Meteorological Condition for Submillimeter Observations in Sendai

スポンサーリンク

概要

• 論文の詳細を見る

• Atmospheric transmittance at a submillimeter wavelength is investigated from meteorological data. The astronomical observations are possible in a period from January to March for each year in Sendai, and 22 days (24% in the period) are in good conditions. The good transmittance frequently occurs in the conditions of a low temperature, a low vapor pressure, and a strong wind on the surface of the earth.Atmospheric transmittancesubmillimeter wavelengthwater vapor

• 東北大学の論文
• 1987-03-20

著者

• Kameya Osamu

  Astronomical Institute Faculty Of Science Tohoku University

• Takeuti Mine

  Astronomical Institute Tohoku University

• TAKAKUBO Keiya

  Astronomical Institute, Faculty of Science, Tohoku University

• Takakubo Keiya

  Astronomical Institute Faculty Of Science Tohoku University

関連論文

• Measurement of Stellar Mass by Pulsar Timing Observation(Massive Astrophysical Compact Halo Objects)
• Thermal Instability of Hydrogen-Burning Shell in Very Massive Stars
• Linear Pulsation Properties of the Proto-Planetary-Nebula Stars(Proceedings of the Workshop on the Hydrodynamic Study of Accretion Disks and Pulsating Stars)
• Effect of Irradiation on the Disk of the Epsilon Aurigae System
• Meteorological Condition for Submillimeter Observations in Sendai
• Hydrogen Emission Profiles at Positive Latitudes : II. On the Warm HI Component of the Interstellar Medium
• Hydrodynamic Models of Classical Cepheids. : I. A Technique to Search the Limiting-amplitude Oscillation
• Nonlinear Properties of a Self-Exciting Oscillator
• Resonance Phenomenon in Classical Cepheids
• Revision of Pulsation Properties of Yellow Bright Stars
• A Remark on the nature of RV Tauri Stars(Proceedings of the Workshop on the Hydrodynamic Study of Accretion Disks and Pulsating Stars)
• Hydrodynamic Study of a Proto-Planetary-Nebula Star(Proceedings of the Workshop on the Hydrodynamic Study of Accretion Disks and Pulsating Stars)
• Vertical Instability of One-Zone Accretion Disks(Proceedings of the Workshop on the Hydrodynamic Study of Accretion Disks and Pulsating Stars)
• Preface(Proceedings of the Workshop on the Hydrodynamic Study of Accretion Disks and Pulsating Stars)
• Comment on an Enigmatic Star, UU Her(Proceedings of the Workshop on the Activities and Ejecta of Supergiant Stars)
• Spectroscopic observations of F supergiant stars and a summary of related data(Proceedings of the Workshop on the Activities and Ejecta of Supergiant Stars)
• Preface(Proceedings of the Workshop on the Activities and Ejecta of Supergiant Stars)
• Workshop on Irregular Stellar Pulsation at Mizusawa
• Derivation of the Modal Coupling Coefficients of a Classical Cepheid Model
• Effect of Helium Enrichment in a Classical Cepheid Model
• The Steady Accretion Discs Irradiated by the Central Neutron Star
• Note on a Hydrodynamic Model of FG Sge
• Note on Intermittent Bursts of a Hydrodynamic Model
• Hydrodynamic Models of Classical Cepheids. II. Two-mode Resonance
• On Linear Nonadiabatic Pulsations of Yellow Bright Stars
• The Characteristic of the Large-amplitude Pulsation in a Model Yellow Supergiant Star
• VLBI Astrometry of the Semiregular Variable RX Bootis

もっと見る 閉じる

スポンサーリンク