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Rim Fire map, with color scheme indicating the USFS estimated daily fire progression based on the NIROPS observation closest to local midnight for 17 August to 22 September 2013. Solid blue and dashed black arrows indicate the approximate area burned during spread event #1 and spread event #2, respectively. 

Rim Fire map, with color scheme indicating the USFS estimated daily fire progression based on the NIROPS observation closest to local midnight for 17 August to 22 September 2013. Solid blue and dashed black arrows indicate the approximate area burned during spread event #1 and spread event #2, respectively. 

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The 2013 Rim Fire, which burned over 104,000 ha, was one of the most severe fire events in California’s history, in terms of its rapid growth, intensity, overall size, and persistent smoke plume. At least two large pyrocumulonimbus (pyroCb) events were observed, allowing smoke particles to extend through the upper troposphere over a large portion o...

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... conditions. The intense burning and rapid spread observed during the primary burning period of 17-31 August generally coincided with warm temperatures and relative humidity (RH) values below 40% each afternoon. However, several key changes in local meteorology were also observed. During the first few days of the fire, a large portion of California was under the influence of a broad upper-level low that became cutoff from the mean synoptic flow in the days preceding ignition (Fig. 3a). The North American Regional Reanalysis (NARR; #narr_datasets; Mesinger et al. 2006) shows that the center of the low was located off the southern California coastline on the first day of burning (18 August), and low-level winds (850 hPa) were light and southeasterly near the Rim Fire. As is typical with large cutoffs, the low then began to retrograde (e.g., Holton 2004), causing low-level winds near the fire to shift more northerly by the evening of 19 August (Fig. 4a). This directed the fire front to the south, or generally downhill (Fig. 1). During 20 - 22 August, the low progressed back toward California, causing low-level winds to become southwesterly (Fig. 4b- d), redirecting the fire to the northeast along generally uphill slopes (Fig. 1). As near-surface pressure gradients increased between the low and an inland ridge, wind speeds increased from 5 kt (3 m·s ) to 15-20 kt (8-10 m·s ). This combination of stronger winds in a general uphill and up-canyon direction very likely increased the rate of fire spread. Relatively cold upper-tropospheric air associated with the cutoff low provided sufficient instability for scattered convection and some precipitation in the higher terrain near the fire. The two pyroCb events also occurred during this period, on 19 and 21 August. Convective activity then diminished as the cutoff low merged with a broad synoptic trough approaching the Pacific Northwest. Southwesterly synoptic flow on the eastern side of the trough pushed the ...
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... conditions. The intense burning and rapid spread observed during the primary burning period of 17-31 August generally coincided with warm temperatures and relative humidity (RH) values below 40% each afternoon. However, several key changes in local meteorology were also observed. During the first few days of the fire, a large portion of California was under the influence of a broad upper-level low that became cutoff from the mean synoptic flow in the days preceding ignition (Fig. 3a). The North American Regional Reanalysis (NARR; #narr_datasets; Mesinger et al. 2006) shows that the center of the low was located off the southern California coastline on the first day of burning (18 August), and low-level winds (850 hPa) were light and southeasterly near the Rim Fire. As is typical with large cutoffs, the low then began to retrograde (e.g., Holton 2004), causing low-level winds near the fire to shift more northerly by the evening of 19 August (Fig. 4a). This directed the fire front to the south, or generally downhill (Fig. 1). During 20 - 22 August, the low progressed back toward California, causing low-level winds to become southwesterly (Fig. 4b- d), redirecting the fire to the northeast along generally uphill slopes (Fig. 1). As near-surface pressure gradients increased between the low and an inland ridge, wind speeds increased from 5 kt (3 m·s ) to 15-20 kt (8-10 m·s ). This combination of stronger winds in a general uphill and up-canyon direction very likely increased the rate of fire spread. Relatively cold upper-tropospheric air associated with the cutoff low provided sufficient instability for scattered convection and some precipitation in the higher terrain near the fire. The two pyroCb events also occurred during this period, on 19 and 21 August. Convective activity then diminished as the cutoff low merged with a broad synoptic trough approaching the Pacific Northwest. Southwesterly synoptic flow on the eastern side of the trough pushed the ...
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... and ejected it through central California between 21 and 22 August (Fig. 3a). The digging trough also maintained a strong pressure gradient over central California, producing strong surface winds (Fig. 4d). This coincides with the rapid uphill fire spread observed during spread event #1 (Fig. 1), marked by the largest increases in both area burned and FRP (Fig. 2). During 24 August and part of 25 August, the Rim Fire’s growth slowed and FRP decreased (Figs. 1, 2). This was largely influenced by increasing RH, reduced wind speed, and the lowest surface temperatures observed during the primary burning period. While the air temperature was lower, the passage of a shortwave trough (Fig. 3b) caused low-level wind speeds to increase again during the afternoon and evening of 25 August, coinciding with the initiation of spread event #2. By the end of August, temperatures warmed and RH values reached another relative minimum. However, surface wind conditions were not as favorable as during the major spread events. Portions of the fire were also becoming increasingly contained, either by fire suppression teams or natural barriers. As a result, extreme fire spread did not occur. Burning continued through 10 September at a slower rate of spread than the primary burning period (Figs. 1, 2). During 11-21 September, FRP dropped significantly and very slow growth was observed. The first substantial (> 12 mm) synoptic rainfall occurred on 21-22 September, effectively ending the satellite fire detection record for the Rim Fire (Fig. 2). However, smoldering and occasional weak flare-ups continued into early October. A variety of fire weather indices are currently available to forecast the potential for “extreme fire danger” across North America. In the Continental United States ...
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... fire weather forecasts commonly employ the Haines Index: an integer scale (1-6) based on two equally weighted ingredients for moisture and stability, respectively derived from a lower-level (850 or 700 hPa) dew point depression and lower atmospheric lapse rate (Haines 1988; Potter et al. 2008). The specific pressure levels used for the Haines Index calculations vary, depending on local topography. The majority of the Rim Fire’s primary burning period, including spread event s #1 and #2, was marked by a dry lower troposphere, with a low-level thermal lapse rate near dry- adiabatic. As a result, all fire weather indices, including the Haines Index, indicated maximum fire danger (value of 6) nearly every afternoon. Figure 5 highlights the high Haines Index environment on the first afternoon of spread event #1 (22 August), using the NARR-derived sounding for the Rim Fire coincident with the Aqua MODIS overpass at 2130 UTC. The upper limit of the Haines Index can be extended for increased sensitivity to the most extreme fire danger (Mills and McCaw 2010). However, this “Continuous Haines Index” also produced values near the 95 percentile of fire danger (value of ~8-10). Therefore, lower-atmospheric fire weather indices, such as the Haines Index, lack the fidelity for distinguishing days with extreme fire spread from those with more gradual spread. During the Rim Fire, the largest spread and FRP was generally initiated as an upper-level disturbance passed over (or near) the fire (Fig. 3). A similar link has been highlighted by previous studies (e.g., Brotak and Reifsnyder 1977; Westphal and Toon 1991; Werth and Ochoa 1993). The impact on surface wind speed and RH is inferred from Fig. 6, using hourly observations from the Remote Automatic Weather Station (RAWS, at Crane Flat Lookout (37.76 N, 119.82 W, elevation of 2025.1 m; Fig. 1). These data confirm that spread event #1 coincided with some of ...
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... 6. Primary burning period surface observations (black curve) of hourly mean wind speed (top) and relative humidity (bottom) from the RAWS station at Crane Flat Lookout ( located within Yosemite National Park at 37.76°N, 119.82°W (Fig. 1), with an elevation of 2025.1 m (6644 ft). Daytime (green triangles) and nighttime means (blue circles) were calculated using the hours of 16-03 UTC (9 AM - 8 PM) and 04-15 UTC (9 PM - 8 AM), respectively. The time series of cumulative fire area based on nighttime NIROPS observations is displayed in red. Spread events #1 and #2 are highlighted with yellow shading, and the approximate time of the shortwave passage (8/25, evening) is denoted by the dashed brown vertical line.  ...
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... and relative humidity (bottom) from the RAWS station at Crane Flat Lookout ( located within Yosemite National Park at 37.76 N, 119.82 W (Fig. 1), with an elevation of 2025.1 m (6644 ft). Daytime (green triangles) and nighttime means (blue circles) were calculated using the hours of 16-03 UTC (9 AM - 8 PM) and 04-15 UTC (9 PM - 8 AM), respectively. The time series of cumulative fire area based on nighttime NIROPS observations is displayed in red. Spread events #1 and #2 are highlighted with yellow shading, and the approximate time of the shortwave passage (8/25, evening) is denoted by the dashed brown vertical ...
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... Using these resources, the limitations of traditional fire weather indices and conflicting hypotheses surrounding pyroCb development are examined. Variations in smoke plume altitude and transport are also explored. Therefore, the analysis of the Rim Fire is an important step toward improving methodologies currently used for regional fire weather, air quality, and visibility forecasts. Using nightly airborne-based observations, the United States Forest Service (USFS) National InfraRed OPerationS (NIROPS) provides fire perimeter maps and burned area estimates for many fire events, especially when there is an immediate risk to life and property ( NIROPS analyses were posted at an irregular schedule during the Rim Fire, generally between 03 and 09 UTC (9 PM - 3 AM local time). Figure 1 displays the estimated daily fire progression based on the NIROPS observation closest to local midnight each day. Steady growth was observed for the first two days (17-18 August), with the fire front generally spreading in all directions. On 19 August, the front was displaced noticeably to the south. By 20 August, the direction of spread shifted to the east-northeast and the rate of spread increased further, exploding in relative size during the evening of 21 August. As shown in Fig. 2 (red curve), this period of extreme fire spread (spread event #1) persisted through 23 August, burning 36206 ha (~35% of the total burned area). A second significant spread event (#2) began during the evening of 25 August, and burned 12067 ha (~12% of the total) by the evening of 26 August. Several space-borne sensors have fire detection capabilities, and are typically used in combination with (or in place of) NIROPS burned area estimates. The ...

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... During June-August 2013, 88 enormous wildfires were observed in Western North America, producing 26 intense pyroCb storms [24]. One of the biggest wildfires in the history of California was reported to burn around 104,000 ha of land and created two intense pyroCb events [25]. ...
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... PyroCb development is a dynamic process of fire-atmospheric coupling that is driven by the interaction of large and vigorous wildfires and favorable meteorological conditions. Most pyroCb events begin with an extreme fire capable of developing a deep convective plume, while requiring instability and moisture aloft to facilitate condensation, latent heat release, and subsequent enhancement of the buoyancy of growing convective cells [9,[17][18][19]. Therefore, analysis and prediction of pyroCb development is often based on atmospheric indices, which measure atmospheric instability, and surface-based fire risk indices, which measure the potential for fire development. ...
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... Peaks in FRP during the Rim Fire likely coincided with the most intense burning (Fig. 3.7). Although diurnal variability in FRP is evident, it is equally evident that variation in FRP does not follow a simple diurnal distribution as Peterson et al. (2015) described for the Western Regional Air Partnership and Western Governors Association (Air Resources Inc. 2005). The co-occurrence of high FRP on days with weaker atmospheric stability is likely tied to a greater vertical extent of the smoke plumes and an enhanced probability of smoke injection into the free troposphere (Val Martin et al. 2010;Peterson et al. 2014). ...
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