USA flag An official website of the United States government  v

HDPWS

MetadataRightsList Access

The ISEST Master CME List

ResourceID
spase://NASA/Catalog/ACE/ISEST_Master_CME_List

Description
CME and ICME Event list - a comprehensive event list of chain of cause-effect of solar eruptive events from Sun to Earth. The ISEST (International Study of Earth-Affecting Solar Transients) is one of the four projects of the VarSITI (Variability of the Sun and Its Terrestrial Impact) program, which runs from 2014 to 2018. The VarSITI is the current scientific program of SCOSTEP (Scientific Committee on Solar-Terrestrial Physics.

Metadata Rights
CC0-1.0: Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions. The actual data/software may be subject to a different license.

View XML | Edit

Details

Version:2.7.1

Catalog

ResourceID
spase://NASA/Catalog/ACE/ISEST_Master_CME_List
NamingAuthority
NASA
ResourceType
Catalog
ResourceHeader
ResourceName
The ISEST Master CME List
ReleaseDate
2026-02-02 13:10:21Z
RevisionHistory
RevisionEvent
ReleaseDate
2025-06-19 10:12:30
Note
Only known prior ReleaseDate of the metadata
RevisionEvent
ReleaseDate
2026-02-02 13:10:21Z
Note
Added MetadataRightsList. Added ResourceType and NamingAuthority. Updated to 2.7.1. ZCB
Description
CME and ICME Event list - a comprehensive event list of chain of cause-effect of solar eruptive events from Sun to Earth. The ISEST (International Study of Earth-Affecting Solar Transients) is one of the four projects of the VarSITI (Variability of the Sun and Its Terrestrial Impact) program, which runs from 2014 to 2018. The VarSITI is the current scientific program of SCOSTEP (Scientific Committee on Solar-Terrestrial Physics.
Contacts
Role Person StartDate StopDate Note
1. Author spase://SMWG/Person/Phil.Hess
2. Author spase://SMWG/Person/Jie.Zhang
3. MetadataContact spase://SMWG/Person/Olga.Y.Uritskaya

AccessInformation
InstrumentIDs
PhenomenonType
CoronalMassEjection
PhenomenonType
InterplanetaryCoronalMassEjection
TimeSpan
StartDate
2007-05-21 21:00:00
StopDate
2013-02-17 15:00:00
Parameter #1
Name
ICME EVENT START
Description
Beginning of the ICME signature in-situ at ACE
Support
SupportQuantity
Temporal
Parameter #2
Name
ICME EVENT END
Description
Estimated End of ICME signature in-situ at ACE
Support
SupportQuantity
Temporal
Parameter #3
Name
CME in LASCO
Description
First appearance of the CME in LASCO C2, or STEREO COR2 in the event of a LASCO data gap.
Support
SupportQuantity
Temporal
Parameter #4
Name
ICME TYPE
Description
Describes the signature in-situ, Shock Front (SH), MC (Magnetic Cloud), EJ (CME Ejecta Front)
Support
SupportQuantity
Other
Parameter #5
Name
AR
Description
The Source Active region of the CME, if there is one
Support
SupportQuantity
Other
Parameter #6
Name
Surface Location
Description
The location of the Active Region or, if there is no AR, the approximate location of the eruption.
Support
SupportQuantity
Positional
Parameter #7
Name
Flare Magnitude
Description
If the CME is associated with a flare, the strength of the flare.
Support
SupportQuantity
Other
Parameter #8
Name
Flare Onset Time
Description
The beginning of the flare
Support
SupportQuantity
Temporal
Parameter #9
Name
SEEDS VEL C2
Description
The velocity of the CME, as determined by the SEEDS C2 Catalog. These velocities are for quick reference only, and should not be taken at face value. There are different errors that are present in these velocities and they should not be used for an serious study or research work
Support
SupportQuantity
Velocity
Parameter #10
Name
SEEDS VEL A
Description
The velocity of the CME, as determined by the SEEDS STEREO Catalog. These velocities are for quick reference only, and should not be taken at face value. There are different errors that are present in these velocities and they should not be used for an serious study or research work
Support
SupportQuantity
Velocity
Parameter #11
Name
SEEDS VEL B
Description
The velocity of the CME, as determined by the SEEDS STEREO Catalog. These velocities are for quick reference only, and should not be taken at face value. There are different errors that are present in these velocities and they should not be used for an serious study or research work
Support
SupportQuantity
Velocity
Parameter #12
Name
AVG. VEL
Description
The average velocity of the CME as calculated by determining the time of the CME in C2 and the beginning of the signature in-situ
Support
SupportQuantity
Velocity
Parameter #13
Name
Velocity
Description
The average velocity of the ejecta at ACE
Support
SupportQuantity
Velocity
Parameter #14
Name
Transit time
Support
SupportQuantity
Temporal
Parameter #15
Name
DST PEAK
Description
The lowest value of the DST index
Support
SupportQuantity
Other
Parameter #16
Name
DST PEAK TIME
Description
The time when the lowest value of the DST index occurs (as long as the peak is below -40)
Support
SupportQuantity
Temporal
Parameter #17
Name
EJECTA START TIME
Description
The beginning of the CME Ejecta in-situ (if there is no shock this is the same as the ICME start time)
Support
SupportQuantity
Temporal
Parameter #18
Name
Quality Rating
Description
This denotes the quality of the event's signature in-situ, 1 is the best, 3 is the worst.
Support
SupportQuantity
DataQuality
Parameter #19
Name
In-Situ Link
Description
A link to the in-situ data for the event
Support
SupportQuantity
WebResource
Parameter #20
Name
C2 Link
Description
A link to a movie of the CME in LASCO C2
Support
SupportQuantity
WebResource
Parameter #21
Name
COR2 Link
Description
A link to a movie of the CME in STEREO COR2
Support
SupportQuantity
WebResource
Parameter #22
Name
EIT/AIA Link
Description
A link to a movie of the eruption on the Sun as seen by either the SOHO EIT or SDO AIA instrument
Support
SupportQuantity
WebResource
Parameter #23
Name
CDAW VEL C2
Description
The velocity of the CME, as determined by the CDAW CME Catalog. These velocities are for quick reference only, and should not be taken at face value. There are different errors that are present in these velocities and they should not be used for an serious study or research work
Support
SupportQuantity
Velocity