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GEOPHYSICAL RESEARCH LETTERS,
VOL. 32,
L14106,
doi:10.1029/2005GL023056,
2005
Interplanetary shocks unconnected with earthbound coronal mass ejections
T. A. Howard
School of Physics and Astronomy, University of Birmingham, Edgbaston, UK
S. J. Tappin
School of Physics and Astronomy, University of Birmingham, Edgbaston, UK
Abstract
An associated study by Howard and Tappin (2005) identified 7 Earthbound forward shocks (of which 3 were geoeffective) which
were not connected with any detectable coronal mass ejection activity along the Sun-Earth line. This largely unexplored result
lends evidence to the fact that some large interplanetary transients are not detected by coronagraphs. This letter explores
two possibilities for the formation of the interplanetary foreward shock, namely Corotating Interaction Regions (CIR) or Erupting
Magnetic Structures (EMS). Data from EPAM, SWEPAM and MAG on board ACE provided details of the interplanetary shock and associated
energetic ions along the Sun-Earth line, while evidence of magnetic field reorientation at the Sun was investigated using
EIT on board SOHO, the GOES network and ground-based Hα and radio telescopes. No evidence was found to associate 6 of the
shocks with CIRs, although we were uncertain about one event, and in each case evidence of chromospheric activity at the Sun
was detected between the estimated onset time of the transient and the arrival of the shock at ACE. The nature of this surface
activity included X-Ray (≥C5.0) and Hα flares, associated Type III and Type II radio bursts and disappearing filaments. These
results lead to the proposal that EMS are the likely source of some interplanetary transients.
Received 22
March
2005;
accepted 23
June
2005;
published 23
July
2005.
Index Terms: 2101 Interplanetary Physics: Coronal mass ejections (7513); 2102 Interplanetary Physics: Corotating streams; 2114 Interplanetary Physics: Energetic particles (7514); 2139 Interplanetary Physics: Interplanetary shocks; 2164 Interplanetary Physics: Solar wind plasma.
Read Full Article (file size: 417529 bytes) Cited by
Citation: Howard, T. A., and S. J. Tappin
(2005),
Interplanetary shocks unconnected with earthbound coronal mass ejections,
Geophys. Res. Lett.,
32,
L14106,
doi:10.1029/2005GL023056.
Copyright 2005 by the American Geophysical Union.
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