M. Hof

Continuous Coherent Lyman-αExcitation of Atomic Hydrogen

Miscarriage Among Flight Attendants

Optical clockworks and the measurement of laser frequencies with a mode-locked frequency comb

The pros and cons of ecological risk assessment based on data from different levels of biological organization

FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: COSMOLOGICAL INTERPRETATION

Chemistry of Aerogels and Their Applications

Particle dark matter: evidence, candidates and constraints

Diffuse Continuum Gamma Rays from the Galaxy

NAIRAS aircraft radiation model development, dose climatology, and initial validation

Which fraction of the measured cosmic-ray antiprotons might be due to neutralino annihilation in the galactic halo?

Power Analysis for the NOEC: What is the Probability of Detecting Small Toxic Effects on Three Different Species using the Appropriate Standardized Test Protocols?

What level of effect is a no observed effect?

Prospects for indirect detection of neutralino dark matter

Antiprotons at Solar Maximum

Cosmic ray nuclei, antiprotons and gamma rays in the galaxy: a new diffusion model

Phase Coherent Vacuum-Ultraviolet to Radio Frequency Comparison with a Mode-Locked Laser

The Chemical Composition of the Sun

Forty years of antiprotons

On the reconstruction of Cherenkov rings from aerogel radiators

Continuous Wave Coherent Lyman-αRadiation

Noble Gases in the Solar System

FOLSOMIA CANDIDA(COLLEMBOLA): A “Standard” Soil Arthropod

Perspectives for detection of a higgsino-like relic neutralino

Measurement of the Abundance of Radioactive¹⁰Be and Other Light Isotopes in Cosmic Radiation up to 2 GeV Nucleon⁻¹with the Balloon‐borne Instrument ISOMAX

HOW TO MEASURE NO EFFECT. PART IV: HOW ACCEPTABLE IS THE ECx FROM AN ENVIRONMENTAL POLICY POINT OF VIEW?

The Absolute Flux of Protons and Helium at the Top of the Atmosphere Using IMAX

The Cosmic‐Ray³He/⁴He Ratio from 200 MeV per Nucleon⁻¹to 3.7 GeV per Nucleon⁻¹

Measurement of 0.25–3.2 GeV Antiprotons in the Cosmic Radiation