Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-30T10:46:56.515Z Has data issue: false hasContentIssue false
  • English
  • Français

EUV Observation with Normal Incidence Multilayer Telescopes

Published online by Cambridge University Press:  12 April 2016

Hideyo Kunieda ,
Koujun Yamashita ,
Takashi Yamazaki ,
Kazuaki Ikeda ,
Kazutami Misaki ,
Yoshiyuki Takizawa ,
Masato Nakamura ,
Ichiro Yoshikawa  and
Asami Yamaguchi
Hideyo Kunieda
Affiliation:
Department of Physics, Nagoya University, Nagoya 464-01
Koujun Yamashita
Affiliation:
Department of Physics, Nagoya University, Nagoya 464-01
Takashi Yamazaki
Affiliation:
Department of Physics, Nagoya University, Nagoya 464-01
Kazuaki Ikeda
Affiliation:
Department of Physics, Nagoya University, Nagoya 464-01
Kazutami Misaki
Affiliation:
Department of Physics, Nagoya University, Nagoya 464-01
Yoshiyuki Takizawa
Affiliation:
Department of Earth and Planetary Physics, University of Tokyo, Tokyo 113
Masato Nakamura
Affiliation:
Department of Earth and Planetary Physics, University of Tokyo, Tokyo 113
Ichiro Yoshikawa
Affiliation:
Department of Earth and Planetary Physics, University of Tokyo, Tokyo 113
Asami Yamaguchi
Affiliation:
National Astronomical Observatory, Mitaka 181

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The EUV emission from hot interstellar plasmas is observed by normal incidence telescopes on board a sounding rocket. It was performed on January 29, 1995, to observe the sky area around the HZ 43 close to the north galactic pole. The wave bands (δλ ~ 10 Å) are provided at 130 and 170 Å by the multilayer coating on the reflectors of 20 cm in diameter and of 30 cm in focal length. The focal plane images are detected by Csl coated MCP’s. The observed flux of HZ 43 is 1.5 counts s−1 at 130 Å and 3 counts s−1 at 170 Å. The diffuse emission is 27 c/s/deg2 at 130 Å and 20 c/s/deg2 at 170 Å. Those preliminary numbers are subjects to change along with the data analysis.

Type
I. Summaries of Recent Missions
Information
International Astronomical Union Colloquium , Volume 152: Astrophysics in the Extreme Ultraviolet , 1996 , pp. 21 - 26
Copyright
Copyright © Kluwer 1996

References

Kato, T. 1976, Radiation from Hot Thin Plasmas from 1 to 250 Å, ApJS, 30, 397 Google Scholar