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New evidence for ozone depletion in the upper stratosphere. / Semenov, V. S.; Farrugia, C. J.; Biernat, H. K.; Lebedeva, V. V.; Rijnbeek, R. P.

In: Geophysical Research Letters, Vol. 21, No. 22, 01.11.1994, p. 2437-2440.

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

Harvard

Semenov, VS, Farrugia, CJ, Biernat, HK, Lebedeva, VV & Rijnbeek, RP 1994, 'New evidence for ozone depletion in the upper stratosphere', Geophysical Research Letters, vol. 21, no. 22, pp. 2437-2440. https://doi.org/10.1029/94GL02482

APA

Semenov, V. S., Farrugia, C. J., Biernat, H. K., Lebedeva, V. V., & Rijnbeek, R. P. (1994). New evidence for ozone depletion in the upper stratosphere. Geophysical Research Letters, 21(22), 2437-2440. https://doi.org/10.1029/94GL02482

Vancouver

Semenov VS, Farrugia CJ, Biernat HK, Lebedeva VV, Rijnbeek RP. New evidence for ozone depletion in the upper stratosphere. Geophysical Research Letters. 1994 Nov 1;21(22):2437-2440. https://doi.org/10.1029/94GL02482

Author

Semenov, V. S. ; Farrugia, C. J. ; Biernat, H. K. ; Lebedeva, V. V. ; Rijnbeek, R. P. / New evidence for ozone depletion in the upper stratosphere. In: Geophysical Research Letters. 1994 ; Vol. 21, No. 22. pp. 2437-2440.

BibTeX

@article{fc610d34b4fc41a794d9b3dddf4bd4b1,
title = "New evidence for ozone depletion in the upper stratosphere",
abstract = "We highlight one result of a time‐dependent analysis of reconnection at the terrestrial magnetopause, namely, that the Petschek‐type reconnection process is inevitably accompanied by the generation of surface waves. These waves propagate along the magnetopause at a speed which is generally different from that of the shocks and discontinuities bounding the region of heated and accelerated plasma, the so‐called outflow region of reconnected plasma. The surface waves play a central role in the reconnection process because it is through them that the perturbations of the magnetic field and velocity normal to the magnetopause are transmitted along the current sheet from the source region to the system at large. Since reconnection acts as a source of surface waves, the present general view that transient phenomena at the magnetopause are due either to surface waves (generated by, for example, variations in the solar wind) or to transient reconnection should be revised in the interests of a more unified treatment.",
author = "Semenov, {V. S.} and Farrugia, {C. J.} and Biernat, {H. K.} and Lebedeva, {V. V.} and Rijnbeek, {R. P.}",
year = "1994",
month = nov,
day = "1",
doi = "10.1029/94GL02482",
language = "English",
volume = "21",
pages = "2437--2440",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "American Geophysical Union",
number = "22",

}

RIS

TY - JOUR

T1 - New evidence for ozone depletion in the upper stratosphere

AU - Semenov, V. S.

AU - Farrugia, C. J.

AU - Biernat, H. K.

AU - Lebedeva, V. V.

AU - Rijnbeek, R. P.

PY - 1994/11/1

Y1 - 1994/11/1

N2 - We highlight one result of a time‐dependent analysis of reconnection at the terrestrial magnetopause, namely, that the Petschek‐type reconnection process is inevitably accompanied by the generation of surface waves. These waves propagate along the magnetopause at a speed which is generally different from that of the shocks and discontinuities bounding the region of heated and accelerated plasma, the so‐called outflow region of reconnected plasma. The surface waves play a central role in the reconnection process because it is through them that the perturbations of the magnetic field and velocity normal to the magnetopause are transmitted along the current sheet from the source region to the system at large. Since reconnection acts as a source of surface waves, the present general view that transient phenomena at the magnetopause are due either to surface waves (generated by, for example, variations in the solar wind) or to transient reconnection should be revised in the interests of a more unified treatment.

AB - We highlight one result of a time‐dependent analysis of reconnection at the terrestrial magnetopause, namely, that the Petschek‐type reconnection process is inevitably accompanied by the generation of surface waves. These waves propagate along the magnetopause at a speed which is generally different from that of the shocks and discontinuities bounding the region of heated and accelerated plasma, the so‐called outflow region of reconnected plasma. The surface waves play a central role in the reconnection process because it is through them that the perturbations of the magnetic field and velocity normal to the magnetopause are transmitted along the current sheet from the source region to the system at large. Since reconnection acts as a source of surface waves, the present general view that transient phenomena at the magnetopause are due either to surface waves (generated by, for example, variations in the solar wind) or to transient reconnection should be revised in the interests of a more unified treatment.

UR - http://www.scopus.com/inward/record.url?scp=0028547514&partnerID=8YFLogxK

U2 - 10.1029/94GL02482

DO - 10.1029/94GL02482

M3 - Article

AN - SCOPUS:0028547514

VL - 21

SP - 2437

EP - 2440

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

IS - 22

ER -

ID: 53093001