Comparing methods for sampling large- and medium-sized mammals: camera traps and track plots

Activities involving fauna monitoring are usually limited by the lack of resources; therefore, the choice of a proper and efficient methodology is fundamental to maximize the cost-benefit ratio. Both direct and indirect methods can be used to survey mammals, but the latter are preferred due to the difficulty to come in sight of and/or to capture the individuals, besides being cheaper. We compared the performance of two methods to survey medium and large-sized mammal: track plot recording and camera trapping, and their costs were assessed. At Jatai Ecological Station (S21 degrees 31`15 ``- W47 degrees 34`42 ``-Brazil) we installed ten camera traps along a dirt road directly in front of ten track plots, and monitored them for 10 days. We cleaned the plots, adjusted the cameras, and noted down the recorded species daily. Records taken by both methods showed they sample the local richness in different ways (Wilcoxon, T=231; p;;0.01). The track plot method performed better on registering individuals whereas camera trapping provided records which permitted more accurate species identification. The type of infra-red sensor camera used showed a strong bias towards individual body mass (R(2)=0.70; p=0.017), and the variable expenses of this method in a 10-day survey were estimated about 2.04 times higher compared to track plot method; however, in a long run camera trapping becomes cheaper than track plot recording. Concluding, track plot recording is good enough for quick surveys under a limited budget, and camera trapping is best for precise species identification and the investigation of species details, performing better for large animals. When used together, these methods can be complementary.

Lacustrine records of Holocene flood pulse dynamics in the Upper Paraguay River watershed (Pantanal wetlands, Brazil)

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Recognition of Cretaceous, Paleocene, and Neogene tectonic reactivation through apatite fission-track analysis in Precambrian areas of southeast Brazil: Association with the opening of the south Atlantic Ocean

Apatite fission-track analysis was used for the determination of thermal histories and ages in Precambrian areas of southeast Brazil. Together with geological and geomorphologic information, these ages enable us to quantify the thermal histories and timing of Mesozoic and Cenozoic epirogenic and tectonic processes. The collected samples are from different geomorphologic blocks: the high Mantiqueira mountain range (HMMR) with altitude above 1000 m, the low Mantiqueira mountain range (LMMR) under 1000 m, the Serra do Mar mountain range (SMMR), the Jundiá and Atlantic Plateaus, and the coastline, all of which have distinct thermal histories. During the Aptian (∼120 Ma), there was an uplift of the HMMR, coincident with opening of the south Atlantic Ocean. Its thermal history indicates heating (from ∼60 to∼80 °C) until the Paleocene, when rocks currently exposed in the LMMR reached temperatures of ∼100 °C. In this period, the Serra do Mar rift system and the Japi erosion surface were formed. The relief records the latter. During the Late Cretaceous, the SMMR was uplifted and probably linked to its origin; in the Tertiary, it experienced heating from ∼60 to ∼90 °C, then cooling that extends to the present. The SMMR, LMMR, and HMMR were reactivated mainly in the Paleocene, and the coastline during the Paleogene. These processes are reflected in the sedimentary sequences and discordances of the interior and continental margin basins. © 2002 Elsevier Science Ltd. All rights reserved.

Astroparticle physics with nuclear track detectors

This thesis is mainly about the search for exotic heavy particles -Intermediate Mass Magnetic Monopoles, Nuclearites and Q-balls with the SLIM experiment at the Chacaltaya High Altitude Laboratory (5230 m, Bolivia), establishing upper limits (90% CL) in the absence of candidates, which are among the best if not the only one for all three kind of particles. A preliminary study of the background induced by cosmic neutron in CR39 at the SLIM site, using Monte Carlo simulations. The measurement of the elemental abundance of the primary cosmic ray with the CAKE experiment on board of a stratospherical balloon; the charge distribution obtained spans in the range 5≤Z≤31. Both experiments were based on the use of plastic Nuclear Track Detectors, which records the passage of ionizing particles; by using some chemical reagents such passage can be make visible at optical microscopes.

Jack Harvey, UM Men's Track Coach, 1994

[at 1994 Len Paddock Meet]

1977 UM Track Team

Top Row: Calvin Williams, Mike Boehmer, Tim Thomas, Dan Heikkinen, Greg Thomas, Scott Walters, Sam Angell, Mike Hetes.

3rd Row: asst. coach Greg Syphax, Doug Sweazey, Bruce McFee, Jim Baumgartner, Charles Crouther, Jay Anstaett, Gary Hicks, Warren T. Dobson, James Henry.

2nd Row; Bob Scheper, Arnett Chisholm, John Risk, Don Wheeler, Randy Foss, Lynn Dobosy, Scott Hurd, asst. coach Ron Warhurst

Front Row: Steve Elliott, Bill Donakowski, James Grace, co-captain Jeff McLeod, coach Jack Harvey, co-captain Greg Meyer, Andy Johnson, Dave Furst, Doug Hennigar.

1981 UM Track Team

Top Row: Mike Murphy, Chris Fitzpatrick, Phil Wells, James Ross, Dave Walmroth

4th Row: Dave Hall, Scott Ericksson, George Yoanides, Dave Lugin, Johnny Nielsen, Mike Finn

3rd Row: asst. coach Ron Warhurst, Dorian Diemer, Gerard Donakowski, Derek Harper, Bill O'Reilly, Vern Rottman

2nd Row: James Henry, Shelby Johnson, Andrew Bruce, Butch Woolfolk, Mike Shea, Craig Camp, Kent Bernard

Front Row: Dan Beck, Bill Weidenbach, Darold Gholston, coach Jack Harvey, Dave Lewis, Ken Gardner

Not Pictured: Marshall Parks, Tony Krpan, Mark Pruente, Vince Bean, Doug Heikkinen, Dan Heikkinen