What does BSFR mean?
BSFR means Bulk Survey for Release
This acronym/slang usually belongs to Government & Military category.
What is the abbreviation for Bulk Survey for Release?
Bulk Survey for Release can be abbreviated as BSFR
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Most popular questions people look for before coming to this page
Q: A: |
What does BSFR stand for? BSFR stands for "Bulk Survey for Release". |
Q: A: |
How to abbreviate "Bulk Survey for Release"? "Bulk Survey for Release" can be abbreviated as BSFR. |
Q: A: |
What is the meaning of BSFR abbreviation? The meaning of BSFR abbreviation is "Bulk Survey for Release". |
Q: A: |
What is BSFR abbreviation? One of the definitions of BSFR is "Bulk Survey for Release". |
Q: A: |
What does BSFR mean? BSFR as abbreviation means "Bulk Survey for Release". |
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What is shorthand of Bulk Survey for Release? The most common shorthand of "Bulk Survey for Release" is BSFR. |
Abbreviations or Slang with similar meaning
- SINGG - Survey for Ionization in Neutral-Gas Galaxies
- CFR - Call for Release
- HFR - Hold for Release
- NFR - Not for Release
- RFR - Ready for Release
- STARE - Survey for Transient Astronomical Radio Emission
- STEPSS - Survey for Transiting Extrasolar Planets in Stellar Systems
- AFRPB - Application For Release of Performance Bond
- ARPB - Application for Release of Performance Bond
- CHEMPACK - Accelerated and standardised test procedures fortesting the effects of Chemicals on the Performance of Plastic Packagings and intermediate bulk Containers for the transport of dangerous goods
- ICRI - International Center for Release and Integration
- SED - Survey for Eating Disorders
- SMDP-VET - Survey for a Multi-Dimensional Pilot VET concept enabling the full integration in the labour market of Greek-Pontian women fromthe former USSR living in the periphery of Athens
- SRF - Survey for the Future
- from - for release on May
- from - for Release of Medical
- from - for release on Monday
- seds - Survey for Eating Disorders
- 2MASSI - Two-Micron All Sky Survey, Incremental release
- HK - Survey for metal-poor stars based on the strength of CaII H and K absorption lines