Leeside cold front of 10 November 2014: Blowing dust and deep-tropospheric gravity waves

A strong cold front pushed southward across the Plains during the day on November 10, 2014.  The temperature gradient across the front was quite dramatic, as seen by the surface observations at 23:00 UTC:


Visible imagery from GOES-East during the afternoon hours centered over Colorado clearly showed the southward progress of the cold front as dust was being lofted at the edge of the cold front where surface winds are strongest:


Note the rapid movement of the cold front as it moves from southeast Colorado towards northeast New Mexico as you can easily trace it by the blowing dust.

The GOES-West shortwave albedo product also clearly shows the blowing dust:


Confirming the existence of the dust is this webcam along I-25 at Raton Pass (along the New Mexico / Colorado border):


Another interesting aspect of this event are the deep-tropospheric gravity waves created by the leeside cold front.  The GOES water vapor imagery shows narrow bands coincident with the cold front as it moves southward immediately to the lee of the Rockies:


Relatively strong vertical motion exists along these narrow bands in a broad zone through the upper troposphere and into the lower stratosphere.  The resulting vertical displacements are up to 1 km, making them appear in the water vapor imagery.

Interestingly enough, the synthetic water vapor imagery from the 4-km NSSL WRF-ARW model also depicts these narrow bands associated with the leeside cold front:


The model was too slow with the leeside cold front, and this is a known model bias due to sharp inversions that exist with shallow arctic fronts.

For more information on leeside cold fronts and their appearance in water vapor imagery see:

Ralph, F.M., P.J. Neiman, and T.L. Keller, 1999:  Deep-Tropospheric Gravity Waves Created by Leeside Cold Fronts. J. Atmos. Sci., 56, 2986-3009.

Posted in Synthetic NSSL WRF-ARW Imagery | Leave a comment

Convective Initiation Application via the Split Window Difference product

One of the exciting new products that will be available on GOES-R is the split window difference (SWD) which is simply the difference between the 10.35 micron and 12.3 micrometer channels.  This channel difference has been shown to provide information about atmospheric column water vapor.  Higher SWD values (larger positive difference) can correspond to deepener low-level moisture in a cloud-free environment.  This signature can be utilized to anticipate where and when convective initiation will occur in cloud-free conditions away from complex terrain (such as the Great Plains).  Although similar bands were available on some previous GOES instruments, their coarse resolution and poor signal-to-noise ratio made them less useful for identifying subtle small-scale features in the low level moisture field.

In order to demonstrate this product (since the 12.3 micron channel is not available on the current GOES imager), we use synthetic imagery from the 4-km NSSL WRF-ARW model.  Here is an example of the SWD on a day with a dryline across Texas:

The larger (positive difference) values of SWD are shown in warm colors, while the location of the cross section (shown below) is illustrated by the east-west oriented black line.  Next, we will look at output from the NSSL WRF-ARW model along the cross section line:

The white line indicates SWD values (scale on the right) while the colors are specific humidity.  SWD values are greatest along the dryline where the depth of the moisture is greatest.  The low-level temperature lapse rate also plays a role in the SWD, but as can be seen in the cross section, the depth of the moisture is the dominating factor.

A loop of the synthetic SWD from the NSSL WRF-ARW:


shows the animation from 1500 – 0000 UTC at hourly intervals from the model.  On the left is the synthetic IR (10.35 micron) band and on the right is the synthetic SWD product (larger SWD values are shown in warmer colors).

The first thing to note is the skies are clear before convective initiation across Texas which is necessary to make use of the product in this way.  The larger SWD values develop along the dryline prior to convective initiation.  Keep in mind this synthetic data is at hourly intervals, but once GOES-R becomes available, the data will be displayed at 5 (or even 1) minute intervals.

We can preview how this data may appear on GOES-R by looking at an example from the MSG (Meteosat Second Generation) SEVERI instrument over Europe.  An event occurred on 6 July 2012 where convection developed along a convergence boundary under clear skies prior to initiation.  Also, this event occurred over flat terrain (Poland) which is important since complex terrain complicates this signature.

Here is the zoomed in visible imagery (over Poland) from the MSG satellite from 0845 – 1500 UTC 6 July 2012:


The key to note is the clear skies prior to convective initiation.

Here is the zoomed in SWD imagery (over Poland) from the MSG satellite over the same time period:


Focus on the clear area (that was shown in the visible image) from the center of the scene southeastward.  SWD values gradually increase (going toward warmer colors) indicating deepening moisture along this convergence boundary, followed by convective initiation (expanding regions of blue/purple later in the loop).

A local maximum in SWD developed over a convergence boundary (under clear skies) about 2 hours prior to convective initiation.  Forecasters can make use of this information when attempting to predict where / when convective initiation will occur.  As looking at this imagery becomes routine with GOES-R for diagnosing convective initiation (under clear skies beforehand), experience with this product will lead to greater forecaster confidence in timing and location of convective initiation.

For more detailed information on this product, see this article:

Lindsey, D.T., Grasso, L., Dostalek, J.F., and J. Kerkmann, 2014: Use of the GOES-R Split-Window Difference to Diagnose Deepening Low-Level Water Vapor. J. Appl. Meteor. Climatol., 53, 2005–2016.  http://dx.doi.org/10.1175/JAMC-D-14-0010.1

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GOES-14 SRSO for 11 May 2014 Severe Weather Event

GOES-14 was operating on super rapid scan operations schedule for May 11, 2014, meaning that images were being taken every 1 minute.  This high temporal resolution data will be routinely available for severe weather events with GOES-R, therefore it is beneficial to learn how to maximize the value added by this dataset.  SPC issued a moderate risk for portions of Nebraska and Kansas which will be the focus here.  The GOES visible imagery from 1838 to 2011 UTC is shown here:


To aid in interpretation of this loop, an annotated image is shown:

Around this time, a southwest-northeast oriented cold front was surging southward in western Kansas while a dryline was positioned just east of this cold front where convective initiation occurs in southwest Kansas.  An east-west oriented warm front is annotated above, which was slowly moving northward.  Moderate instability and high shear existed along the warm front in southeast Nebraska.  The warm sector is characterized by cloud streets, parallel to the low-level (southerly) flow while north of the warm front a much more stable air mass exists characterized by stable wave clouds oriented perpendicular to the winds at inversion top level.

Earlier convective initiation occurs in southwest Kansas along the dryline.  The high temporal resolution allows one to see multiple updrafts attempting to penetrate the capping inversion and eventually lead to thunderstorm development.  The first sign of convective initiation are shadows projected by anvil cirrus.

Further north, in the region delineated with an oval in the annotated image above, we can see attempts at convective initiation along the western portion of the warm front, near the intersecting cold front.  Multiple updrafts merge into one dominant updraft region where the supercell develops.  Initial motion of these updrafts is towards the northeast, but by the end of the loop as we see one dominant updraft we can already see indications of this storm turning towards the right (east) along the warm front.

For access to real-time GOES SRSO (when available) click here:


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More dust – this time amidst the clouds – 29 April 2014 case

A recent post took a look at the CIRA dust products for the widespread blowing dust event across the Southern Plains behind a strong cold front on 27 April.  The associated upper-level trough moved into the middle of the nation and became a giant closed low that stalled for days.  Figure 1 shows the position of the closed 500 mb low along with an analysis of sea level pressure and NOWRAD radar reflectivity for midweek (0000 UTC on 30 April).  The giant upper-level low affected the weather across much of the nation; here we focus on the strong northerly winds on its backside across the plains of eastern Colorado and the Texas and Oklahoma Panhandles.

Figure 1. 500 mb and MSLP analysis with NOWRAD radar reflectivity for 0000 UTC/30 April.

We will take a closer look at the 2000 UTC time, which is when the Suomi/NPP satellite passed over the area of interest.  The surface plot near this time is shown in Figure 2.

Figure 2. Surface METAR plot at 1943 UTC on 29 April.

The very strong northerly winds, with gusts as high as 70 mph in eastern Colorado, produced intense areas of blowing dust that created very hazardous driving conditions, forcing a number of roads to close during the day (including for a time Interstate 70 in eastern Colorado).  A picture taken in the late morning near the intersection of Highway 40 and 287, in eastern Colorado south of I-70, shows the near zero visibility (Figure 3).

Figure 3. Photo from eastern Colorado in the late morning showing the near zero visibility in blowing dust.

What was particularly interesting about this case, and challenging for forecasters, was the blowing dust being present amidst lots of clouds and even rain (and some snow) showers, as seen in the next two figures showing conditions near 2000 UTC.

Figure 4. NOWRAD radar reflectivity image at 2000 UTC on 29 April.

Figure 5. GOES visible satellite image at 1945 UTC.

Often blowing dust events occur without many clouds present, since the associated airmass is often quite dry (see for example the blog from 27 April).  In this case it is certainly difficult to see dust plumes across the eastern Plains of Colorado amidst all the cloudiness, or farther to the south, given all the cloudiness.  Did the CIRA dust products help in this regard?  First we will focus on eastern Colorado, then shift farther to the south centering on the Texas Panhandle, all for the 2000 UTC Suomi/NPP pass.  As noted in previous blogs, Polar orbiting satellites have higher spatial resolution but limited time resolution, but are useful to replicate products that will be available at both high spatial and time resolution in the GOES-R era.  In Figure 6 a True Color visible image is shown, followed by the CIRA Pink Dust product in Figure 7.

Figure 6. Suomi/NPP True Color visible satellite image at 2000 UTC centered on Colorado.

Figure 7. CIRA Suomi/NPP Pink Dust satellite image at 2000 UTC centered on Colorado. Dust appears as pink colors.

The True Color visible image is striking, but the dust is difficult to see, whereas it is much more obvious in the CIRA Pink Dust product in Figure 7.  The same is true for the blowing dust farther to the south at this time across the Texas Panhandle, with the dust not so easy to see in the visible True Color image in Figure 8 but very obvious with the CIRA Pink Dust product in Figure 9.

Figure 8. True Color visible image at 2000 UTC centered over the Texas Panhandle.

Figure 9. CIRA Pink Dust product at 2000 UTC centered over the Texas Panhandle.

CIRA also has a dust discrimination product using GOES, which allows for much better time resolution than from the Polar satellites, but considerably lower spatial resolution (10 km using a split window technique from GOES sounder data).  This type of image for this case at 1945 UTC is shown in Figure 10.

FIgure 10. CIRA dust discrimination product from the GOES sounder data, for 1945 UTC on 29 April. Dust appears as yellow, or red for thicker dust.

With the lower resolution it is not so easy to see the dust amidst the clouds in Figure 10, but the technique does a nice job of showing the dust farther to the south.

You can find more information on this (and other CIRA GOES-R Proving Ground products) product at http://rammb.cira.colostate.edu/research/goes-r/proving_ground/cira_product_list/ The products are available for display in AWIPS I or II; contact CIRA if interested in receiving them.

Posted in Blowing Dust (Blue-light absorption technique), Blowing Dust Detection (Split-window technique) | Leave a comment

April 27 – Severe weather followed by blowing dust across the Plains

The extensive outbreak of severe weather on Sunday 27 April (see SPC plot of reports below in Figure 1) made headlines with many destructive tornadoes.  A strong cold front associated with an intense low lifting out of the Rockies led to the large outbreak (Figure 2 shows the low at 1200 UTC Monday morning 28 April).  Meanwhile very strong winds behind the front produced a large area of blowing dust across the Southern Plains.  In this blog entry we will take a look at this dust area through some satellite products designed to highlight blowing dust.140427_rpts Reports Graphic

Figure 1.  Plot of severe weather reports from the Storm Prediction Center for 27 April.

Click Image For Station Plots

Figure 2.  Surface mslp analysis with fronts at 1200 UTC on Monday 28 April.

First a comparison is made between how the dust storm looked on Sunday afternoon on GOES visible imagery currently on AWIPS and imagery from about the same time from the Suomi/NPP (Polar orbiting) satellite with the VIIRS instrumentation.  The products from the Suomi/NPP satellite represent the type of imagery that will be available at high spatial and temporal resolution when the GOES-R satellite is launched.  For now the spatial resolution is high (1 km) but the temporal resolution is low, with 2 times that can be shown using VIIRS for this case, one at 1859 UTC and the other at 2038 UTC.  Similar looking imagery is also available from the MODIS Aqua and Terra Polar orbiting satellites, but is not shown here as the image swaths are at about the same time.

Images for the first time are shown in Figures 3-5.  Figure 3 shows how the dust appears in AWIPS for a GOES visible image at 1852 UTC, overlaid with METAR observations from 1900 UTC. Gusty (30 mph or greater gusts) southwest winds prevail across much of Kansas and Oklahoma, with even strong winds farther west across the High Plains, lifting plumes of dust.  Visible imagery from VIIRS with a true color background at 1857 UTC is shown in Figure 4.  So much dust is lifted that it looks like we can easily see the plumes in the AWIPS image, and somewhat better in the true color image.  It is not always so easy to see where the dust plumes are, however, so CIRA has developed a product that highlights the dust in a pink color (a similar version uses yellow for the dust), and this image is shown also for 1857 UTC in Figure 5.  You can find more information on this (and other CIRA GOES-R Proving Ground products) product at http://rammb.cira.colostate.edu/research/goes-r/proving_ground/cira_product_list/ The dust plumes are easily seen in this image, which represents a product that will be available in the GOES-R era.  Notice how the southernmost plume of dust in the Texas Panhandle is easily seen, whereas it is not so obvious in the GOES visible image shown in Figure 3.

Figure 3. GOES visible image at 1852 UTC on 27 April from AWIPS overlaid with 1900 UTC observations.

Figure 4. Suomi/NPP True Color image at 1857 UTC on 27 April.

Figure 5. CIRA Suomi/NPP Pink dust image at 1857 UTC.

The same images are shown for the second available time (2038 UTC).  Strong southwest winds continue to prevail across the Southern Plains, with areas of dust discernible in the visible image (Figure 6) across west-central KS and OK and the TX Panhandle.  The Suomi/NPP images are shown for two areas in Figures 7-10.  For the northern area most of the dust shown in the Pink dust image can also be seen in the two visible images.  Figures 9 and 10 show the area farther to the south, and here the CIRA dust product in Figure 10 highlights dust plumes farther to the south that are not so obvious in the AWIPS visible imagery or even the true color image, showing the potential value of such a product.

Figure 6. GOES visible image from AWIPS at 2038 UTC on 27 April with 2000 UTC observations

Figure 7. Suomi/NPP True Color image at 2038 UTC.

Figure 8. CIRA Suomi/NPP Pink Dust image at 2038 UTC over the same area.

Figure 9. Suomi/NPP True Color image at 2038 UTC but zoomed in on the Texas Panhandle.

Figure 10. CIRA Suomi/NPP Pink Dust image at 2038 UTC also over the Texas Panhandle.

Dust discrimination imagery can also be created from the current GOES satellites through the GOES sounder, with a split window technique that uses the 10.7 um (more-transparent longwave) and 12.0 um (less-transparent longwave) infrared window bands.  The resolution is much lower (10 km) than for images from the Polar satellites (and from what will be available in the GOES-R era), but there is the advantage of hourly time resolution, which means one can loop the imagery.  Further description of the imagery and how it is made can be found on the link to the CIRA products page given earlier.  An example of this GOES-based dust imagery produced by CIRA for this case is shown in Figure 11 for 1846 UTC and in Figure 12 at 2046 UTC on 27 April.  Dust appears as yellow or red (red for thicker dust).

Figure 11. CIRA GOES-based dust product at 1846 UTC on 27 April.

Figure 12. CIRA GOES-based dust product at 2046 UTC on 27 April.

The imagery shown in this example is available now for display in AWIPS I or II; contact CIRA if interested.

Posted in Blowing Dust (Blue-light absorption technique), Blowing Dust Detection (Split-window technique) | Leave a comment

An even stronger cold front and even more blowing dust – 18 March 2014

In a recent post we showed a dust storm that moved through southeast Colorado and into the Texas Panhandle on 11 March with a strong cold front.  Another cold front, even a bit stronger than the one last week, pushed southward through the same area almost exactly one week later as a deepening surface low emerged from the Rockies into the South-Central Plains (see Figure 1 below).  Here we will again take a look at the CIRA Proving Ground Pink and Yellow Dust Products from MODIS.

Figure 1. Visible image combined with radar reflectivity at 1745 UTC on 18 March, overlaid with 1800 UTC METAR observations and a pressure (MSLP) analysis.

A closer look at the area of interest is shown in Figures 2 and 3, where we also get a feel for how well the dust showed up in this case with GOES visible satellite imagery.

Figure 2. Visible satellite image at 1630 UTC with the 1700 UTC METAR plot.

In the image about the cold front has moved into the Texas Panhandle with a distinct wind shift.  Stronger wind gusts exceeding 50 mph are found just to the north in southeastern Colorado, where temperatures have dropped into the 40s.  Even colder air lies just to the north, with Limon (at the northern edge of the image) reporting heavy snow.  One area of blowing dust is in southeastern Colorado with the stronger winds, although it is not obviously dust from the image above.  Another area of dust is seen blowing from west to east ahead of the cold front in the warmer air and dry westerly flow, and this dust is more apparent in the image, as it is in the next image (below) from 30 minutes later.

Figure 3. Visible satellite image at 1700 UTC with the 1700 UTC METAR plot.

The next visible image (Figure 4) is from one hour later, and at this time we also have a MODIS pass so we can compare how the dust looks with the two CIRA dust products.

Figure 4. Visible satellite image at 1800 UTC with the 1800 UTC METAR plot.

Here are the two dust products for near this time; the “pink” dust product (Figure 5) and the “yellow” dust product (Figure 6).

Figure 5. CIRA Proving Ground Pink Dust Product at 1810 UTC.

Figure 6. CIRA Proving Ground Yellow Dust Product at 1810 UTC.

In both CIRA products the dust is clearly distinguished from the background clouds (which are bluish in the Yellow Dust Product and more cyan colored in the Pink Dust Product).  It is especially easy to see the large amount of dust in far southeastern Colorado into the Oklahoma Panhandle with the stronger winds behind the cold front. This particular area of dust continued to consolidate during the afternoon as it pushed southward.  A lot of wave structure is seen in the dust, given the horizontal resolution of 1 km in the MODIS-based imagery.  Figure 7 shows the visible image at 1900 UTC again with a METAR plot at the same time.  The image in Figure 8 is the same for 2000 UTC.  We can compare these images with the CIRA dust products from the next MODIS pass at 1948 UTC, in Figures 9 and 10.

Figure 7. Visible satellite image at 1900 UTC with the 1900 UTC METAR plot.

Figure 8. Visible satellite image at 2000 UTC with the 2000 UTC METAR plot.

Figure 9. CIRA Proving Ground Pink Dust Product at 1948 UTC.

Figure 10. CIRA Proving Ground Yellow Dust Product at 1948 UTC.

The CIRA Dust product images again reveal two areas of blowing dust, a dense area just moving into the Texas Panhandle associated with the stronger northerly winds and sharp cooling behind the cold front.  The southern area of dust is still in the same general area  as before (near Lubbock, TX (LBB), similar to what occurred a week earlier when they experienced a pre-frontal dust event before a second one behind the cold front).  There likely is more blowing dust in southeastern Colorado than is shown in the imagery, but it is obscured by low cloudiness in the colder air well behind the front.

A more recent addition to the Polar orbiting satellites is the Suomi/NPP satellite with the VIIRS instrumentation, which also has the channels needed to make an image similar to the one shown in Figure 10.  The pass on this day was at 1946 UTC, and the CIRA pink dust image is shown in Figure 11 below.

Figure 11. CIRA pink dust image at 1946 UTC from the VIIRS instrument aboard the Suomi/NPP satellite.

The area of dense dust well behind the cold front continued to expand as it moved southward across the Texas Panhandle, becoming a larger scale Haboob that spread through Amarillo (AMA) and LBB, again almost exactly a week after the previous event. Some METAR observations are shown below (Figure 12, from La Junta (LHX) and Figure 13, from Lamar (LAA), both in southeastern Colorado and equally far south, from AMA in Figure 14 (located in the central Texas Panhandle) and then farther south from LBB, in Figure 15).

Figure 12. METAR observations from La Junta (LHX), Colorado from 0853 UTC (bottom) to 2003 UTC (top) on 18 March.

Figure 13. METAR observations from Lamar (LAA), Colorado from 0853 UTC (bottom) to 2003 UTC (top) on 18 March.

Figure 14. METAR observations from Amarillo (AMA), Texas from 1153 UTC/18 March (bottom) to 1153 UTC/19 March (top).

Figure 15. METAR observations from Lubbock (LBB), Texas from 1253 UTC/18 March (bottom) to 0853 UTC/19 March (top).

The various NWS Weather Forecast Offices (WFOs) issued numerous statements, warnings and other graphical products to convey information about the blowing dust, which can be very hazardous to travel when visibilities are suddenly reduced.  Below we show a sample of these from north to south.  First is a look at the “Weather Story” from the Boulder (BOU) WFO issued on the morning of 18 March, in Figure 16, then moving farther south the same product from the Pueblo (PUB) Colorado WFO in Figure 17.

Figure 16. BOU WFO Weather Story graphic conveying information on the blowing dust. Note the snow also in the forecast area.

Figure 17. The Pueblo WFO Weather Story graphic shows the area where both a Dust Storm and a High Wind Warning had been issued.

Social media is also used to help convey warnings and other information from a WFO.  In Figure 18 is an example of such a product from the AMA WFO, highlighting the area of dust near LBB and the “Wall of dust” approaching from the north.  An image posted by NWS personnel from the WFO, along with another image as the dust entered a neighborhood, both from the WFO Facebook page, are shown in Figure 19.

Figure 18. A graphic image posted by WFO AMA on their Facebook page showing the dust areas.

Figure 19. Photos of the dust on the AMA WFO Facebook page from the late afternoon on 18 March.

The Weather Story issued by the LBB WFO late in the afternoon on 18 March also nicely describes in graphical form the two areas of dust (Figure 20).

Figure 20. Weather Story graphic from the LBB WFO.

A picture posted on their Facebook page shows the dusty scene in the afternoon in the area of dust that persisted ahead of the cold front (Figure 21).

Figure 21. Dusty scene in Lubbock, Texas in the dust area ahead of the cold front during the afternoon of 18 March, posted on the WFO LBB Facebook page.

Posted in Blowing Dust (Blue-light absorption technique) | 1 Comment

More blowing dust with strong cold front on 11 March 2014

A strong cold front moved south across the High Plains on Tuesday afternoon and evening, bringing an episode of blowing dust with it.  Here we look at what happened and how it appeared with some GOES-R Proving Ground products that highlight blowing dust.  The sequence of surface maps displayed below in Figure 1 show the southward plunge across the plains east of the Front Range, with very strong northerly winds pushing the cold air rapidly southward.  It appears that the strongest northerly winds (20 to 30 knots sustained with gusts over 40 knots) occur behind the initial frontal surge.

Figure 1. Sequence of surface plots showing the push of cold air southward on 11 March.

One of the problems that operational meteorologists have when it comes to blowing dust is that it can be hard to see in conventional visible satellite imagery.  We demonstrate this with the GOES visible image below taken from AWIPS.

Figure 2. Visible satellite image at 1745 UTC with METAR observations.

A number of stations report visibility restrictions due to haze (in southeastern Colorado) or haze and blowing dust (for example, KGCK in southwestern Kansas).  But it is difficult to see this dust in the image.  The CIRA MODIS dust products use the 11 and 12 micrometer thermal IR bands form the Moderate Resolution Imaging Spectroradiometer (MODIS) instruments which fly on the polar-orbiting NASA Terra and Aqua satellites to highlight dust in either yellow or pink.  Because the satellites are Polar orbiters we only get one pass each during the daytime over the area of interest.  An example of each product is shown below for the pass closest to the time of the image shown in Figure 2.

Figure 3. CIRA yellow dust product for 1805 UTC, with METARs.

Figure 4. Pink dust product for 1805 UTC on 11 March.

Both dust products clearly highlight the most intense areas of blowing dust, which are found in southeastern Colorado at 1805 UTC.  A similar comparison is made below for the time of the next pass at 1945 UTC, in Figures 5-7 below (note that for this time we have a visible image at the same time).

Figure 5. GOES visible image from AWIPS at 1945 UTC with 2000 UTC METARs.

Figure 6. CIRA yellow dust product for 1945 UTC with 2000 UTC METARs.

Figure 7. CIRA pink dust product for 1945 UTC.

Blowing dust can be a significant hazard to all modes of travel, and in an earlier blog we documented traffic accidents that occurred during a dust storm earlier this winter in eastern Colorado.  The National Weather Service (NWS) Weather Forecast Offices (WFOs) at Boulder and Pueblo issued Dust Advisories for this event (shown below in Figures 8 and 9) and included discussion of the dust in their “Weather Stories” (Figures 10 and 11).

Figure 8. Boulder WFO forecast graphic page for Tuesday afternoon showing the location of the Dust Advisory.

Figure 9. Pueblo WFO forecast graphic page for Tuesday afternoon showing the location of the Dust Advisory.

Figure 10. Boulder WFO "Weather Story" graphic page for Tuesday afternoon.

Figure 11. Pueblo WFO forecast graphic page for Tuesday afternoon.

The strong winds and dust moved south into the Texas Panhandle during the late afternoon and evening hours of Tuesday (after 0000 UTC on 12 March).  An extraordinary photo taken from a low flying aircraft was posted on the WFO Amarillo Facebook Page and is shown below.

Figure 12. Great view of the arc of dust (with some small clouds) moving south near Amarillo, Texas, as taken from a low-flying aircraft. Courtesy of WFO Amarillo.

The dust then moved further south into the Lubbock (LBB) WFO forecast area.  WFO LBB made an excellent post on this event (see http://www.srh.noaa.gov/lub/?n=events-2014-20140311-wind) and images below are taken from this summary.  The first one is a view of the dust at sunset (about 8 PM Local Time) approaching Lubbock (Figure 13).  Their graphic summary of the event follows in Figure 14, then in Figure 15 is a summary of wind gusts in the WFO LBB forecast area.

Figure 13. View of the approaching dust from Lubbock, Texas near 8pm on Tuesday, 11 March.

Figure 14. Description of the dust event from WFO LBB.

Figure 15. Collection of wind gust reports (mph) from WFO LBB.

The METAR observations from LBB nicely show a period of blowing dust that continued for several hours, as shown below in the last figure.

Figure 16. METAR observations for KLBB from 1053 UTC on 11 March (bottom) to 1153 UTC on 12 March (top).

Posted in Blowing Dust (Blue-light absorption technique), Blowing Dust Detection (Split-window technique) | Leave a comment

Great Lakes Ice Cover

The exceptionally cold winter over the Great Lakes region has led to relatively high ice coverage across the Great Lakes.  The GLERL analysis of ice cover percentage across the Great Lakes is 91% as of March 4:

To put this into a historical perspective, the ice coverage across the Great Lakes is highest since 1980 according to this image from the Canadian Ice Service (Environment Canada):

The highest Great Lakes ice coverage is just prior to the above graph at 95% set in 1979.

Given the historical level of ice coverage across the Great Lakes, it is of interest to look at satellite imagery of the ice cover on the Great Lakes.  First we will look at a VIIRS image (courtesy CIMSS at University of Wisconsin – Madison):

Click on the image then click “full size is 3055 x 1499″ to see the image at highest resolution.  One of the noteworthy aspects of the image are the cracks evident in the ice evident on the Great Lakes.  These cracks can be seen to move in animated geostationary satellite imagery from the GOES satellite (imagery provided by Dan Lindsey):

The winds at low-levels play a key role in the distribution of cracks along the ice.

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A look at the 16 Jan 2014 dust storm in eastern Colorado using VIIRS imagery

Strong winds coupled with dry soil led to widespread blowing dust across the eastern plains of Colorado and areas east on Thursday 16 January 2014.  A short video clip shows the blowing dust obscuring visibilities in Logan County in far northeastern Colorado (see www.youtube.com/watch?v=uxMdMTzlRFI ).  The lowered visibilities in the blowing dust resulted in a multi-car accident that closed Interstate 70 near Burlington Colorado (close to the Kansas border) for several hours from 11:30 AM MST to 4:25 PM (1830 to 2325 UTC).  A story of the dust storm and the accidents that closed Interstate 70,  courtesy of Denver 7 News, can be found here http://www.thedenverchannel.com/news/local-news/dust-storm-closes-eb-i-70-us-24-to-kansas-line-us-34-closed-as-poor-visibilty-causes-accidents.

Below is a surface plot from early afternoon on the 16th showing sustained wind speeds of 30 to 40 knots with gusts as high as 55 knots.

Surface plot at 2043 UTC on 16 January.

In this blog entry we will take a look at how the dust appeared in standard GOES visible imagery and compare this to different imagery from the SUOMI NPP VIIRS instrument Polar satellite.  Some of the images we will show demonstrate the capabilities that will be available when GOES-R is launched.

We start with a look at “standard” GOES visible imagery during the event, shown for two times below.  In the visible images the plains of eastern Colorado and surrounding areas have a collection of clouds at different levels in addition to some areas of old snow cover as well as the blowing dust.  From this imagery alone it is difficult to distinguish between these.

Shown below is similar type of visible satellite imagery but using VIIRS with a natural color background and of course higher spatial resolution (~0.5 km vs 1.o km from the current GOES).  Right away we can see that the improved contrast and resolution allows one to see dust plumes in the first image below from 1848 UTC, but things are not so apparent in the second image from 2029 UTC.

VIIRS True Color visible satellite image at 1848 UTC on 16 January.

VIIRS True Color visible image at 2029 UTC on 16 January.

Using different bands from VIIRS a specialized type of imagery can be created which isolates the dust, making it stand out far more clearly.  CIRA creates two types of dust discrimination imagery, one with the dust highlighted in yellow and the other where the dust has a pinkish color, as shown below.  The purpose of these products is to clearly isolate dust from other surrounding clouds and general background.

Pink dust product using NPP VIIRS imagery at 1848 UTC on 16 January

Pink dust product using NPP VIIRS imagery at 2029 UTC on 16 January

The above imagery is especially useful for the 2029 UTC time, when the earlier visible satellite image showed a more complex mix of dust and clouds.  Similar imagery is also made using MODIS Polar orbiting satellites.  Shown below are the pink and yellow dust products using the MODIS Aqua satellite imagery at 2020 UTC.

Pink dust product using Aqua MODIS imagery at 2020 UTC on 16 January.

Yellow dust product using Aqua MODIS imagery at 2020 UTC on 16 January

We noted earlier that there was also snow in the background in some spots across the Plains, as well of course in the mountains.  The next set of imagery shows the CIRA snow/cloud (discriminates snow from clouds) and snow/cloud layer (further discrimination of the type of clouds, pinkish for generally higher ice clouds and yellow for generally lower water clouds).

Snow/cloud discriminator product using NPP VIIRS imagery at 1848 UTC on 16 January

Snow/cloud layer discriminator product using NPP VIIRS imagery at 1848 UTC on 16 January

Snow/cloud discriminator product using NPP VIIRS imagery at 2029 UTC on 16 January

The snow/cloud layer discriminator product uses the 1.38 micron “cirrus” band to isolate higher level ice clouds (an added step from the binary snow/cloud discriminator product).  An example of the cirrus imagery by itself is shown below for the 2020 UTC time.

Cirrus product using Aqua MODIS imagery at 2020 UTC on 16 January

Posted in Blowing Dust (Blue-light absorption technique), Blowing Dust Detection (Split-window technique), MODIS Snow/Cloud Discriminator | 1 Comment

Fog and Low Clouds in Eastern Colorado as seen with GeoColor and Day Night Band NPP VIIRS imagery on 20 Dec 2013

The Suomi NPP VIIRS Day/Night Band (DNB), which can use moonlight to produce visible-light imagery during the nighttime, offers a unique capability that is slated to continue on the JPSS constellation concurrent to the GOES-R era.  This presents intriguing potential for synergy between the DNB and Advanced Baseline Imager.  One can use the imagery just as visible imagery is currently used in the daytime, so there are many applications.  Here we show how fog and low clouds distinctly appear during the nighttime hours using the DNB imagery, shown below first on a larger scale and then zoomed in over Colorado.

DNB imagery over the western half of the CONUS at 0914 UTC on 20 December 2013.

DNB imagery centered over Colorado at 0914 UTC on 20 December 2013.

Lights from the various towns and cities are seen in the DNB imagery.  City lights are also a part of one of the earlier CIRA Proving Ground demonstration imagery known as GeoColor imagery.  GeoColor is intended to be a survey type imagery that has a seamless transition from night to day by combining different bands and background imagery.  The current version uses a static nightime background of city lights (though it will be possible to update to quasi-real time imagery using Polar satellites), as seen in the image below for the same time as the DNB images displayed above.  An added feature of the GeoColor imagery is the use of the 11-3.9 micron difference (the standard AWIPS fog product) to color low clouds and fog in a pinkish tone to highlight them from other clouds, as seen below.  One characteristic of the imagery that has been noticed during cases of fog is that there may be some information about the thickness and/or density of the fog by how much of the city lights appear through the fog layer, and it will be interesting to examine more DNB imagery in this regard.

GeoColor imagery over the western half of the CONUS at 0945 UTC on 20 December 2013.

Note how in the GeoColor imagery higher clouds appear in white tones, and we can see that high clouds extend across portions of eastern Colorado, covering the lower clouds and fog.  However, going back to the DNB imagery,  the cirrus barely shows in this imagery (as it would with visible imagery in the daytime) and we are therefore able to see the low clouds and fog more clearly.  This example shows how VIIRS and GOES-R could be used in synergy during the GOES-R era.

Posted in GeoColor Imagery, Uncategorized | 1 Comment