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Plasma Sheet Behavior During Substorms

E. W. Hones
- Vol. 30, pp 178-184
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TLDR
In this paper, it was shown that plasmoid release is a fundamental process whereby the magnetosphere gives up excess stored energy and plasma, much like comets are seen to do, and that the phenomena of the substorm seen at earth are a byproduct of that fundamental process.
Abstract
Auroral or magnetic substorms are periods of enhanced auroral and geomagnetic activity lasting one to a few hours that signify increased dissipation of energy from the magnetosphere to the earth Data acquired during the past decade from satellites in the near-earth sector of the magnetotail have suggested that during a substorm part of the plasma sheet is severed from earth by magnetic reconnection, forming a plasmoid, ie, a body of plasma and closed magnetic loops, that flows out of the tail into the solar wind, thus returning plasma and energy that have earlier been accumulated from the solar wind Very recently this picture has been dramatically confirmed by observations, with the ISEE 3 spacecraft in the magnetotail 220 R/sub E/ from earth, of plasmoids passing that location in clear delayed response to substorms It now appears that plasmoid release is a fundamental process whereby the magnetosphere gives up excess stored energy and plasma, much like comets are seen to do, and that the phenomena of the substorm seen at earth are a by-product of that fundamental process

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LA-UR--63-3361
DE84 003833
TITLE
Plasma Sheet Behavior During Substorms
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PLASMA SHEET BEHAVIOR DURING SUBSTORM
.
Edwaud U. Hones, Jr.
UnLvcrsfty
of CallfornLa, Los Alamos National Laboratory
Los Alamos, N?l 97545
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-2-
values of
solar wind parameters at the orbit of the earth are: density
N
10/cm3; flow speed
N 450 km/see; magnetic field strength ~ 10 nano:eslas,
Thefieconstitute a particle flux
of -4.5 x 108/cm2-see, a kinesic energy flux
of roughly 1 erglrrn2-eec,
2
and a magnetic energy flux of -10-2 erg/cm -sec.
A! 1 Large-scale objects orbitfng the sun encounter this continual flow of
mn::er
and energy and, becauge of :he cohesive influence of the IUF, they can
res:rilln, locally, the solar wind’s flow and thereby store solar whd plaama
and energy In their ‘tmagne~ospheres.ri
The magnetosphere of :hoae planets
havlnR suhs:anttal intrinsic mngnc~tc fLelds (e.g., Mercury. Earth,
JupLter,

-3-
very good evidence that
it
does.
This evidence, gnimed during the past
decade,
largely from satellite measurements of partLcles, plasmas, and fields
in the outer magnetosphere, suggests very strongly that durfng “subs~orms” the
earth’s magnetosphere spont~neouely dlveeta
Lteelf of a su56tantlal portLon of
the “plasma sheet”
that e~tends across the mldplane cf
its magnetotail. In
fact it now appeara that thf6 is the basic underlying physical procesd Ln a
suhs~orrn,i.e., the magnctotall gcttlng
rld of stored plasma and energy t;,.~c
it. can no longer restra!.n.
ThLs
paper
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-4-
:he earth’s magnetic field, bombarding the upper
1980, for an excellent description of auroras and
atmosphere. (See
the development
Esther,
of our
understanding of
:hem from antiquity up to modern times.)
The International Geophysical
Year (ICY) of 1957-1958 brought globally-
organlzcd
research
efforts,
along with modern rocket
and eatelllte
Cechnologtes,
to beer on geophysics probleme
, with a strong focus on auroral
,~ndinngnctosphericresearch. Widespread networkg of all-nky cameras and
magne~oneters
were
eatahlished
to RWiy
the large-scfile space and :lme
varfa:lons of auroraa and
their a~socLated mhgnetf.c
sign~turen.
Using data
~~kilbofll
(IS64) ldcntlfied a sequence of systematic and
mIroL”al clLsplays whLch he cnlled an “aurorFIlsuhs:orm.”
Chiet
Lfc nlnng the auroral oval are lIILf!r.iiilttf2ntlyactlvatd.
It 19
I
L 1,1:
hrLght, aCLLVCB and t;pcctncularnuroL.ald~spl{.ysare seen.

Citations
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Journal ArticleDOI

Neutral line model of substorms: Past results and present view

TL;DR: In this article, the authors reviewed the NENL model of magnetospheric substorms, including the role of coupling with the solar wind and interplanetary magnetic field, the growth phase sequence, the expansion phase (and onset), and the recovery phase.
Journal ArticleDOI

Current understanding of magnetic storms: storm-substorm relationships

TL;DR: In this paper, the authors summarize the current understanding of the storm/substorm relationship by clearing up a considerable amount of controversy and by addressing the question of how solar wind energy is deposited into and is dissipated in the constituent elements that are critical to magnetospheric and ionospheric processes during magnetic storms.
Journal ArticleDOI

The driving of the plasma sheet by the solar wind

TL;DR: In this paper, the coupling of the plasma sheet to the solar wind was studied statistically using measurements from various satellite pairs: one satellite in the sun and one in either the magnetotail central plasma sheet or the near-Earth plasma sheet.
Journal ArticleDOI

Substorm currents: Growth phase and onset

TL;DR: In this paper, it was shown that a modest increase in particle energy density can produce a substantial increase in cross-tail current, and that the increased currents carried by unaccelerated preexisting particles in the changing growth phase magnetic field can play a significant role in altering magnetic field at synchronous altitude.
Journal ArticleDOI

Growth-Phase Thinning of the Near-Earth Current Sheet During the Cdaw-6 Substorm

TL;DR: The thinning of the near-Earth current sheet during the growth phase of the Coordinated Data Analysis Workshop (CDAW) 6 magnetospheric substorm is studied in this paper.
References
More filters
Journal ArticleDOI

The development of the auroral substorm.

TL;DR: In this paper, a working model of simultaneous auroral activity over the entire polar region is presented in terms of the auroral substorm, which has two characteristic phases, an expansive phase and a recovery phase.
Journal ArticleDOI

Satellite studies of magnetospheric substorms on August 15, 1968: 9. Phenomenological model for substorms

TL;DR: In this paper, the authors present a phenomenological model of the magnetospheric substorm sequence, which can be divided into three main phases: the growth phase, the expansion phase, and the recovery phase.
Journal Article

Satellite studies of magnetospheric substorms on August 15, 1968. IX - Phenomenological model for substorms.

TL;DR: In this article, observations made during three substorms on August 15, 1968, are shown to be consistent with current theoretical ideas about the cause of substorm, and the phenomenological model described in several preceding papers is further expanded.
Journal ArticleDOI

The magnetotail and substorms

TL;DR: In this article, a phenomenological or qualitative model of the substorm sequence is presented, where the flux transport is driven by the merging of the magnetospheric and interplanetary magnetic fields.
Journal ArticleDOI

The Earth's magnetic tail

TL;DR: In this article, the topology of the magnetic field within the magnetosphere and the position of both its boundary and the detached collisionless bow shock wave were investigated. But the results were limited to the Imp 1 satellite, and the range of the magnetometers was between 0.25 and 300γ.
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