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Gap analyses by variable, type of mission or WIGOS subcomponent
Variable sorting criteria
Each instrument is assigned with an up-to-5-step rating, evaluated as a blend of several elements. For this particular Variable, the rating is driven by:
the observed solar area (disk only or disk + corona);
the spectral range.
RATING CRITERIA:
1
Disk + corona, large spectral range
2
Disk + corona, narrow spectral range
3
Disk only, large spectral range
4
Disk only, narrow spectral range
5
Show sorting criteria
Measurement timeline for
Solar radio flux spectrum
Hint: Move around in the timeline by scrolling up, down, left or right.
This table has a large number of results.
Instrument
NRT ?
Relevance
Satellite
ECT/Lon
Orbit
DLR
1992
1993
1994
1995
1996
1997
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
RPW 1 - primary Solar Orbiter 25 ° Solar X
X X X X X X X X X X GOLF 3 - high SOHO L1 X
X X X X X X X X X X X X X X X X X X X X X X X X X X X X X X SORS 4 - fair Coronas-I 82.5 ° DRIFT SORS 4 - fair Coronas-F 82.5 ° DRIFT X
X X X X
All instruments for measuring Solar radio flux spectrum
Instruments
Relevance
Operational limitations
RPW 1 - primary GOLF 3 - high SORS 4 - fair