric Observatory) there will be several VUV telescope/spectrometer systems to observe the solar disk and its corona in the wavelength range 15 nm to 160 nm. ... J. Hollandt and M. Kuhne: Physikalisch-Technishe ...
Highlights of Astronomy, 1995
Journal of the Optical Society of America, 1974
Lecture Notes in Physics, 1995
The Ultraviolet Coronagraph Spectrometer (UVCS) is an instrument onboard the Solar and Heliospher... more The Ultraviolet Coronagraph Spectrometer (UVCS) is an instrument onboard the Solar and Heliospheric (SOHO) spacecraft, a joint ESA/NASA mission to be launched in 1995. The UVCS will provide ultraviolet spectroscopic measurements to determine the primary plasma parameters of the solar corona (temperatures, densities, velocities), from its base to as high as 10 R. We review briefly, here, its science objectives
Journal for the History of Astronomy
SPIE Proceedings, 1992
The HiRES High-Resolution EUV Spectroheliometer is a sounding rocket instrument yielding very hig... more The HiRES High-Resolution EUV Spectroheliometer is a sounding rocket instrument yielding very high spatial, spectral, and temporal resolution images of the solar outer atmosphere, on the basis of a 45-cm Gregorian telescope feeding a normal-incidence stigmatic EUV ...
Instrumentation in Astronomy VI, 1986
ABSTRACT
Observing Photons in Space, 2013
The Astrophysical Journal, 1974
ABSTRACT
The Astrophysical Journal, 1987
ABSTRACT
Physica Scripta, 1980
The classical methods for measuring transition probabilities, viz. the determination of lifetimes... more The classical methods for measuring transition probabilities, viz. the determination of lifetimes and branching ratios, and the absorption, hook, and emission techniques are briefly reviewed. The main advantages and difficulties of each method, as well as the accuracies reached, are described. Improved evaluation methods for hook spectrograms are summarized and the advances made with combinations of classical methods for determining and assessing oscillator strengths are described. The hitherto rarely exploited potential of magneto-rotation measurements for deriving accurate oscillator strengths and the promise of optogalvanic spectroscopy are mentioned. Applications of non-linear optical methods for f-value determinations are also discussed.
Metrologia, 1993
... On board the ESA/NASA space mission SOHO (Solar and Heliospheric Observatory) there will be s... more ... On board the ESA/NASA space mission SOHO (Solar and Heliospheric Observatory) there will be several VUV telescope/spectrometer systems to observe the solar disk and its corona in the wavelength range 15 nm to 160 nm. ... J. Hollandt and M. Kuhne: Physikalisch-Technishe ...
Highlights of Astronomy, 1995