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Papers by Martin C E Huber

Research paper thumbnail of Recommendations on post focus instrumentation for LEST

Research paper thumbnail of Source standards for the radiometric calibration of astronomical telescopes in the VUV spectral range

Research paper thumbnail of The Century of Space Science, Volume I

Research paper thumbnail of Refractive index of He in the region 920�1910 �

Journal of the Optical Society of America, 1974

Research paper thumbnail of The Ultraviolet Coronagraph Spectrometer

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

Research paper thumbnail of Results and experiences from Apollo and other Lunar missions

Research paper thumbnail of Opening remarks

Research paper thumbnail of Book Review: The century of space science / Kluwer, Dordrecht, 2001, 2 Vols. 1846 pp., ISBN 0-7923-7196-8

Research paper thumbnail of Book review: The century of space science / Johan A. M. Bleeker, Johannes Geiss, Martin C. E. Huber (eds.), Kluwer Academic Publ., Dordrecht, The Netherlands, XIV + 1846 pp., 2001, ISBN 0-7923-7196-8

Journal for the History of Astronomy

Research paper thumbnail of Radiance of Solar Spectral Lines observed with CDS and SUMER on SOHO (CD-ROM Directory: contribs/pauluhn)

Research paper thumbnail of Design and test of a high-resolution EUV spectroheliometer

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 ...

Research paper thumbnail of <title>An Imaging Extreme Ultraviolet Spectrometer For Astrophysical Investigations In Space</title>

Instrumentation in Astronomy VI, 1986

ABSTRACT

Research paper thumbnail of Calibration

Observing Photons in Space, 2013

Research paper thumbnail of UVCS/SOHO capability for determining coronal conditions before, during and after CMEs

Research paper thumbnail of Observations of the Chromospheric Network: Initial Results from the Apollo Telescope Mount

The Astrophysical Journal, 1974

ABSTRACT

Research paper thumbnail of Absolute oscillator strengths for 108 lines of SI I between 163 and 410 nanometers

The Astrophysical Journal, 1987

ABSTRACT

Research paper thumbnail of Transition Probabilities and Their Accuracy

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.

Research paper thumbnail of Hollow Cathode Transfer Standards for the Radiometric Calibration of VUV Telescopes of the Solar and Heliospheric Observatory (SOHO)

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 ...

Research paper thumbnail of Book Review: The century of space science / eds.: Johan A. M. Bleeker Johannes Geiss, Martin C. E. Huber. Kluwer, Dordrecht, 2 Vols., 1846 pp., 2002, ISBN 0-7923-7196-8

Research paper thumbnail of Joint Discussion 6: Sun and Heliosphere — Challenges for Solar-Terrestrial Physics, Magneto- and Hydrodynamics

Highlights of Astronomy, 1995

Research paper thumbnail of Recommendations on post focus instrumentation for LEST

Research paper thumbnail of Source standards for the radiometric calibration of astronomical telescopes in the VUV spectral range

Research paper thumbnail of The Century of Space Science, Volume I

Research paper thumbnail of Refractive index of He in the region 920�1910 �

Journal of the Optical Society of America, 1974

Research paper thumbnail of The Ultraviolet Coronagraph Spectrometer

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

Research paper thumbnail of Results and experiences from Apollo and other Lunar missions

Research paper thumbnail of Opening remarks

Research paper thumbnail of Book Review: The century of space science / Kluwer, Dordrecht, 2001, 2 Vols. 1846 pp., ISBN 0-7923-7196-8

Research paper thumbnail of Book review: The century of space science / Johan A. M. Bleeker, Johannes Geiss, Martin C. E. Huber (eds.), Kluwer Academic Publ., Dordrecht, The Netherlands, XIV + 1846 pp., 2001, ISBN 0-7923-7196-8

Journal for the History of Astronomy

Research paper thumbnail of Radiance of Solar Spectral Lines observed with CDS and SUMER on SOHO (CD-ROM Directory: contribs/pauluhn)

Research paper thumbnail of Design and test of a high-resolution EUV spectroheliometer

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 ...

Research paper thumbnail of <title>An Imaging Extreme Ultraviolet Spectrometer For Astrophysical Investigations In Space</title>

Instrumentation in Astronomy VI, 1986

ABSTRACT

Research paper thumbnail of Calibration

Observing Photons in Space, 2013

Research paper thumbnail of UVCS/SOHO capability for determining coronal conditions before, during and after CMEs

Research paper thumbnail of Observations of the Chromospheric Network: Initial Results from the Apollo Telescope Mount

The Astrophysical Journal, 1974

ABSTRACT

Research paper thumbnail of Absolute oscillator strengths for 108 lines of SI I between 163 and 410 nanometers

The Astrophysical Journal, 1987

ABSTRACT

Research paper thumbnail of Transition Probabilities and Their Accuracy

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.

Research paper thumbnail of Hollow Cathode Transfer Standards for the Radiometric Calibration of VUV Telescopes of the Solar and Heliospheric Observatory (SOHO)

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 ...

Research paper thumbnail of Book Review: The century of space science / eds.: Johan A. M. Bleeker Johannes Geiss, Martin C. E. Huber. Kluwer, Dordrecht, 2 Vols., 1846 pp., 2002, ISBN 0-7923-7196-8

Research paper thumbnail of Joint Discussion 6: Sun and Heliosphere — Challenges for Solar-Terrestrial Physics, Magneto- and Hydrodynamics

Highlights of Astronomy, 1995

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