So here is how I view the process. (Obviously the literature does a better job of explaining this but we just went through this event so it's somewhat relevant and definitely useful as an exercise.)
On 3/14/2024, at 12Z, there was a
strong inversion at the base of the EML. (I think the word used by meteorologists in place of
strong is "stout", which always makes me think of
beer or
Friar Tuck.)
Here's the 12Z OUN sounding (it includes my analysis of Carlson's Lid Strength Index, which is preliminary as I work out the bugs, but it's a quick and easy graphic to use since I have it already on my HD.) The sounding is classified as a Lid-ERL because I haven't automated the detection of the top of the EML, so the static stability of the layer above the inversion just misses Carlson's threshold of 4.5˚C/100mb. (But it's an EML.)
The potential temperature just above the EML base is about 311K, and just below the EML base it is about 300K. So if we look at isentropic surfaces through those values, we should be able to demonstrate the homogeneity of the EML as well as it's source region.
| Along the 311K surface (in the EML), winds are
generally SW and the humidity is very low. It seems obvious that the EML has its
origin over the Desert SW/MX.
|
| For comparison:
Just below the EML base the air mass contrast
is very high. The base of the EML inversion
ranges from about 900mb to 850mb ahead
of the dryline. |
Anyone who wants to chime in on the region of slightly-higher specific humidities over OK/TX (in the EML) that would be great. I get that, along the front, ascent represents a diabatic process than can push moisture across isentropic surfaces, so the ribbon of slightly-higher humidities along the position of the surface front makes sense. Not quite so clear about the area E of the dryline in OK/TX.