Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Geomagnetic storm
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==Definition== A geomagnetic storm is defined<ref name="gonzalez">Gonzalez, W. D., J. A. Joselyn, Y. Kamide, H. W. Kroehl, G. Rostoker, B. T. Tsurutani, and V. M. Vasyliunas (1994), What is a Geomagnetic Storm?, J. Geophys. Res., 99(A4), 5771β5792.</ref> by changes in the [[Disturbance storm time index|Dst]]<ref>{{cite journal |url=http://wdc.kugi.kyoto-u.ac.jp/dstdir/dst2/onDstindex.html |last1=Sugiura |first1=M. |first2=T. |last2=Kamei |title=Equatorial Dst index 1957β1986 |journal=IAGA Bulletin |issue=40 |editor1=A. Berthelier |editor2=M. Menville |publisher=ISGI Publ. Off. |location=Saint. Maur-des-Fosses, France |date=1991}}</ref> (disturbance β storm time) index. The Dst index estimates the globally averaged change of the horizontal component of the Earth's magnetic field at the magnetic equator based on measurements from a few magnetometer stations. Dst is computed once per hour and reported in near-real-time.<ref>{{cite web |url=http://wdc.kugi.kyoto-u.ac.jp/wdc/Sec3.html|title=World Data Center for Geomagnetism, Kyoto}}</ref> During quiet times, Dst is between +20 and β20 nano-[[Tesla (unit)|Tesla]] (nT).{{citation needed|date = April 2022}} A geomagnetic storm has three phases: initial, main and recovery. The initial phase is characterized by Dst (or its one-minute component SYM-H) increasing by 20 to 50 nT in tens of minutes. The initial phase is also referred to as a storm sudden commencement (SSC). However, not all geomagnetic storms have an initial phase and not all sudden increases in Dst or SYM-H are followed by a geomagnetic storm. The main phase of a geomagnetic storm is defined by Dst decreasing to less than β50 nT. The selection of β50 nT to define a storm is somewhat arbitrary. The minimum value during a storm will be between β50 and approximately β600 nT. The duration of the main phase is typically 2β8 hours. The recovery phase is when Dst changes from its minimum value to its quiet time value. The recovery phase may last as short as 8 hours or as long as 7 days.<ref name="gonzalez" /> [[File:Aurora borealis2, Churchill, MB.JPG|thumb|Aurora borealis]] The size of a geomagnetic storm is classified as moderate (β50 nT > minimum of Dst > β100 nT), intense (β100 nT > minimum Dst > β250 nT) or super-storm (minimum of Dst < β250 nT).<ref>{{Cite journal|last1=Cander|first1=L. R.|last2=Mihajlovic|first2=S. J.|date=1998-01-01|title=Forecasting ionospheric structure during the great geomagnetic storms|journal=Journal of Geophysical Research: Space Physics|language=en|volume=103|issue=A1|pages=391β398|doi=10.1029/97JA02418|issn=2156-2202|bibcode = 1998JGR...103..391C |doi-access=free}}</ref>
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Geomagnetic storm
(section)
Add topic