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Table D 40, BUFR template for DMSP satellites #156
Comments
https://github.com/wmo-im/CCT/wiki/Teleconference.2&3May.2023 notes: |
@amilan17 Many thanks |
https://github.com/wmo-im/CCT/wiki/Teleconference.6.7.June.2023 notes: |
@marijanacrepulja there is a comment in the PR and I changed the reference in the title from Table D 10 to 40. |
@sergioh-pessoal I have uploaded sample BUFR file and output of decoding. Many thanks for supporting validation. |
https://github.com/wmo-im/CCT/wiki/Teleconference.13.July.2023 notes: Marijana updated branch; @sergioh-pessoal will validate within a week; |
Hi @marijanacrepulja I was be able to successfully decoded the sample after replaced 1-11-000 by 1-10-000 So I think that this template can be considered validated But it is necessary to replace the descriptor 1-11-000 to 1-10-000 in the table. The result is attached Regards |
I updated the changes in the branch. See the differences here |
@sergioh-pessoal Many thanks for supporting the validation and for spotting the typo in delayed replication. The sample was encoded using 1-10-000. |
Initial request
In support for assimilation of DMSP satellites in ERA6, ECMWF is proposing new BUFR template for representation of observations from SSM/T1, SSM/T2 and SSH instruments.
Amendment details
Comments
No response
Requestor(s)
Marijana Crepulja, Roberto Ribas, Bill Bell, Adrien Oyono Owono (all from ECMWF)
Stakeholder(s)
The Copernicus Climate Change Service (C3S)
Example: Manual on Codes (WMO-No. 306), Volume I.2, BUFR D table
Expected impact of change
MEDIUM
Collaborators
No response
References
No response
Validation
No response
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