Properties of high-latitude CME-driven disturbances during Ulysses second northern polar passage

被引:39
作者
Reisenfeld, DB
Gosling, JT
Forsyth, RJ
Riley, P
St Cyr, OC
机构
[1] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[2] Imperial Coll Space & Atmospher Phys, Blackett Lab, London SW7 2BW, England
[3] Sci Applicat Int Corp, San Diego, CA 92121 USA
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20770 USA
关键词
CORONAL MASS EJECTIONS; SOLAR-WIND; MISSION; SHOCK;
D O I
10.1029/2003GL017155
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Ulysses observed five coronal mass ejections (CMEs) and their associated disturbances while the spacecraft was immersed in the polar coronal hole (CH) flow above 70degrees N in late 2001. Of these CMEs, two were very fast (>850 km s(-1)) driving strong shocks in the wind ahead, and two others were over-expanding. The two fast CMEs were observed leaving the Sun by LASCO/SOHO, and were observed in the ecliptic by Genesis and ACE. These were large events, spanning at least from the northern heliospheric pole to the ecliptic. One-dimensional hydrodynamic simulations indicate that these could be described as overpressured CMEs launched from the Sun at speeds initially faster than ambient, but then decelerating to the ambient solar wind speed as they propagated outward. The two over-expanding CMEs mark their first occurrence since Ulysses' first orbit when such CMEs were only observed in polar CH flow.
引用
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页码:ULY5 / 1
页数:4
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