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Characteristics of Reconnection Sites and Fast Flow Channels in an MHD Simulation. Supplementary MHD simulation movie mS4-BIF.mp4 for 14 March 2008.

(2020). Characteristics of Reconnection Sites and Fast Flow Channels in an MHD Simulation. Supplementary MHD simulation movie mS4-BIF.mp4 for 14 March 2008. [Data set]. Journal of Geohysical Research - Space Physics. https://doi.org/10.21978/p8rw5g. Accessed on .

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ResourceID
spase://NASA/DisplayData/UCLA/Global-MHD-code/mS4-BIF/PT10S

Description

Section 4.1 of the text describes our procedure for identifying the locations of x-lines in a map of the neutral surface.
At each value of Y in an interpolated grid, we scan the entire length of the trace of Vx from -10 to -70 Re. A function finds all
intervals of Vx>=250 km/s and Vx less then or equal to -250 km/s. We call these earthward and tailward fast flow intervals. We define
a bifurcation of fast flow as the point at which Vx changes sign from fast earthward to fast tailward flow. In simple cases, this
transition occurs in about 2 Re (20 grid points). The zero crossing is the location of the x-line at this value of Y. As described
in the text, we process the arrays of zero crossings to define a line in the neutral surface. We display this information as lines
parallel to X at fixed Y. Intervals of fast earthward flow are represented by a thick red line. Fast flow is a thick blue line. The
zero crossing is a gray circle. After completion of the plot, we add x-lines as colored ropes (yellow with black stripes). Each map is
in a file and subsequently made into a movie. The movie illustrates the formation and evolution of x-lines.

  The movie begins at 04:00 UT with at least five significant x-lines and six earthward flow channels. This is the start of the growth 
  phase of a substorm. As time advances the locations of the x-lines change as flow channels move away from them. New lines form and 
  channels merge. When the movie approaches substorm onset at 04:44 UT the x-lines merge into a single long x-line stretching diagonally 
  across the tail. About 04:35, the nose of the fast earthward flow channel penetrates close to the Earth, and then begins to sweep 
  westward to earlier local times. At this, time the movie mS02 and the text Figure 13 shows magnetic flux accumulating close to the Earth. 
  At 04:50 UT, the single channels spawns new channels that flow directly toward Earth rather  than along the diagonal channel.

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Version:2.3.1

DisplayData

ResourceID
spase://NASA/DisplayData/UCLA/Global-MHD-code/mS4-BIF/PT10S
ResourceHeader
ResourceName
Characteristics of Reconnection Sites and Fast Flow Channels in an MHD Simulation. Supplementary MHD simulation movie mS4-BIF.mp4 for 14 March 2008.
DOI
https://doi.org/10.21978/p8rw5g
ReleaseDate
2022-03-16 00:00:00Z
Description

Section 4.1 of the text describes our procedure for identifying the locations of x-lines in a map of the neutral surface.
At each value of Y in an interpolated grid, we scan the entire length of the trace of Vx from -10 to -70 Re. A function finds all
intervals of Vx>=250 km/s and Vx less then or equal to -250 km/s. We call these earthward and tailward fast flow intervals. We define
a bifurcation of fast flow as the point at which Vx changes sign from fast earthward to fast tailward flow. In simple cases, this
transition occurs in about 2 Re (20 grid points). The zero crossing is the location of the x-line at this value of Y. As described
in the text, we process the arrays of zero crossings to define a line in the neutral surface. We display this information as lines
parallel to X at fixed Y. Intervals of fast earthward flow are represented by a thick red line. Fast flow is a thick blue line. The
zero crossing is a gray circle. After completion of the plot, we add x-lines as colored ropes (yellow with black stripes). Each map is
in a file and subsequently made into a movie. The movie illustrates the formation and evolution of x-lines.

  The movie begins at 04:00 UT with at least five significant x-lines and six earthward flow channels. This is the start of the growth 
  phase of a substorm. As time advances the locations of the x-lines change as flow channels move away from them. New lines form and 
  channels merge. When the movie approaches substorm onset at 04:44 UT the x-lines merge into a single long x-line stretching diagonally 
  across the tail. About 04:35, the nose of the fast earthward flow channel penetrates close to the Earth, and then begins to sweep 
  westward to earlier local times. At this, time the movie mS02 and the text Figure 13 shows magnetic flux accumulating close to the Earth. 
  At 04:50 UT, the single channels spawns new channels that flow directly toward Earth rather  than along the diagonal channel.
Acknowledgement
Mostafa El-Alaoui, Raymond J. Walker; Robert L. McPherron
PublicationInfo
Authors
R.L. McPherron; M. El-Alaoui; R.J. Walker; and R.L. Richard
PublicationDate
2020-08-31 00:00:00Z
PublishedBy
Journal of Geohysical Research - Space Physics
Funding
Agency
NASA
Project
Substorm current wedge development and evolution using THEMIS observation and simulations
AwardNumber
NNX17AB83G
Funding
Agency
NASA
Project
Structure and evolution of plasma sheet fast flows using THEMIS observation and global MHD simulations
AwardNumber
NNX15AI63G
Funding
Agency
NSF
Project
GEM: A Statistical Study of the Substorm Sequence and Phenomena Associated with Expansion Onset
AwardNumber
1602588
Contacts
RolePersonStartDateStopDateNote
1.GeneralContactspase://SMWG/Person/Robert.L.McPherron
2.MetadataContactspase://SMWG/Person/James.M.Weygand
InformationURL
Name
Virtual Magnetospheric Observatory directory containing movies for Journal of Gephysical Research publication.
URL
Description

Supplimentary movies for JGR publication

AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
Virtual Magnetospheric Observatory
URL
Description

Virtual Magnetospheric Observatory

Language
EN
Format
AVI
Acknowledgement
If data downloaded from the VMO Data Repository are used in publication kindly acknowledge the Virtual Magnetospheric Observatory, Earth, Planetary and Space Science Department, University of California, Los Angeles for providing access to the data.
ProcessingLevel
Raw
ProviderName
UCLA M. El-Alaoui MHD Simulation
ProviderResourceName
MHD Simulation Movies
ProviderProcessingLevel
Raw
InstrumentIDs
MeasurementType
ThermalPlasma
TemporalDescription
TimeSpan
StartDate
2008-03-14 04:00:00
StopDate
2008-03-14 05:00:00
DisplayCadence
PT10S
ObservedRegion
Earth.Magnetosphere
Keywords
MHD Simulation
Substorm
High Speed Earthward Flows
Parameter #1
Name
MHD simulation movie of GSM X component of position for 14 March 2008
ParameterKey
X component of position
Description

Two dimensional display of this movie of the GSM X component of position is on the original.

Cadence
PT10S
Units
Re
CoordinateSystem
CoordinateRepresentation
Cartesian
CoordinateSystemName
GSM
Structure
Size
3840 1890
Description

Each image is 3840 pixels by 1890 pixels and there are 360 frames in the movie.

ValidMin
-70
ValidMax
0
Support
Qualifier
Direction
SupportQuantity
Positional
Parameter #2
Name
MHD simulation movie of GSM Y component of position for 14 March 2008
ParameterKey
Y component of position
Description

Two dimensional display of this movie of the GSM Y component of position is on the original.

Cadence
PT10S
Units
Re
CoordinateSystem
CoordinateRepresentation
Cartesian
CoordinateSystemName
GSM
Structure
Size
3840 1890
Description

Each image is 3840 pixels by 1890 pixels and there are 360 frames in the movie.

ValidMin
-20
ValidMax
20
Support
Qualifier
Direction
SupportQuantity
Positional
Parameter #3
Name
MHD simulation movie of GSM X component of plasma flow velocity for 14 March 2008
ParameterKey
Vx component of plasma flow
Description

Two dimensional display of this movie of the GSM X component of plasma flow velocity is on the original, not interpolated grid. Red means Vx flows earthward and is greater then or equal to 250 km/s, Blue means Vx flows tailward and is less then or equal to 250 km/s, and white means flows are between -250 and 250 km/s.

Cadence
PT10S
Units
km/s
CoordinateSystem
CoordinateRepresentation
Cartesian
CoordinateSystemName
GSM
Structure
Size
3840 1890
Description

Each image is 3840 pixels by 1890 pixels and there are 360 frames in the movie.

ValidMin
-250
ValidMax
250
Support
Qualifier
Vector
SupportQuantity
Velocity
Parameter #4
Name
MHD simulation movie of GSM plasma flow velocity for 14 March 2008
ParameterKey
Vx and Vy components of plasma flow
Description

Two dimensional display of this movie of the GSM plasma flow velocity interpolated grid.

Cadence
PT10S
Units
km/s
CoordinateSystem
CoordinateRepresentation
Cartesian
CoordinateSystemName
GSM
Structure
Size
3840 1890
Description

Each image is 3840 pixels by 1890 pixels and there are 360 frames in the movie.

ValidMin
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ValidMax
300
Support
Qualifier
Vector
SupportQuantity
Velocity