Masthead: Kaweah Range

Sierra Nature Notes, Volume 3, December 2003

Persistence of pikas, Cont'd (pg 3 of 5)

Discussion

Persistence of low-elevation pikas: climatic and other influences
Loss of pika populations from lower elevations and latitudes, such as the loss of nearly 30% of interior Great Basin populations recorded during the 20th century, is consistent with losses that have occurred over the last 14,000 years (Grayson 1993). Given the recent extirpation of pikas from low-elevation sites within 150 km (93 mi) of Lava Beds (Beever 1999; fig. 2), current persistence of pikas in Craters and Lava Beds National Monuments is noteworthy. Although population losses in the Great Basin occurred not surprisingly at sites that were drier and warmer than those at which populations persisted, estimated climates at Lava Beds and Craters were notably drier and hotter than even those locations in the Great Basin where pikas have been recently extirpated. However, the tubes, caves, and deep, complex lava formations that occur across both monuments undoubtedly provide pikas with relatively cool refugia during times of heat stress. Interestingly, though, pikas were not exclusively confined to caves and lava tubes during my July surveys, suggesting that temperature influences provide only a partial solution to the mystery of how pikas persist in these monuments. Pika behavior plays a substantial role in mediating the effects of thermal stress, and measuring temperature regimes that pikas experience throughout the day and across seasons may provide another clue to understanding how they persist in these low-elevation areas.

“Pika behavior plays a substantial role in mediating the effects of thermal stress....”

Table 1: Locations sampled for pikas in Lava Beds and Craters of the Moon National Monuments, July 1995.

 

Location

Elevation (m)

Search effort (hr)*

Date of Historic record, if available

Pikas detected in 1995 survey?

LAVA

BEDS

Heppe Ice Cave

1610

0.75

1991

No

Catacombs parking lot

1525

2.00

1961, 1962

Yes

Juniper Cave

1510

0.50

1960

No

Catacomb Cave , upper Sentinel entrance

1490–1525

2.50 [3]

1963

Yes

Maze Cave collapse

1490

1.00 [2]

 

No

Merrill Ice Cave

1490

1.50

1962

Yes

Thunderbolt Cave , upstream entrance

1490

0.25

1990

No

Lower Sentinel entrance

1475

0.75 [3]

 

Yes

Indian Well Cave

1450

0.50

 

Yes

Symbol Bridge

1440

1.00 [3]

1972

Yes

Skull Cave road

1400

1.00

 

No

Fleener Chimneys area

1365

0.75

1984

Yes

Schonchin Lava Flow

1340

1.00

 

No

Trail to Black Crater; Battlefield Trail

1340

0.75

 

Yes

Devil’s Homestead Lava Flow

1280

0.50

 

No

TOTALS (N = 15 sites, 22 searches)

Mean = 1450 m

16.0 hr

 

10 individuals

 

 

Location

Elevation (m)

Search effort (hr)*

Date of Historic record, if available

Pikas detected in 1995 survey?

CRATERS

 

OF

 

THE

 

MOON

North Crater Flow trail

1830

2.00

1990

Yes

Base of North  Crater

1830

1.25

 

Yes

Scenic turnout near Spatter Cones parking lot

1830

1.00

 

No

Highway Flow

1810

4.00 [2]

 

No

Spatter Cones, trail to Big Crater

1810

2.25

 

Yes

Trail to Buffalo Caves

1790

0.75

 

Yes

Picnic table turnout

1780

1.00

 

Yes

Base of Big Sink, Tree Molds Road

1780

0.75

 

Yes

Jct of main loop road and Tree Molds road

1780

0.50

1990

No

Caves Area Trail to Needles Cave

1760

3.25

 

Yes

Devil’s Orchard Trail

1750

3.25

1989, 1990

Yes

Caves Area Trail

1750

2.25

1991

Yes

TOTALS (N = 12 sites, 13 searches)

Mean = 1790 m

18.5 hr

 

27 individuals

* Number of searches (if >1) appear in brackets

In both monuments, pikas apparently use habitats that fulfill three requirements. First, pikas generally inhabit large, contiguous areas of (rocky) volcanic habitat, as opposed to isolated pockets of lava formations. Second, although pikas were not always located near edges of lava flows, areas with pikas possessed average or greater amounts of vegetation accessible within distances comparable to dimensions of home ranges. Finally, pikas appeared to be associated at the fine scale with microtopography characterized by rocks large enough to provide space for subsurface movement and tunneling (as is found in aa and block lava flows), as opposed to the smooth pahoehoe lava flows that have little relief. Because collapsed lava tubes, lava flow margins, cave entrances, fault scarps, fault cracks, and internal talus zones all provide talus-like areas that pikas may inhabit, geologic mapping of the monuments may provide additional insight into pika distribution.

Continued Next Page

 

 

 



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