Harvest system selection and design for damage reduction in noble fir stands : a case study on the Warm Springs Indian Reservation

Many high-elevation stands of noble fir in the northern Oregon Cascades are being actively managed. Forest managers are investigating different activities that will control stand impacts and the subsequent spread of Heterobasidion annosum a rot pathogen on the Warm Springs Indian Reservation. The purpose of this study was to quantify the relationship of logging production and costs with associated residual stand damage during a commercial thinning operation. Investigated in the study were four ground-based harvesting systems and two different harvest unit layout methods. The harvest systems encompassed a variety of equipment and mechanization levels ranging from mechanized felling and bunching with grapple skidders to manual felling, limbing, and bucking using a rubber-tired skidder equipped with a winch line. In addition, each harvest system was compared using two layout methods. The first method was conventional or logger's choice and the second was a designated method incorporating proven methods for reducing stand damage. Log lengths varied from whole-tree to log-length depending on the harvest system employed. Logging production and costs were determined for the harvesting systems using a combination of detailed and shift level time studies. A stand damage survey conducted simultaneously with production studies determined percent residual stand damage, specific equipment causing damage, and individual scar characteristics. Harvesting costs for the four different systems and layout methods ranged from $67.77/MBF-$92.68/MBF, with residual stand damage of 20.12-62.62%. Equipment size, log lengths, and layout method were found to affect total residual stand damage. Reducing the use of larger, more mechanized pieces of equipment in the stand and keeping log length to a minimum resulted in a significant decrease in residual stand damage. Cost differences between designated and conventional layout methods for each harvest system were minimal. The main difference in harvesting cost was between the different systems and log lengths. Harvesting costs varied, being similar for the highest and lowest mechanized systems but increasing with the intermediate harvesting systems

Thinning with prescribed fire and timber harvesting mechanization for fuels reduction and forest restoration

In the Blue Mountains of northeastern Oregon, prescribed fire and mechanical harvesting economics were investigated for fuels reduction and forest restoration. Using a cut-to-length harvesting system, three single-grip harvesters and three forwarders produced significantly different production rates. For the harvesters, significant variables that affected production rates were found to be: harvested material removed (live tree, standing dead tree, or downed wood), tree species, tree diameter, and distance traveled between processing. For the forwarder, significant variables that affected production rates were forwarding distance and the number of stops required to accumulate its rated payload. From the thinning, net revenues per acre ranged from $143 to$718 and averaged $315. Prescribed fire costs ranged from$24 to $87 per acre and averaged$51. Prescribed fire intensity was found to be significantly higher in the mechanically thinned stands with tons of downed woody material being a significant predictor of fire intensity. Mean fire intensity was found to be 94.7° and 157.6° Celsius for the burn and thin and burn treatments, respectively. The addition of activity fuel from the mechanical thinning was the primary factor that increased fire intensity. From the production data, net revenue was determined for stump-to-mill operations and predictive equations were used to develop a cost model that investigated stand conditions of significance. This information provided a framework for conducting sensitivity analysis on the effects of these significant variables to production and cost at differing levels. Equations were derived from the simulations and used to determine alternative scenarios for stand conditions in and around the study area. The economics of fuels reduction and forest restoration needs to proceed with an increased level of cost analysis. While many areas in need of fuels reduction have produced positive net revenues, others have produced a loss. Land mangers need to understand how equipment selection, material removed, stand conditions, market prices, and market locations affect harvesting costs and net revenue. Information provided in this paper can be used by land managers to aid in assessing the economic feasibility of a given operation and determine which treatment combinations are optimal

Response of reverse convection to fast IMF transitions

The nature of the transition that high‐latitude reverse convection makes in response to fast interplanetary magnetic field (IMF) changes is investigated using observations from multiple spacecraft and a ground magnetometer array. We focused on two fast IMF‐transition events on 22 April 2006. Immediately after the first event, three ST5 spacecraft identified a clear change in the distribution of the polar cap field‐aligned current. Coordinate observations with the Greenland magnetometer chain showed that the near‐noon Hall current distribution, which is closely related to the polar cap field‐aligned current or reverse convection, was in a transition state for about 10 min. For the second event, the Greenland magnetic perturbations also showed that a transition state occurred in the near‐noon sector for 10–15 min. Three DMSP spacecraft that traversed the polar cap provided evidence showing that variations of the ground magnetic perturbations were produced by the transition from clockwise plasma circulation to the anticlockwise circulation over the polar cap. A simple calculation based on the Biot‐Savart law shows that the near‐noon transition state is consistent with the approach of a new convection region to the near‐noon sector at the speed of 0.5–1 km s–1, which is coupled with the moving away of the old convection region at a similar speed. For the higher‐latitude sunward flow region, it is found that the convection takes a transition state almost simultaneously (within 1 min) with that in the near‐noon sector, i.e., quasi‐instantaneous response.Key PointsTransition state with a timescale of ~10 min in the near‐noon polar cap for BZ > 0The state is consistent with the passage of old and new convection regionsAlmost simultaneous initial response in the upstream polar cap and the near noonPeer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/111947/1/jgra51794.pd

A low-power data acquisition system for geomagnetic observatories and variometer stations

A modern geomagnetic observatory must provide data of high stability, continuity, and resolution. The INTERMAGNET network has therefore specified quantitative criteria to ensure a high quality standard of geomagnetic observatories. Here, we present a new data acquisition system which was designed to meet these criteria, in particular with respect to 1 Hz data. This system is based on a Raspberry Pi embedded PC and runs a C+ +  data acquisition software. As a result, the data acquisition system is modular, cheap, and flexible, and it can be operated in remote areas with limited power supply. In addition, the system is capable of near-real-time data transmission, using a reverse SSH tunnel to work with any network available. The system hardware was successfully tested at the Niemegk observatory for a period of 1 year and subsequently installed at the Tatuoca observatory in Brazil

Saturation magnetostriction and its low-temperature variation inferred for natural titanomaghemites: implications for internal stress control of coercivity in oceanic basalts

Highly oxidized titanomaghemite in oceanic basalts often carries remanent magnetization of high coercivity (stability), helping preserve the oceanic magnetic anomaly pattern. We study the source of this high coercivity in four oceanic basalts (from ODP sites 238, 572D, 470A and 556) containing highly oxidized titanomaghemite (titanium content parameter x ≈ 0.55 and oxidation parameter z ≈ 0.9 on average). Most of the titanomaghemite is likely in singledomain grains with uniaxial anisotropy because the ratio of saturation remanence J RS to saturation magnetization Js approaches 0.50 (JRS/JS = 0.46 on average). We show that the uniaxial anisotropy is very likely magnetostrictively controlled through internal stresses σi in the titanomaghemite grains. This allows us to use a novel indirect method to estimate the saturation magnetostriction λS of the titanomaghemite. A saturation remanence J RS is given along the axis of a cylindrical sample of each basalt. Then a small compression σ is applied repeatedly along this axis and the reversible change ∆JRS in JRS is measured. Combining equations from single-domain theory for this piezomagnetic effect and for the sample’s coercive force HC gives λS = 1.39HCJS 1/σ ∆JRS/JRS (using cgs units, or with HC in mT, J S in kA m and σ in Pa). This yields four λS estimates (with ca 50 per cent expected error) ranging from 3 × 10−6 to 10 × 10−6 and averaging 6 × 10−6. Theory for the piezomagnetic effect yields four σ i estimates averaging 2 × 108 Pa. This is similar to the internal stress magnitude thought to be responsible for the high coercivity of ball-milled single-domain titanomagnetite (x ≈ 0.6) and natural single-domain haematite. We also show that cooling to 120 ◦K causes HC J S for each oceanic basalt to vary in approximate proportion to (1− T TC)n with n between 1.9 and 2.0 (where T is temperature and T C is Curie point, both in ◦K). This implies that λS of titanomaghemite with x ≈ 0.55 and z ≈ 0.9 also varies in approximate proportion to (1− T TC)n with n near 1.9 or 2.0 on cooling to 120 ◦K (assuming that σ i remains constant on cooling). Our results support the hypothesis that coercivity (magnetic stability) is often magnetostrictively controlled by internal stresses in the highly oxidized titanomaghemites typical of oceanic basalts older than ca 10 Myr.We suggest that this hypothesis can be further tested by more extensive observation of whether cooling to 120 ◦K often causes HC J S of such basalts to vary in approximate proportion to (1 − T TC)n with n near 1.9 or 2.0

The geomagnetic observatory on Tristan da Cunha: Setup, operation and experiences

The island Tristan da Cunha is located in the South Atlantic Anomaly, and until recently the area has been one of the largest gaps in the global geomagnetic observatory network. As part of the Danish project SAADAN we set up a geomagnetic observatory on the island. Here we report on how we established the observatory in 2009 and on its operation in 2010

Using Principal Component Analysis of Satellite and Ground Magnetic Data to Model the Equatorial Electrojet and Derive Its Tidal Composition

The intensity of the equatorial electrojet (EEJ) shows temporal and spatial variability that is not yet fully understood nor accurately modeled. Atmospheric solar tides are among the main drivers of this variability but determining different tidal components and their respective time series is challenging. It requires good temporal and spatial coverage with observations, which, previously could only be achieved by accumulating data over many years. Here, we propose a new technique for modeling the EEJ based on principal component analysis (PCA) of a hybrid ground-satellite geomagnetic data set. The proposed PCA-based model (PCEEJ) represents the observed EEJ better than the climatological EEJM-2 model, especially when there is good local time separation among the satellites involved. The amplitudes of various solar tidal modes are determined from PCEEJ based tidal equation fitting. This allows to evaluate interannual and intraannual changes of solar tidal signatures in the EEJ. On average, the obtained time series of migrating and nonmigrating tides agree with the average climatology available from earlier work. A comparison of tidal signatures in the EEJ with tides derived from neutral atmosphere temperature observations show a remarkable correlation for nonmigrating tides such as DE3, DE2, DE4, and SW4. The results indicate that it is possible to obtain a meaningful EEJ spectrum related to solar tides for a relatively short time interval of 70 days

Observations of Particle Loss due to Injection-Associated Electromagnetic Ion Cyclotron Waves

We report on observations of electromagnetic ion cyclotron (EMIC) waves and their interactions with injected ring current particles and high energy radiation belt electrons. The magnetic field experiment aboard the twin Van Allen Probes spacecraft measured EMIC waves near L = 5.5–6. Particle data from the spacecraft show that the waves were associated with particle injections. The wave activity was also observed by a ground-based magnetometer near the spacecraft geomagnetic footprint over a more extensive temporal range. Phase space density profiles, calculated from directional differential electron flux data from Van Allen Probes, show that there was a significant energy-dependent relativistic electron dropout over a limited L-shell range during and after the EMIC wave activity. In addition, the NOAA spacecraft observed relativistic electron precipitation associated with the EMIC waves near the footprint of the Van Allen Probes spacecraft. The observations suggest EMIC wave-induced relativistic electron loss in the radiation belt

In situ spatiotemporal measurements of the detailed azimuthal substructure of the substorm current wedge

The substorm current wedge (SCW) is a fundamental component of geomagnetic substorms. Models tend to describe the SCW as a simple line current flowing into the ionosphere toward dawn and out of the ionosphere toward dusk, linked by a westward electrojet. We use multispacecraft observations from perigee passes of the Cluster 1 and 4 spacecraft during a substorm on 15 January 2010, in conjunction with ground-based observations, to examine the spatial structuring and temporal variability of the SCW. At this time, the spacecraft traveled east-west azimuthally above the auroral region. We show that the SCW has significant azimuthal substructure on scales of 100km at altitudes of 4000-7000km. We identify 26 individual current sheets in the Cluster 4 data and 34 individual current sheets in the Cluster 1 data, with Cluster 1 passing through the SCW 120-240s after Cluster 4 at 1300-2000km higher altitude. Both spacecraft observed large-scale regions of net upward and downward field-aligned current, consistent with the large-scale characteristics of the SCW, although sheets of oppositely directed currents were observed within both regions. We show that the majority of these current sheets were closely aligned to a north-south direction, in contrast to the expected east-west orientation of the preonset aurora. Comparing our results with observations of the field-aligned current associated with bursty bulk flows (BBFs), we conclude that significant questions remain for the explanation of SCW structuring by BBF-driven wedgelets. Our results therefore represent constraints on future modeling and theoretical frameworks on the generation of theSCW. Key Points The substorm current wedge (SCW) has significant azimuthal structure Current sheets within the SCW are north-south aligned The substructure of the SCW raises questions for the proposed wedgelet scenari