Time-averaged Field Research Articles

Inclination flattening and the geocentric axial dipole hypothesis

William Gilbert first articulated what has come to be known as the geocentric axial dipole hypothesis. The GAD hypothesis is the principle on which paleogeographic reconstructions rely to constrain paleolatitude. For decades, there have been calls for permanent non-dipole contributions to the time-averaged field. Recently, these have demanded large contributions of the axial octupole, which, if valid, would call into question the general utility of the GAD hypothesis. In the process of geological recording of the geomagnetic field, “Earth filters” distort the directions. Many processes, for example, sedimentary inclination flattening and random tilting, can lead to a net shallowing of the observed direction. Therefore, inclinations that are shallower than expected from GAD can be explained by recording biases, northward transport, or non-dipole geomagnetic fields. Using paleomagnetic data from the last 5 million years from well-constrained lava flow data allows the construction of a statistical geomagnetic field model. Such a model can predict not only the average expected direction for a given latitude, but also the shape of the distribution of directions produced by secular variation. The elongation of predicted directions varies as a function of latitude (from significantly elongate in the up/down direction at the equator to circularly symmetric at the poles). Sedimentary inclination flattening also works in a predictable manner producing elongations that are stretched side to side and the degree of flattening depending on the inclination of the applied field and a “flattening factor” f. The twin tools of the predicted elongation/inclination relationship characteristic of the geomagnetic field for the past 5 million years and the distortion of the directions predicted from sedimentary inclination flattening allows us to find the flattening factor that yields corrected directions with an elongation and average inclination consistent with the statistical field model. The method can be tested using sediments deposited in a known field. Application of the elongation/inclination correction method to two magnetostratigraphic data sets from red beds in Asia and Pakistan brings the inclinations into agreement with those predicted from modern GPS measurements and from global paleomagnetic data. There appears to be no compelling reason at this time to abandon the geocentric dipole hypothesis, which has provided such an excellent working model for so long.

Large-eddy simulation of turbulent flow in an unbaffled stirred tank driven by a Rushton turbine

The turbulent flow field generated in an unbaffled stirred tank by a Rushton turbine was computed by large-eddy simulation (LES). The Smagorinsky model was used to model the unresolved, or sub-grid, scales. A general purpose CFD code was appropriately modified in order to allow the computation of the sub-grid viscosity and to perform statistics on the computed results. The numerical predictions were compared with the literature results for comparable configurations and with experimental data obtained using particle image velocimetry. A very good agreement was found as regards both time-averaged resolved fields and turbulence quantities.

地球磁場の形と変動―平均地球磁場と古地磁気永年変化―

Paleomagnetism has been applied to tectonics studies on the basis of the geocentric axial dipole (GAD) field hypothesis. However, the applicability of the GAD hypothesis is still under investigation in the paleomagnetic community. It is directly connected to the precision of the tectonic movements derived from paleomagnetism, so that the the morphology of the geomagnetic field should draw wide attention among Earth scientists. The morphology of the long term geomagnetic features is often represented by the time-averaged field (TAF) and the paleosecular variation (PSV). They are extracted from the paleodirections of lavas erupted during the past 5 My.The recent TAF and PSV models indicate following; (1) the GAD hypothesis is not strictly accurate, (2) the geocentric axial quadupole (g02) field exists in the TAF and it cannot be neglected, and (3) the inclination anomaly calculated from the averaged paleomagnetic data consists also of the apparent effect of the PSV, which additionally cannot be ignored. These components should be paid close attentions to specially in the case of detailed tectonics such as highresolution plate motion. The inclination anomaly due to g02 in the TAF and the effect of the PSV would produce a mistake of the paleolatitude, which becomes totally up to several degrees.

Influence of Hydrogen Addition on Flow Structure in Confined Swirling Methane Flame

The flowfield of a lean premixed swirl-stabilized burner simulating typical features of land-based gas-turbine combustors was investigated using particle-image velocimetry. Fuel and air were premixed upstream and burned at atmospheric pressure in a quartz-tube combustor operated at a theoretical swirl number of 1.5. Instantaneous-velocity-field measurements were obtained for a nonreacting flow, a methane flame, and a hydrogen-enriched methane flame. Flow measurements were used to obtain two-dimensional vorticity and normal-strain, turbulent-kinetic-energy, and kinetic-energy-dissipation-rate fields. Results show that the average- and instantaneous-velocity fields were affected by the addition of hydrogen to methane. The instantaneous-velocity fields showed smaller eddies that were not present in the time-averaged fields. Higher values of turbulent kinetic energy were observed in the jet region of the methane flame, suggesting the unsteady nature of combustion. The instantaneous vorticity and normal strain were four to seven times higher than the averaged values, indicating the importance of smaller vortical structures to local flame-extinction phenomena.

Experimental Investigation Of The Velocity Field In Buoyant Diffusion Flames Using PIV And TPIV Algorithm

We investigated a simultaneous temporally and spatially resolved 2-D velocity field above a burning circular pan of alcohol using particle image velocimetry (PIV). The results obtained from PIV were used to assess a thermal particle image velocimetry (TPIV) algorithm previously developed to approximate the velocity field using the temperature field, simultaneously captured by an infrared (IR) thermal camera. By tracing “thermal particles,” which were assumed to be virtual particles that corresponded to pixels of temperature values in successive IR images, the TPIV algorithm estimated a larger scale instantaneous velocity field than either a single-point velocity measurement (e.g., LDV) or the area velocity measurement such as PIV. Instantaneous velocity fields obtained from both methods are presented. Time series vertical velocity profiles and time-averaged velocity vector fields are compared. The comparison demonstrates the applicability and performance of the TPIV algorithm in wildfire research.

Bone Cell Survival in Microgravity: Evidence that Modeled Microgravity Increases Osteoblast Sensitivity to Apoptogens

Studies were performed to evaluate the effects of modeled microgravity on the induction of osteoblast apoptosis. MC3T3-E1 osteoblast-like cells were cultured in alginate carriers in the NASA-approved high aspect ratio vessel (HARV). This system subjects the cells to a time-averaged gravitational field (vector-averaged gravity) to simulate low gravity conditions. Cells were cultured in the HARV for five days, and then examined for apoptosis. In simulated microgravity, the cells remained vital, although analysis of expressed genes indicated that there was loss of the mature osteoblast phenotype. Additionally, we noted that there was a loss of the mitochondrial membrane potential, a low level of the antiapoptotic protein Bcl-2, as well as Akt protein, and the redox status of the cells was disturbed. All of these parameters indicated that vector-averaged gravity disrupts mitochondrial function, thereby sensitizing osteoblasts to apoptosis. We then used a challenge assay to evaluate the apoptotic sensitivity of the cells subjected to vector-averaged gravity. When challenged with staurosporine, cells subjected to vector-averaged gravity evidenced elevated levels of cell death relative to control cell populations. Another objective of the study was to improve upon conventional carriers by using alginate encapsulation to support cells in the HARV. We have demonstrated that the alginate carrier system affords a more robust system than surface-seeded carriers. This new system has the advantage of shielding cells from mechanical damage and fluid shear stresses on cells in the HARV, permitting carefully controlled studies of the effects of vector-averaged gravity.

Long-term evolution of the geomagnetic dipole moment

The geomagnetic field intensity measured at the surface of the planet is a potential indicator of the dynamo activity in the conducting liquid core of the Earth. Rapid field variations must be generated by the rapid fluid motions within the core, whereas long-term changes could be associated with other processes such as changes in boundary conditions at the core–mantle interface and/or at the outer (liquid)–inner (solid) core boundary. For about 50 years, paleomagnetists gathered records of absolute paleointensity using the magnetization of lava flows distributed over the globe in order to reconstruct the field intensity changes during the past 3000 Ma. Despite recent acquisition of paleointensity records, the temporal distribution of the results remains limited (except within a few time intervals) to extract coherent features of the time-averaged field intensity over periods of a few million years. However, significant informations can be gained from the recent updated paleointensity database by averaging the virtual dipole moment over very long time intervals. The results suggest the existence of a long-term evolution of the dipole field intensity during the past 3 billion years (from 3 × 10 22 A m 2 at 1000–2000 Ma to 8 × 10 22 A m 2 at present times).

Characterization of the plasma in a radio-frequency magnetron sputtering system

In order to understand the fundamental mechanisms in a radio-frequency magnetron sputtering system, the main properties of the argon plasma used in the process have been measured. A complete three-dimensional map of the ion density, electron temperature, and plasma potential has been obtained using a Langmuir probe. The electron temperature as well as the ion density have been found to increase in the region of the so called race track at the cathode. Furthermore, from the plasma potential map, the time-averaged local electric field has been obtained, pointing out the race track as the region where the most intense ion bombardment takes place. Besides, only the ions produced near the race track are accelerated towards the cathode, whereas those produced in the remaining volume move towards the anode. Finally, the dependence of the plasma quantities on the incident radio-frequency power and deposition pressure has been studied. The plasma potential measured using the Langmuir probe has been found to agree with that determined using an energy resolved mass spectrometer in all studied conditions.

Global Soil Moisture from Satellite Observations, Land Surface Models, and Ground Data: Implications for Data Assimilation

Abstract Three independent surface soil moisture datasets for the period 1979–87 are compared: 1) global retrievals from the Scanning Multichannel Microwave Radiometer (SMMR), 2) global soil moisture derived from observed meteorological forcing using the NASA Catchment Land Surface Model, and 3) ground-based measurements in Eurasia and North America from the Global Soil Moisture Data Bank. Time-average soil moisture fields from the satellite and the model largely agree in the global patterns of wet and dry regions. Moreover, the time series and anomaly time series of monthly mean satellite and model soil moisture are well correlated in the transition regions between wet and dry climates where land initialization may be important for seasonal climate prediction. However, the magnitudes of time-average soil moisture and soil moisture variability are markedly different between the datasets in many locations. Absolute soil moisture values from the satellite and the model are very different, and neither agrees...

Serial magnetization transfer imaging in acute optic neuritis

MAGNETIZATION TRANSFER IMAGING (MT) ALLOWS the examination of tissues in more details than conventional MRI. In serial studies of multiple sclerosis lesions, reductions in magnetization transfer ratio (MTR) are thought to be due to demyelination and axonal loss, with later rises due to remyelination. In this study, the authors followed serial changes in MTR in acute optic neuritis in combination with clinical and electrophysiological measurements to determine if the MTR changes over time mirror the picture in multiple sclerosis lesions. They included 29 patients who had acute optic neuritis for a median of 13 days (range 7–24 days) since the onset of visual symptoms. A clinical examination and measurement of visual evoked potentials (VEP) was performed on each patient. Their optic nerves were imaged with a fat-saturated fast spin echo (FSE) sequence and a magnetization transfer sequence. Twenty-one had multiple subsequent examinations over the course of 1 year. In addition, 27 control subjects had their optic nerves imaged up to three times over 1 year. A blinded observer segmented the optic nerves from the MTR maps. Lesions were defined on the acute FSE images and, from the coordinates, the ratio of mean lesion MTR : healthy nerve MTR (lesion ratio) was calculated for each dataset. The time-averaged mean MTR in control optic nerves was 47.7 per cent units (pu). In diseased optic nerves, baseline mean MTR was 47.3 pu, with a mean lesion ratio of 0.98. The diseased optic nerve MTR and lesion ratio declined over time with a nadir at about 240 days at a mean MTR value of 44.2 pu and mean lesion ratio of 0.91. After 1 year the diseased optic nerve mean MTR was 45.1 pu (mean lesion ratio 0.93), although the difference was not significant compared with the nadir value. For each 0.01 increase in time-averaged lesion ratio logMAR visual acuity recovery improved by 0.03 (95% CI, 0.002, 0.08, P = 0.02). Time-averaged VEP central field latency was shorter by 6.1 ms (95% CI 1.5, 10.7, P = 0.012) per 1 pu rise in time-averaged diseased optic nerve MTR. The authors conclude that early fall in diseased optic nerve MTR is consistent with demyelination and Wallerian degeneration of transected axons. The late nadir compared with studies of multiple sclerosis lesions may have been due to slow clearance of myelin debris. Remyelination may have influenced subsequent MTR changes. The observations support using MTR to monitor symptomatic demyelinating lesions.—Valérie Biousse

Contrast of time-averaged images of the solar granulation

The time-averaged images of the solar granulation exhibit a slower decrease in contrast with the averaging time than do time-averaged images of numerically simulated granulation and time-averaged random fields with some parameters typical of granulation. This confirms the hints for long-lived structures in the granulation pattern.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Systematic characterization of low-pressure capacitively coupled hydrogen discharges

This paper presents a systematic characterization of pure hydrogen capacitively coupled discharges, produced in a parallel plate cylindrical setup. A two-dimensional, time-dependent fluid model is used to describe the production, transport, and destruction of electrons and positive ions H+, H2+, and H3+, at different frequencies (13.56–60 MHz), pressures (0.2–8 Torr), rf applied voltages (50–450 V) and geometric dimensions (1.6–12.8 cm radii and 1.6–6.4 cm interelectrode distances). A good agreement is found between calculation results and experimental measurements for the coupled electrical power, the plasma potential, and the self-bias potential, at various frequencies and rf applied voltages. However, the model generally underestimates the electron density with respect to its measured values. The paper discusses different space-time events, such as the development of double-ionization structures or the occurrence of field inversion and field reversal phenomena. The dependencies on pressure and frequency of the time-average electric field distribution are analyzed and related to the electron displacement within space-charge sheaths. This study is later used to understand the variations of the hydrogen dissociation rate, with changes in discharge operating conditions. The influence of reactor dimensions on the spatial profiles of the plasma potential, the rf electric field, the electron density, and the electron mean energy are analyzed in terms of discharge symmetry. An investigation of the space-time averaged rf electric field variations, with changes in the applied voltage, pressure, and geometric dimensions is carried out. These variations are shown to follow a universal similarity curve, if an adequate normalization is used when plotting the rf electric field as a function of pressure. This innovative representation of rf discharges allows a univocal definition of a reactor working point, for given operating conditions.

Putting models to the data test: a case study using Indian Ocean CFC-11 data

A method is presented for comparing time-averaged model output with snapshot data. The focus is on a comparison between the cholorofluorocarbon CFC-11 simulated in the Parallel Ocean Program (POP) model, and the near-synoptic Indian Ocean World Ocean Circulation Experiment (WOCE) CFC data-set collected in 1995. In the thermocline, the simulated fields fairly closely approximate the observations. We seek to distinguish between regions in which there is room for improvement in the model physics, and regions where the mismatch is the result of comparing time-averaged model fields with snapshot data. CFC variance is estimated using an eddy-permitting Miami Isopycnic Coordinate Ocean Model (MICOM) simulation. The results indicate that the widespread method of visual comparison of vertically-gridded data with model output might lead to misattribution of model deficiencies in regions of high oceanic variability. It is suggested that consideration of error-bars obtained from eddy-permitting model simulations in future model-data comparisons could help avoid such potentially erroneous conclusions.

A flow field study of an elliptic jet in cross flow using DPIV technique

The digital particle image velocimetry (DPIV) technique has been used to investigate the flow fields of an elliptic jet in cross flow (EJICF). Two different jet orientations are considered; one with the major axis of the ellipse aligned with the cross flow (henceforth referred to as a low aspect ratio (AR) jet), and the other with the major axis normal to the cross flow (henceforth referred to as a high aspect ratio jet). Results show that the vortex-pairing phenomenon is prevalent in the low aspect ratio jet when the velocity ratio (VR)≥3, and is absent in the high aspect ratio jet regardless of the velocity ratio. The presence of vortex pairing leads to a substantial increase in the leading-edge peak vorticity compared to the lee-side vorticity, which suggests that vortex pairing may play an important role in the entrainment of ambient fluid into the jet body, at least in the near-field region. In the absence of vortex pairing, both the leading-edge and the lee-side peak vorticity increase monotonically with velocity ratio regardless of the aspect ratio. Moreover, time-averaged velocity fields for both AR=0.5 and AR=2 jets reveal the existence of an “unstable focus” (UF) downstream of the jet, at least for VR≥2. The strength and the location of this focus is a function of both the velocity ratio and aspect ratio. In addition, time-averaged vorticity fields show a consistently higher peak-averaged vorticity in the low aspect ratio jet than in the high aspect ratio jet. This behavior could be due to a higher curvature of the vortex filament facing the cross flow in the low aspect ratio jet, which through mutual interaction may lead to higher vortex stretching, and therefore higher peak-averaged vorticity.

Plio‐Pleistocene time‐averaged field in southern Patagonia recorded in lava flows

Paleomagnetic directions were obtained from stepwise alternating‐field or thermal demagnetization of 53 lava flows from southern Patagonia (latitudes 49.5°–52.1°S) that include the Pali‐Aike volcanic field and the Meseta Viscachas plateau lavas. In addition to previous Miocene‐late Quaternary ages of these flows, 40Ar/39Ar dates spanning from 0.1 to 15.4 Ma were obtained for 17 of the sites. All except one of the magnetic polarities coincide with the expected polarities of the magnetic polarity timescale [Cande and Kent, 1995] for the obtained 40Ar/39Ar ages. The mean direction from 33 sites (eliminating sites ≥4 Ma) that pass a selection criteria of α95 ≤ 5° is Dec = 358.7°, Inc = −68.2°, α95 = 3.5°, a value that coincides within the statistical uncertainty with the direction of the geocentric axial dipole for that area (Inc = −68.1°). Likewise, the mean virtual geomagnetic pole (VGP) coincides within the statistical uncertainty with the geographic North Pole. The secular variation described by the VGP angular standard deviation for these sites is 17.1°, a value expected for that latitude according to Model G of paleosecular variation [McFadden et al., 1988]. The characteristics of the data presented are optimum for time‐averaged field (TAF) studies because of the good age control and good quality of the paleomagnetic data: (1) primary components of magnetization were obtained using principal component analysis [Kirschvink, 1980] from at least five points and maximum angular deviation ≤5°, (2) site means were calculated with Fisher statistics using at least three samples, and (c) 38 of the 53 flows had α95 ≤ 5°. No results (five sites) or high α95 values (>5°) were obtained primarily from sites affected by lightning.

Applying the Uncertainty Principle to Single Particle Interactions.

Existing derivations of uncertainty for single-particle interactions violate complementarity because they require that the photon exhibit wave and particle behavior simultaneously, and thus singularly. In order to restore physical consistency to quantum theory, a model of the photon is proposed with spatial extension equal to the wavelength. As a result, uncertainty and indeterminacy must be assigned independent meanings. Uncertainty describes the limit in measurability for instantaneous exchanges of momentum and is due to a photon’s particle properties. It is causal in origin and provides a model for the kinematics of quantum theory. Indeterminacy, however, is statistical in nature and is attributed to the exchange of momentum by time-averaged fields. The need for two limitations on measurability is seen as an extension of the duality principle to measurement theory.

Transitional field clusters from uppermost Oligocene volcanic rocks in the central Walker Lane, western Nevada

Three sections of the Candelaria Hills volcanic sequence, west-central Nevada, appear to have recorded parts of two transitional field records or reversal excursions. Paleomagnetic data and 40 Ar / 39 Ar laser fusion sanidine age estimates for pyroclastic rocks and associated flows show that these rocks recorded the unusual field behavior at about 25.7 Ma and about 23.8 Ma. Fifteen sites yield northeast declination, moderate to shallow negative inclination mean directions and 16 sites yield west to southwest declination, moderate negative inclination directions. Both populations of site mean directions, representing a total of 12 independent eruptive units, are highly discordant to a time-averaged late Tertiary field direction, and neither can be explained by a geologically reasonable magnitude of vertical axis rotation. Virtual paleomagnetic poles (VGPs), estimated from the directional data, lie at low to intermediate latitudes; 29 of the 31 flows at intermediate latitudes (<60°), and 11 at very low latitudes (<30°). Two well-grouped VGP clusters are defined by these data with each cluster roughly corresponding to one of the age groups. Stratigraphically corrected VGPs from most of the 23.8 Ma group roughly cluster at intermediate to low latitudes at about 150°E longitude. The cluster at about 150°E corresponds to VGP clusters that have been interpreted to reflect a long lasting near-dipole configuration during several field reversals. The second stratigraphically corrected cluster lies at intermediate to low latitudes at about 80°E longitude and, notably, is defined by pyroclastic flows of the 25.7 and 23.8 Ma age groups. The VGP data at about 80°E do not fall into any previously identified preferred longitudinal band, however, they are consistent with data from some sedimentary records of reversal excursions in western North America. We recognize that the VGPs returned to a preferred location in both age populations, which we interpret as a preferred directional position, thus reflecting a potentially stable non-dipole component during a complete reversal or a reversal excursion. The observation that the VGPs maintained a preferred location during separate high amplitude events supports the hypothesis that preferred VPG clusters and thus persistent non-dipole field components can factor into the behavior of the geomagnetic field during full reversals or reversal excursions.

Serial magnetization transfer imaging in acute optic neuritis.

In serial studies of multiple sclerosis lesions, reductions in magnetization transfer ratio (MTR) are thought to be due to demyelination and axonal loss, with later rises due to remyelination. This study followed serial changes in MTR in acute optic neuritis in combination with clinical and electrophysiological measurements to determine if the MTR changes over time mirror the picture in multiple sclerosis lesions, further validating MTR as a marker of tissue integrity. Twenty-nine patients were recruited who had acute optic neuritis for a median of 13 days (range 7-24 days) since the onset of visual symptoms. A clinical examination and measurement of visual evoked potentials (VEP) was performed on each patient. Their optic nerves were imaged with a fat-saturated fast spin echo (FSE) sequence and a magnetization transfer sequence. Twenty-one had multiple subsequent examinations over the course of 1 year. In addition, 27 control subjects had their optic nerves imaged up to three times over 1 year. A blinded observer segmented the optic nerves from the MTR maps. Lesions were defined on the acute FSE images and, from the coordinates, the ratio of mean lesion MTR : healthy nerve MTR (lesion ratio) was calculated for each dataset. The time-averaged mean MTR in control optic nerves was 47.7 per cent units (pu). In diseased optic nerves, baseline mean MTR was 47.3 pu, with a mean lesion ratio of 0.98. The diseased optic nerve MTR and lesion ratio declined over time with a nadir at about 240 days at a mean MTR value of 44.2 pu and mean lesion ratio of 0.91. Subsequently, diseased optic nerve MTR appeared to rise; after 1 year the diseased optic nerve mean MTR was 45.1 pu (mean lesion ratio 0.93), although the difference was not significant compared with the nadir value. For each 0.01 increase in time-averaged lesion ratio logMAR visual acuity recovery improved by 0.03 (95% CI, 0.002, 0.08, P = 0.02). Time-averaged VEP central field latency was shorter by 6.1 ms (95% CI 1.5, 10.7, P = 0.012) per 1 pu rise in time-averaged diseased optic nerve MTR. The early fall in diseased optic nerve MTR is consistent with demyelination and Wallerian degeneration of transected axons. The late nadir compared with studies of multiple sclerosis lesions may have been due to slow clearance of myelin debris. Remyelination may have influenced subsequent MTR changes. The observations support using MTR to monitor symptomatic demyelinating lesions.

Excitation of ion-wave wakefield by the resonant absorption of a short pulsed microwave with plasma.

Unmagnetized, inhomogeneous laboratory plasma irradiated by a high power (eta=E(2)(0)/4pin(e)kT(e) approximately 5.0x10(-2)) short pulsed microwave with pulse length of the order of ion-plasma period (tau(pi) less, similar 2pi/omega(pi)) is studied. Large density perturbation traveling through the underdense plasma with a velocity much greater than the ion sound speed produced by the resonant absorption of the microwave pulse has been observed. In the beginning the density perturbation has large amplitude (deltan/n(0) approximately 40%) and propagates with a velocity of the order of 10(6) cm/s. But later its amplitude as well as the velocity decrease rapidly, and finally the velocity arrives with twice the ion sound speed. The oscillating incident electromagnetic waves enhance highly localized electric field by the resonant absorption process and develop time-averaged force field which pushes plasma electrons from the resonant layer. As the electrons are accelerated to be ejected, they pull plasma ions as a bunch with them by means of self-consistent Coulomb force. This suprathermal ion bunch can excite an ion-wave wakefield.

Early Permian Pangea ‘B’ to Late Permian Pangea ‘A’

The pre-drift Wegenerian model of Pangea is almost universally accepted, but debate exists on its pre-Jurassic configuration since Ted Irving introduced Pangea ‘B’ by placing Gondwana farther to the east by ∼3000 km with respect to Laurasia on the basis of paleomagnetic data. New paleomagnetic data from radiometrically dated Early Permian volcanic rocks from parts of Adria that are tectonically coherent with Africa (Gondwana), integrated with published coeval data from Gondwana and Laurasia, again only from igneous rocks, fully support a Pangea ‘B’ configuration in the Early Permian. The use of paleomagnetic data strictly from igneous rocks excludes artifacts from sedimentary inclination error as a contributing explanation for Pangea ‘B’. The ultimate option to reject Pangea ‘B’ is to abandon the geocentric axial dipole hypothesis by introducing a significant non-dipole (zonal octupole) component in the Late Paleozoic time-averaged geomagnetic field. We demonstrate, however, by using a dataset consisting entirely of paleomagnetic directions with low inclinations from sampling sites confined to one hemisphere from Gondwana as well as Laurasia that the effects of a zonal octupole field contribution would not explain away the paleomagnetic evidence for Pangea ‘B’ in the Early Permian. We therefore regard the paleomagnetic evidence for an Early Permian Pangea ‘B’ as robust. The transformation from Pangea ‘B’ to Pangea ‘A’ took place during the Permian because Late Permian paleomagnetic data allow a Pangea ‘A’ configuration. We therefore review geological evidence from the literature in support of an intra-Pangea dextral megashear system. The transformation occurred after the cooling of the Variscan mega-suture and lasted ∼20 Myr. In this interval, the Neotethys Ocean opened between India/Arabia and the Cimmerian microcontinents in the east, while widespread lithospheric wrenching and magmatism took place in the west around the Adriatic promontory. The general distribution of plate boundaries and resulting driving forces are qualitatively consistent with a right-lateral shear couple between Gondwana and Laurasia during the Permian. Transcurrent plate boundaries associated with the Pangea transformation reactivated Variscan shear zones and were subsequently exploited by the opening of western Neotethyan seaways in the Jurassic.