On the detection of solar coronal high-velocity fields using the XUV Doppler Telescope

Publications of the Astronomical Society of Japan

Volumn 52, Issue 6, 2000, Pages 1165-1174

  Kobayashi, Ken ^a   Hara, Hirohisa ^b   Kano, Ryohei ^b   Nagata, Shin'ichi ^a   Sakao, Taro ^b   Shimizu, Toshifumi ^b   Tsuneta, Saku ^b   Yoshida, Tsuyoshi ^a   Harrison, Richard ^c  

^a UNIVERSITY OF TOKYO   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c RUTHERFORD APPLETON LABORATORY   (United Kingdom)

Author keywords

Sun: atmospheric motions; Sun: corona; Sun: X rays

Indexed keywords

DOPPLER EFFECT; PLASMA DIAGNOSTICS; ROCKETS; TELESCOPES; VELOCITY;

ATMOSPHERIC MOTIONS; DOPPLER; EMISSION LINES; HIGH VELOCITY; NORMAL INCIDENCE; SOLAR CORONA; SUN : CORONA; SUN: ATMOSPHERIC MOTION; SUN:X-RAYS; VELOCITY FIELD; BAND PASS; SUN: ATMOSPHERE;

ELECTROMAGNETIC WAVE EMISSION;

EID: 0034549178     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/52.6.1165     Document Type: Article

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