Hostname: page-component-cb9f654ff-plnhv Total loading time: 0.001 Render date: 2025-09-07T02:32:00.437Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic Field Observation with the Solar Flare Telescope

Published online by Cambridge University Press:  12 April 2016

K. Ichimoto ,
T. Sakurai ,
Y. Nishino ,
K. Shinoda ,
M. Noguchi ,
K. Kumagai ,
H. Imai ,
M. Irie ,
M. Miyashita  and
N. Tanaka
...Show all authors
K. Ichimoto
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
T. Sakurai
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
Y. Nishino
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
K. Shinoda
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
M. Noguchi
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
K. Kumagai
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
H. Imai
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
M. Irie
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
M. Miyashita
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
N. Tanaka
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
I. Sano
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
Y. Suematsu
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan
E. Hiei
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, 181, Japan

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 Solar Flare Telescope was constructed at Mitaka in 1989. This instrument comprises four telescopes which respectively observe (a) Hα images, (b) continuum images, (c) vector magnetic fields, and (d) velocity fields in the photosphere. The instrument aims at the study of energy build-up and energy release in solar flares, in cooperation with the Solar-A satellite. The whole system has been in regular operation since 1992 July. The methods of measuring the magnetic and velocity fields are described.

Information

Type
Session 3. Techniques of Magnetic Field Measurements
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 166 - 169
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Ichimoto, K., Sakurai, T., Yamaguchi, A., Kumagai, K., Nishino, Y., Suematsu, Y., Hiei, E., and Hirayama, T.: 1991, Lecture Notes in Physics, 387, 320 Google Scholar
Hohveger, H., and Muller, E.A.: 1974, Solar Phys., 35, 11 Google Scholar
Unno, W.: 1956, Publ.Astron.Soc.Japan, 8, 108 Google Scholar
Wittmann, A.: 1974, Solar Phys., 35, 11 Google Scholar