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High-speed solar wind streams: A call for key research

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High-speed solar wind streams: A call for key research. / Denton, Michael H.; Borovsky, Joseph E.; Horne, Richard B.; McPherro, Robert L.; Morley, Steven K.; Tsurutani, Bruce T.

In: EOS, Transactions American Geophysical Union, Vol. 89, No. 7, 02.2008, p. 62-63.

Research output: Contribution to journalJournal articlepeer-review

Harvard

Denton, MH, Borovsky, JE, Horne, RB, McPherro, RL, Morley, SK & Tsurutani, BT 2008, 'High-speed solar wind streams: A call for key research', EOS, Transactions American Geophysical Union, vol. 89, no. 7, pp. 62-63.

APA

Denton, M. H., Borovsky, J. E., Horne, R. B., McPherro, R. L., Morley, S. K., & Tsurutani, B. T. (2008). High-speed solar wind streams: A call for key research. EOS, Transactions American Geophysical Union, 89(7), 62-63.

Vancouver

Denton MH, Borovsky JE, Horne RB, McPherro RL, Morley SK, Tsurutani BT. High-speed solar wind streams: A call for key research. EOS, Transactions American Geophysical Union. 2008 Feb;89(7):62-63.

Author

Denton, Michael H. ; Borovsky, Joseph E. ; Horne, Richard B. ; McPherro, Robert L. ; Morley, Steven K. ; Tsurutani, Bruce T. / High-speed solar wind streams: A call for key research. In: EOS, Transactions American Geophysical Union. 2008 ; Vol. 89, No. 7. pp. 62-63.

Bibtex

@article{274d132748f84beda2bc12a7b01a6ad2,
title = "High-speed solar wind streams: A call for key research",
abstract = "The arrival of high-speed solar wind streams (HSSs) at the Earth's magnetopause drives particle and wave phenomena that are distinct from the phenomena caused by other solar wind structures. Although HSS events do not generally produce a particularly strong ring current (the current caused by ions and electrons drifting around the Earth), they do produce storm levels of other magnetospheric phenomena (enhanced convection, heating, precipitation, relativistic electron energization, and so forth) that can persist for an extended time period (e.g., many days). These events contrast with interplanetary coronal mass ejection (ICME) events, where more transient driving (e.g., 1 day) is the norm. As such, the energy input to the magnetosphere during HSS events is comparable to, or may exceed, the energy input to the magnetosphere during ICME events.",
keywords = "CIR HSS Solar Wind Streams DCS-publications-id, art-884, DCS-publications-credits, iono-fa, DCS-publications-personnel-id, 123",
author = "Denton, {Michael H.} and Borovsky, {Joseph E.} and Horne, {Richard B.} and McPherro, {Robert L.} and Morley, {Steven K.} and Tsurutani, {Bruce T.}",
year = "2008",
month = feb,
language = "English",
volume = "89",
pages = "62--63",
journal = "EOS, Transactions American Geophysical Union",
issn = "0096-3941",
publisher = "American Geophysical Union",
number = "7",

}

RIS

TY - JOUR

T1 - High-speed solar wind streams: A call for key research

AU - Denton, Michael H.

AU - Borovsky, Joseph E.

AU - Horne, Richard B.

AU - McPherro, Robert L.

AU - Morley, Steven K.

AU - Tsurutani, Bruce T.

PY - 2008/2

Y1 - 2008/2

N2 - The arrival of high-speed solar wind streams (HSSs) at the Earth's magnetopause drives particle and wave phenomena that are distinct from the phenomena caused by other solar wind structures. Although HSS events do not generally produce a particularly strong ring current (the current caused by ions and electrons drifting around the Earth), they do produce storm levels of other magnetospheric phenomena (enhanced convection, heating, precipitation, relativistic electron energization, and so forth) that can persist for an extended time period (e.g., many days). These events contrast with interplanetary coronal mass ejection (ICME) events, where more transient driving (e.g., 1 day) is the norm. As such, the energy input to the magnetosphere during HSS events is comparable to, or may exceed, the energy input to the magnetosphere during ICME events.

AB - The arrival of high-speed solar wind streams (HSSs) at the Earth's magnetopause drives particle and wave phenomena that are distinct from the phenomena caused by other solar wind structures. Although HSS events do not generally produce a particularly strong ring current (the current caused by ions and electrons drifting around the Earth), they do produce storm levels of other magnetospheric phenomena (enhanced convection, heating, precipitation, relativistic electron energization, and so forth) that can persist for an extended time period (e.g., many days). These events contrast with interplanetary coronal mass ejection (ICME) events, where more transient driving (e.g., 1 day) is the norm. As such, the energy input to the magnetosphere during HSS events is comparable to, or may exceed, the energy input to the magnetosphere during ICME events.

KW - CIR HSS Solar Wind Streams DCS-publications-id

KW - art-884

KW - DCS-publications-credits

KW - iono-fa

KW - DCS-publications-personnel-id

KW - 123

M3 - Journal article

VL - 89

SP - 62

EP - 63

JO - EOS, Transactions American Geophysical Union

JF - EOS, Transactions American Geophysical Union

SN - 0096-3941

IS - 7

ER -