WMO OSCAR | Gap analyses by variable, type of mission or WIGOS subcomponent

No JavaScript detected
Usage of this Website will be severly limited without JavaScript. Please enable JavaScript in your Browser.

Gap analyses by variable, type of mission or WIGOS subcomponent

Select gap analysis type

Select analysis type

Expert system, based on instrument properties Help icon

Simplified, based on mission objectives Help icon

In "Simplified" mode, the results in the analysis are calculated by looking at each instrument's mission objectives: for each instrument we keep track of what the primary, secondary, and opportunity mission objectives are. These mission objectives indicate that an instrument is primarily envisioned to measure variable X, Y and Z, that variables A, B and C are its secondary objective, and that it may offer the opportunity to measure variables I and II although it is not optimized for that. The simplified Gap analysis produces a timeline based on this information. The simplified Gap analysis is only available for analyzing variables, not for missions.

In "Expert system" mode, the results in the analysis are calculated with an expert system. Internally, OSCAR works with a large set of 1700 rules that determine whether or not an instrument is capable of measuring a given variable, and to what degree. When you select "Expert system", the Gap analysis is performed based on this large set of rules.

Measurement timeline for Electrostatic charge Help icon

Hint: Move around in the timeline by scrolling up, down, left or right.

Found 31 results

This table has a large number of results.

Hide lower rated instruments Hide inactive instruments

Instrument	NRT?	Relevance	Satellite	Orbit	1963	1964	1965	1966	1967	1968	1988	1990	1991	1998	1999	2000	2001	2002	2003	2004	2005	2006	2007	2008	2009	2010	2011	2012	2013	2014	2015	2016	2017	2018	2019	2020	2021	2022	2023	2024	2025	2026	2027	2028	2029	2030	2031	2032	2033	2034	2035	2036	2037	2038	2039	2040
ASPOC		3 - high	CLUSTER-A	90 °												X
ASPOC		3 - high	CLUSTER-C	90 °												X	X	X	X	X	X	X	X	X	X
ASPOC		3 - high	CLUSTER-B	90 °												X	X	X	X	X	X	X	X	X	X
ASPOC		3 - high	CLUSTER-D	90 °												X	X	X	X	X	X	X	X	X	X
ASPOC (MMS)		3 - high	MMS-A	28 °																											X	X	X	X	X	X	X	X
ASPOC (MMS)		3 - high	MMS-B	28 °																											X	X	X	X	X	X	X	X
ASPOC (MMS)		3 - high	MMS-C	28 °																											X	X	X	X	X	X	X	X
ASPOC (MMS)		3 - high	MMS-D	28 °																											X	X	X	X	X	X	X	X
DSLP		3 - high	PROBA-2	06:00 asc																					X	X	X	X	X	X	X	X	X	X	X	X	X	X
iMESA-R		3 - high	STPSat-3	40.5 °																									X	X	X	X	X	X	X	X	X	X
KSEM/CM	Yes	3 - high	GEO-KOMPSAT-2A	128.2°E																														X	X	X	X	X	X	X	X	X	X	X	X
LP		3 - high	TIROS-7	58.2 °	X	X	X	X	X	X
LP		3 - high	STSat-2C	80 °																									X	X
PASTEC		3 - high	SPOT-4	10:30 desc										X	X	X	X	X	X	X	X	X	X	X	X	X	X
SEM/IMS		3 - high	FY-1A	15:30 asc							X
SEM/IMS		3 - high	FY-1B	07:50 desc								X	X
SEM/IMS		3 - high	FY-1C	07:00 desc											X	X	X	X	X	X
SEM/IMS		3 - high	FY-1D	09:00 desc														X	X	X	X	X	X	X	X	X	X	X
SEM/IMS		3 - high	FY-3A	09:05 desc																				X	X	X	X	X	X	X	X
SEM/IMS		3 - high	FY-3B	14:45 asc																						X	X	X	X	X	X	X	X	X	X	X
SEM/IMS		3 - high	FY-3C	08:20 desc																									X	X	X	X	X	X	X	X
SEP-fields	Yes	3 - high	FY-4A	104.7°E																												X	X	X	X	X	X	X	X
SEP-fields		3 - high	FY-4B	133°E																																	X	X	X	X	X	X	X	X
SEP-fields		3 - high	FY-4D	105°E																																						X	X	X	X	X	X	X	X
SEP-fields		3 - high	FY-4E	86.5°E																																							X	X	X	X	X	X	X	X
SEP-fields		3 - high	FY-4F	105°E																																										X	X	X	X	X	X	X	X
SEP-fields		3 - high	FY-4G	86.5°E																																													X	X	X	X	X	X	X	X
SPS/IMS		3 - high	KOMPSAT-1	10:50 asc											X	X	X	X	X	X	X	X	X	X
SWS/SEM/IMS	Yes	3 - high	FY-3D	13:29 asc																													X	X	X	X	X	X	X
SWS/SEM/IMS		3 - high	FY-3E	05:40 desc																																	X	X	X	X	X	X	X
SWS/SEM/IMS		3 - high	FY-3J	05:00 desc																																							X	X	X	X	X	X	X	X	X

All instruments for measuring Electrostatic charge

Instruments	Relevance	Operational limitations
ASPOC	3 - high
ASPOC (MMS)	3 - high
DSLP	3 - high
iMESA-R	3 - high
KSEM/CM	3 - high
LP	3 - high
PASTEC	3 - high
SEM/IMS	3 - high
SEP-fields	3 - high
SPS/IMS	3 - high
SWS/SEM/IMS	3 - high

Instrument Types Select
ECT Range Select
Orbit Types Select Select	Inclination Range Edit
Longitude range Select
Additional filters Select

OSCAR

Gap analyses by variable, type of mission or WIGOS subcomponent

Select gap analysis type

Select analysis type

Select a Variable

Select a type of Mission

Select a WIGOS subcomponent

Variable sorting criteria

	Each instrument is assigned with a 5-step rating, evaluated as a blend of several elements. For this particular Variable, the rating is driven by: the observed region (platform environment).. RATING CRITERIA:
1	-
2	-
3	Measured in the platform environment
4	-
5	-