Shock waves and coronal transients: The event of 1980 April 17

D. E. Gary; T. E. Gergely; M. R. Kundu

doi:10.1016/0273-1177(86)90166-3

Shock waves and coronal transients: The event of 1980 April 17

D. E. Gary
, T. E. Gergely
, M. R. Kundu

Research output: Contribution to journal › Article › peer-review

2 Scopus citations

Abstract

The coronal mass ejection (CME) event of 1980 April 17 was observed with the SMM coronagraph, and an accompanying Type II (shock wave related) burst was observed simultaneously with the Culgoora and Clark Lake radioheliographs. The method of analysis of the combined radio observations is presented. Although the radio positions were affected by severe ionospheric refraction, the combined radio observations allow a useful reduction in the range of possible positions of the 80 MHz source when the 43 MHz source is required to lie within the range of position angles of the CME. The positions of the 80 MHz radio sources under this assumption are compared with the positions of the CME loop.

Original language	English (US)
Pages (from-to)	311-314
Number of pages	4
Journal	Advances in Space Research
Volume	6
Issue number	6
DOIs	https://doi.org/10.1016/0273-1177(86)90166-3
State	Published - 1986
Externally published	Yes

All Science Journal Classification (ASJC) codes

Aerospace Engineering
Astronomy and Astrophysics
Geophysics
Atmospheric Science
Space and Planetary Science
General Earth and Planetary Sciences

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10.1016/0273-1177(86)90166-3

Cite this

@article{71d8b6267067475db1f851620467b108,

title = "Shock waves and coronal transients: The event of 1980 April 17",

abstract = "The coronal mass ejection (CME) event of 1980 April 17 was observed with the SMM coronagraph, and an accompanying Type II (shock wave related) burst was observed simultaneously with the Culgoora and Clark Lake radioheliographs. The method of analysis of the combined radio observations is presented. Although the radio positions were affected by severe ionospheric refraction, the combined radio observations allow a useful reduction in the range of possible positions of the 80 MHz source when the 43 MHz source is required to lie within the range of position angles of the CME. The positions of the 80 MHz radio sources under this assumption are compared with the positions of the CME loop.",

author = "Gary, \{D. E.\} and Gergely, \{T. E.\} and Kundu, \{M. R.\}",

note = "Funding Information: Acknowledgement: We express our sincere gratitude to the many people, working with the Culgoora, Clark Lake, and S1I11 C/P research groups, whose hard work contributed greatly to this work. This work was supported under NSF grant AT11—86l0330 to Caltech.",

year = "1986",

doi = "10.1016/0273-1177(86)90166-3",

language = "English (US)",

volume = "6",

pages = "311--314",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Elsevier Ltd",

number = "6",

}

TY - JOUR

T1 - Shock waves and coronal transients

T2 - The event of 1980 April 17

AU - Gary, D. E.

AU - Gergely, T. E.

AU - Kundu, M. R.

N1 - Funding Information: Acknowledgement: We express our sincere gratitude to the many people, working with the Culgoora, Clark Lake, and S1I11 C/P research groups, whose hard work contributed greatly to this work. This work was supported under NSF grant AT11—86l0330 to Caltech.

PY - 1986

Y1 - 1986

N2 - The coronal mass ejection (CME) event of 1980 April 17 was observed with the SMM coronagraph, and an accompanying Type II (shock wave related) burst was observed simultaneously with the Culgoora and Clark Lake radioheliographs. The method of analysis of the combined radio observations is presented. Although the radio positions were affected by severe ionospheric refraction, the combined radio observations allow a useful reduction in the range of possible positions of the 80 MHz source when the 43 MHz source is required to lie within the range of position angles of the CME. The positions of the 80 MHz radio sources under this assumption are compared with the positions of the CME loop.

AB - The coronal mass ejection (CME) event of 1980 April 17 was observed with the SMM coronagraph, and an accompanying Type II (shock wave related) burst was observed simultaneously with the Culgoora and Clark Lake radioheliographs. The method of analysis of the combined radio observations is presented. Although the radio positions were affected by severe ionospheric refraction, the combined radio observations allow a useful reduction in the range of possible positions of the 80 MHz source when the 43 MHz source is required to lie within the range of position angles of the CME. The positions of the 80 MHz radio sources under this assumption are compared with the positions of the CME loop.

UR - https://www.scopus.com/pages/publications/45949131309

UR - https://www.scopus.com/pages/publications/45949131309#tab=citedBy

U2 - 10.1016/0273-1177(86)90166-3

DO - 10.1016/0273-1177(86)90166-3

M3 - Article

AN - SCOPUS:45949131309

SN - 0273-1177

VL - 6

SP - 311

EP - 314

JO - Advances in Space Research

JF - Advances in Space Research

IS - 6

ER -

Shock waves and coronal transients: The event of 1980 April 17

Abstract

All Science Journal Classification (ASJC) codes

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