{"id":11722,"date":"2021-02-08T16:40:59","date_gmt":"2021-02-09T02:40:59","guid":{"rendered":"http:\/\/www.eaobservatory.org\/jcmt\/?page_id=11722"},"modified":"2022-06-30T11:42:05","modified_gmt":"2022-06-30T21:42:05","slug":"wvm","status":"publish","type":"page","link":"https:\/\/www.eaobservatory.org\/jcmt\/instrumentation\/wvm\/","title":{"rendered":"WVM"},"content":{"rendered":"

The JCMT relies on its in-cabin line-of-sight 183 GHz radiometer, the WVM (Water Vapour Monitor) to measure the PWV (Precipitable Water Vapour) and report the sky opacity at (the historically used) 225 GHz. The WVM is critical for both SCUBA-2<\/a> observations (see the note about extinction correction<\/a>) and also for use by N\u0101makanui<\/a>, as well as determining the current weather conditions<\/a> for programs to observe under, according to the JCMT’s Flexible Observing<\/a> Guidelines.<\/p>\n

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The WVM works by obtaining measurements of the 183 GHz water line in a number of channels.<\/p>\n

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The three double side band frequency channels of the water vapour monitor super imposed on the spectrum of the water line for 0.5, 1 and 1.5 mm of PWV (image taken from Atmospheric Water Vapour and Astronomical Millimetre Interferometry by Martina Corinna Wiedner<\/a>)<\/p><\/div>\n

 <\/p>\n

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The WVM box with the two electronics plates. The upper plate is the RF plate. The horn and mixer are in the centre of the RF plate the horn is pointing away from the photographer to the flip mirror. The lower plate contains the IF electronics. The warm and cold loads are circled. (image taken from Atmospheric Water Vapour and Astronomical Millimetre Interferometry by Martina Corinna Wiedner<\/a>).<\/p><\/div>\n

For archival values of the WVM you can visit: WVM Archive Interface<\/a>.<\/p>\n

 <\/p>\n

Correcting WVM issues in SCUBA-2 data<\/h2>\n

If WVM data are missing from raw files, but the full data from the WVM are available on disk at CADC, the WESLEY recipe can be used to copy the WVM data into the raw files, and then reduce as normal. To obtain WVM data files visit first visit JCMT CADC<\/a> archive page and search the JCMT’s collection using the selected instrument as: “wvm”. Then run up starlink’s<\/a> ORACDR<\/p>\n

oracdr_scuba2_850 \r\n<\/pre>\n
then run:<\/p>\n
wesley --files files.list INSERT_JCMT_WVM_DATA -verbose -log sf -nodisplay\r\n -recpars=\"JCMT_WVM_FILE=20200217.wvm\"\r\n<\/pre>\n
ensuring 20200217.wvm is in cwd\/ORAC_DATA_OUT and where files.list are the raw files you wish to reduce.<\/p>\n
These are the information written into the WVM .wvm files:<\/p>\n
1) isoTime Time and date string
\n2) airMass Air Mass
\n3) tAmb Ambient temperature (kelvin)
\n4) tSky[0] Sky temperature 0 (kelvin)
\n5) tSky[1] Sky temperature 1 (kelvin)
\n6) tSky[2] Sky temperature 2 (kelvin)
\n7) tWat The effective temperature
\n8) tOff The line of site opacity
\n9) mmH2O_a The line-of sight water density in mm
\n10) mmH2O_z The water density at zenith in mm
\n11) finalTau The Tau at zenith
\n12) tSys[0] The system temperature of receiver 0
\n13 tSys[1] The system temperature of receiver 1
\n14) tSys[2] The system temperature of receiver 2
\n15) azimuthDeg Antenna azimuth in degrees<\/p>\n
 <\/p>\n
Users with SCUBA-2 data taken 20210128<\/h3>\n
On UT 20210128 an adjustment was made to the WVM method that was in place for a day and impacts SCUBA-2 data taken on that date. Users that had data taken will need to follow the method outlines above, running the welsley command on raw SCUBA-2 data prior to reducing data. the .wvm file that should be used on that date is found at the following link: 20210128_OLD.wvm<\/a><\/p>\n
 <\/p>\n","protected":false},"excerpt":{"rendered":"
The JCMT relies on its in-cabin line-of-sight 183 GHz radiometer, the WVM (Water Vapour Monitor) to measure the PWV (Precipitable Water Vapour) and report the sky opacity at (the historically used) 225 GHz. The WVM is critical for both SCUBA-2 observations (see the note about extinction correction) and also for\u2026 Continue reading<\/a><\/p>\n","protected":false},"author":5,"featured_media":0,"parent":134,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"_links":{"self":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/11722"}],"collection":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/comments?post=11722"}],"version-history":[{"count":16,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/11722\/revisions"}],"predecessor-version":[{"id":12623,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/11722\/revisions\/12623"}],"up":[{"embeddable":true,"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/pages\/134"}],"wp:attachment":[{"href":"https:\/\/www.eaobservatory.org\/jcmt\/wp-json\/wp\/v2\/media?parent=11722"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}