Speak to Tailor Echo , 2. Report to Tailor Nika , -Wait 45 seconds 3. Speak to Tailor Nika , 4. Speak to Nightfire Messenger , 2. Speak to Apothecary Trone , -Wait 40 seconds 3. Speak to Apothecary Trone , 4.
Speak to Apothecary Trone , — 15 Minute time limit. Kill as many as you can. Speak to Short-Tail Lochmur , 2. Speak to Lochmur. Drake , Reward Coin: 3. Drake , — Collect Three Chest of Treasures , 2. Speak to Guard Bulbeyes , 2. Speak to Blacksmith Dmitrii , 3. Speak to Liasion Officer Kwong , 4. Speak to Shipping Office Chiang , 5. New quest goal: -Kill 15 Neon Worms 3.
Keep it for a later quest 3. Continue on to quest: Treason Level 14 Sad Message 1. Continue on to quest: Island and City Missing Captain 1. Speak to Merchants Ambassador Shimmin , 2. Speak to Escort Captain Tankis , 4. Speak to Teleporter Reviero , 3. Speak to the Elder , Warrior Recommendation 1. Rep:3 Level 16 Never Return 1. Speak to the Elder , -Automatically Teleport to Cloud Temple Other ways to get there, glowing circle in the building behind the elder, via the quest option at the teleporter.
Collect 1 Leadership Proof Farmable from body at , -Quest Treason will auto-trigger when you reach the body. Spirit: , Rep:2 Treason 1. Speak to Murmuring Person , 2. Following the local appearance of a spur of stratospheric volcanic debris from the subtropics, a series of jet streaks subsequently conditioned the troposphere through tropopause foldings with sulfur based particles that became effective cloud forming nuclei in cirrus clouds.
Aerosol and ozone measurements suggest a complicated history of stratospheric- tropospheric exchanges embedded with the upper level flow, and cirrus cloud formation was noted to occur locally at the boundaries of stratospheric aerosol enriched layers that became humidified through diffusion, precipitation, or advective processes.
Apparent cirrus cloud alterations include abnormally high ice crystal concentrations up to approximately L exp. Implications for volcanic-cirrus cloud climate effects and unusual nonvolcanic aerosol jet stream cirrus cloud formation are discussed. The evolution of synoptic-scale dynamics associated with a middle and upper tropospheric cloud event that occurred on 26 November is examined.
Using data from the wind profiler demonstration network and a temporally and spatially augmented radiosonde array, emphasis is given to explaining the evolution of the kinematically-derived ageostrophic vertical circulations and correlating the circulation with the forcing of an extensively sampled cloud field.
This is facilitated by decomposing the horizontal divergence into its component parts through a natural coordinate representation of the flow. Ageostrophic vertical circulations are inferred and compared to the circulation forcing arising from geostrophic confluence and shearing deformation derived from the Sawyer-Eliassen Equation. It is found that a thermodynamically indirect vertical circulation existed in association with a jet streak exit region. The circulation was displaced to the cyclonic side of the jet axis due to the orientation of the jet exit between a deepening diffluent trough and building ridge.
The cloud line formed in the ascending branch of the vertical circulation with the most concentrated cloud development occurring in conjunction with the maximum large-scale vertical motion. The relationship between the large scale dynamics and the parameterization of middle and upper tropospheric clouds in large-scale models is discussed and an example of ice water contents derived from a parameterization forced by the diagnosed vertical motions and observed water vapor contents is presented.
Tracking the global jet streams through objective analysis. Although the tropospheric jet streams are probably the more important single dynamical systems in the troposphere , their study at climatic scale has been usually troubled by the difficulty of characterising their structure.
During the last years, a deal of effort has been made in order to construct long-term scale objective climatologies of the jet stream or at least to understand the variability of the westerly flux in the upper troposphere. A main problem with studying the jets is the necessity of using highly derivated fields as the potential vorticity or even the analysis of chemical tracers. Despite their utility, these approaches are very problematic to construct an automatic searching algorithm because of the difficulty of defining criteria for these extremely noisy fields.
Some attempts have been addressed trying to use only the wind field to find the jet. This direct approach avoids the use of derivate variables, but it must contain some stringent criteria to filter the large number of tropospheric wind maxima not related to the jet currents. This approach has offered interesting results for the relatively simple structure of the Southern Hemisphere tropospheric jets Gallego et al. Dyn, However, the much more complicated structure of its northern counterpart has resisted the analysis with the same degree of detail by using the wind alone.
In this work we present a new methodology able to characterise the position, strength and altitude of the jet stream at global scale on a daily basis. The method is based on the analysis of the 3-D wind field alone and it searches, at each longitude, relative wind maxima in the upper troposphere between the levels of and hPa. An ad-hoc defined density function dependent on the season and the longitude of the detection positions is used as criteria to filter spurious wind maxima not related to the jet.
An automated cloud tracking algorithm is applied to Cassini Imaging Science Subsystem high-resolution apoapsis images of Saturn from and and moderate resolution images from and to define the near-global distribution of zonal winds and eddy momentum fluxes at the middle troposphere cloud level and in the upper troposphere haze. Improvements in the tracking algorithm combined with the greater feature contrast in the northern hemisphere during the approach to spring equinox allow for better rejection of erroneous wind vectors, a more objective assessment at any latitude of the quality of the mean zonal wind, and a population of winds comparable in size to that available for the much higher contrast atmosphere of Jupiter.
Zonal winds at cloud level changed little between and at all latitudes sampled. Upper troposphere zonal winds derived from methane band images are approx.
In westward jet regions winds are approximately the same at both altitudes. Lateral eddy momentum fluxes are directed into eastward jet cores, including the strong equatorial jet , and away from westward jet cores and weaken with increasing altitude on the flanks of the eastward jets , consistent with the upward broadening of these jets.
The conversion rate of eddy to mean zonal kinetic energy at the visible cloud level is larger in eastward jet regions 5. Microchannel plate streak camera. An improved streak camera in which a microchannel plate electron multiplier is used in place of or in combination with the photocathode used in prior streak cameras. The improved streak camera is far more sensitive to photons UV to gamma-rays than the conventional x-ray streak camera which uses a photocathode.
The improved streak camera offers gamma-ray detection with high temporal resolution. It also offers low-energy x-ray detection without attenuation inside the cathode. Using the microchannel plate in the improved camera has resulted in a time resolution of about ps, and has provided a sensitivity sufficient for KeV x-rays. Frosty Wind Streaks. MOC, 2 November As seasonal polar frosts sublime away each spring, winds may re-distribute some of the frost or move sediment exposed from beneath the frost.
This action creates ephemeral wind streaks that can be used by scientists seeking to study the local circulation of the martian [missing text] surveyor MGS Mars Orbiter Camera MOC image shows a suite of wind streaks created in subliming carbon dioxide frost. These dark streaks appear to conform to the shape of the slopes on which they occur, suggesting that slope winds play a dominant role in creating and orienting these streaks.
This picture is located near The image is illuminated by sunlight from the upper left and covers an area 3 km 1. Dark Slope Streak. Dark slope streaks , like the ones in this unnamed crater in Terra Sabaea, are believed to be formed when surface dust is displaced and the darker rock below is exposed.
Rocks falling due to gravity likely formed these streaks. Streak camera receiver definition study. Detailed streak camera definition studies were made as a first step toward full flight qualification of a dual channel picosecond resolution streak camera receiver for the Geoscience Laser Altimeter and Ranging System GLRS. The streak camera receiver requirements are discussed as they pertain specifically to the GLRS system, and estimates of the characteristics of the streak camera are given, based upon existing and near-term technological capabilities.
Important problem areas are highlighted, and possible corresponding solutions are discussed. A case study is conducted implementing the Dell Streak seven-inch android device into eighth grade science classes of one teacher in a rural middle school in the Piedmont region of North Carolina. The purpose of the study is to determine if the use of the Dell Streaks would increase student achievement on standardized subject testing, if the….
Streaking into middle school science: The Dell Streak pilot project. The purpose of the study is to determine if the use of the Dell Streaks would increase student achievement on standardized subject testing, if the Streak could be used as an effective instructional tool, and if it could be considered an effective instructional resource for reviewing and preparing for the science assessments.
A mixed method research design was used for the study to analyze both quantitative and qualitative results to determine if the Dell Streaks ' utilization could achieve the following: 1. A Post Hoc analysis was conducted to identify where the difference occurred.
Finally a T-test determined was there was no statistically significance difference between the mean End-of-Grade tests and four quarterly benchmark scores of the control and the experimental groups. Qualitative research methods were used to gather results to determine if the Streaks were an effective instructional tool.
Classroom observations identified that the teacher's teaching styles and new instructional strategies were implemented throughout the pilot project.
Students had an opportunity to complete a questionnaire three times during the pilot project. Results revealed what the students liked about using the devices and the challenges they were facing. The teacher completed a reflective questionnaire throughout the pilot project and offered valuable reflections about the use of the devices in an educational setting.
The reflection data supporting the case study was drawn. Slope Streaks or RSL? The image shows a region we see many slope streaks , typically dark features on slopes in the equatorial regions on Mars. They may extend for tens of meters in length and gradually fade away with time as new ones form.
The most common hypothesis is that they are generated by dust avalanches that regularly occur on steep slopes exposing fresh dark materials from underneath the brighter dust.
There are many types of slope streaks but one of the most recent and significant findings using HiRISE was the discovery of a new type called "recurring slope lineae," or RSL for short. Recent studies suggest that RSL may form through the flow of briny extremely salty liquid water that can be stable on the surface of Mars even under current climatic conditions for a limited time in summer when it is relatively warm.
How can we distinguish between conventional slope streaks like the ones we see here and RSL? There are many criteria. For instance, RSL are usually smaller in size than regular slope streaks.
However, one of the most important conditions is seasonal behavior, since RSL appear to be active only in summer while regular slope streaks can be active anytime of the year. This site is monitored regularly by HiRISE scientists because of the high density of slope streaks and their different sizes and orientations. If we look at a time-lapse sequence, we will see that a new slope streak has indeed formed in the period since April and we can note how dark it is in comparison to the others indicating its freshness.
However, this period corresponds mainly to the autumn season in this part of Mars, whereas we do not see any major changes in the summer season. This suggests that the feature that developed is a regular slope streak just like all the others in the area.
Vertical structure of tropospheric winds on gas giants. Zonal mean zonal velocity profiles from cloud-tracking observations on Jupiter and Saturn are used to infer latitudinal variations of potential temperature consistent with a shear stable potential vorticity distribution.
Immediately below the cloud tops, density stratification is weaker on the poleward and stronger on the equatorward flanks of midlatitude jets , while at greater depth the opposite relation holds. Thermal wind balance then yields the associated vertical shears of midlatitude jets in an altitude range bounded above by the cloud tops and bounded below by the level where the latitudinal gradient of static stability changes sign. The inferred vertical shear below the cloud tops is consistent with existing thermal profiling of the upper troposphere.
The sense of the associated mean meridional circulation in the upper troposphere is discussed, and expected magnitudes are given based on existing estimates of the radiative timescale on each planet. Triton's streaks as windblown dust. Explanations for the surface streaks observed by Voyager 2 on Triton's southern hemisphere are discussed. For geyser-like erupting dust plumes, it is shown that dust-settling time scales and expected wind velocities can produce streaks with length scales in good agreement with those of the streaks.
Thus, both geyserlike eruptions or direct lifting by surface winds appear to be viable mechanisms for the origin of the streaks. Wind Streaks on Earth; Exploration and Interpretation. Wind streaks , one of the most common aeolian features on planetary surfaces, are observable on the surface of the planets Earth, Mars and Venus.
Due to their reflectance properties, wind streaks are distinguishable from their surroundings, and they have thus been widely studied by remote sensing since the early s, particularly on Mars. In imagery, these streaks are interpreted as the presence - or lack thereof - of small loose particles on the surface deposited or eroded by wind. The existence of wind streaks serves as evidence for past or present active aeolian processes.
Therefore, wind streaks are thought to represent integrative climate processes. As opposed to the comprehensive and global studies of wind streaks on Mars and Venus, wind streaks on Earth are understudied and poorly investigated, both geomorphologically and by remote sensing. The aim of this study is, thus, to fill the knowledge gap about the wind streaks on Earth by: generating a global map of Earth wind streaks from modern high-resolution remotely sensed imagery; incorporating the streaks in a geographic information system GIS ; and overlaying the GIS layers with boundary layer wind data from general circulation models GCMs and data from the ECMWF Reanalysis Interim project.
The study defines wind streaks and thereby distinguishes them from other aeolian features based not only on their appearance in imagery but more importantly on their surface appearance.
This effort is complemented by a focused field investigation to study wind streaks on the ground and from a variety of remotely sensed images both optical and radar.
In this way, we provide a better definition of the physical and geomorphic characteristics of wind streaks and acquire a deeper knowledge of terrestrial wind streaks as a means to better understand global and planetary climate and climate change. In a preliminary study, we detected and mapped over 2, wind streaks in the desert regions of Earth distributed in. Identifying its performance in model prediction may provide us another viewpoint, from the perspective of upper- tropospheric circulation, to understand the predictability of summer climate anomalies in East Asia.
It is found that the coupled models show certain capability in describing the interannual meridional displacement of the EAJ, which reflects the models' performance in the first leading empirical orthogonal function EOF mode. This capability is mainly shown over the region south of the EAJ axis. Additionally, the models generally capture well the main features of atmospheric circulation and SST anomalies related to the interannual meridional displacement of the EAJ.
Further analysis suggests that the predicted warm SST anomalies in the concurrent summer over the tropical eastern Pacific and northern Indian Ocean are the two main sources of the potential prediction skill of the southward shift of the EAJ. In contrast, the models are powerless in describing the variation over the region north of the EAJ axis, associated with the meridional displacement, and interannual intensity change of the EAJ, the second leading EOF mode, meaning it still remains a challenge to better predict the EAJ and, subsequently, summer climate in East Asia, using current coupled models.
On the structure of pulsed plasma jets. A pulsed plasma jet is a turbulent, inhomogeneous fluid mechanical discharge capable of initiating and inhancing combustion. Having shown the ability to ignite lean fuel mixtures, is now offers the potential for real-time control of combustion processes. The fluid mechanical and chemical properties of such jets are explored. The fluid mechanical structure of the jet was examined using two optical diagnostic techniques. Self-light streak photography provided information on the motion of luminous gas particles in its core.
The turbulent, thermal evolution of the jet was explored using high speed laser schlieren cinematography. By examine plasma jet generators with both opaque and transparent plasma cavities, detailed information on plasma formation and jet structure, beginning with the electric arc discharge in the cavity, was obtained.
Molecular beam mass spectroscopy was used to determine temperature and species concentration in the jet. Both noncombustible and combustible jets were studied. Species measurements in combustible jets revealed significant concentrations of radicals and products of complete as well as incomplete combustion. Planetary-scale hydraulic jumps and transonic jet-streaks in the MACDA reanalysis of the Martian atmosphere: a comparison with Earth's lower mesosphere.
The strongest seasonal wind, the northern-winter polar jet , exhibits two intriguing features: i transonic jet streaks and ii the juxtaposition of regions of shooting and tranquil flow, in the sense of Froude-number hydraulics, which suggests a planetary-scale hydraulic jump.
Mesoscale bores have been studied on Mars, but to our knowledge the above two features have not been reported elsewhere. In northern summer it swings negative. Between each winter polar jet and pole, especially in the north, there is a large spread of Q over a small domain of B, which is unlike Earth and may be related to the aforementioned hydraulic jump.
We are currently examining 3D Lagrangian fluid trajectories to better characterize the rotating hydraulics of the system as a function of season. We have utilized an extensive set of independent British Airways flight data recording wind vector and temperature observations the Global Aircraft Data Set [GADS] archive in three ways: a as an independent check of operational analyses; b as an analysis observing system experiment OSE as if the GADS observations were available in real time; and c as the corresponding forecast simulation experiment applicable to future operational forecasts.
This suite of IDL programs provides identification and comprehensive characterization of the dynamical features of the jet streams in the upper troposphere , the lower stratospheric polar night jet , and the tropopause. The output of this software not only provides comprehensive information on the jets and tropopause, but also gives this information in a form that facilitates studies of observations in relation to the jets and tropopauses.
Launched in July and designed to fly for two years, the TES mission is currently in an extended operations phase.
TES is an infrared sensor designed to study Earth's troposphere , the lowermost layer of Earth's atmosphere, which is where we live. The remainder of the TES instrument, and the Aura spacecraft itself, are operating as expected, and TES continues to collect science data. TES is one of four instruments on Aura, three of which are still operating. A PV view of the zonal mean distribution of temperature and wind in the extratropical troposphere.
The dependence of the temperature and wind distribution of the zonal mean flow in the extratropical troposphere on the gradient of pontential vorticity along isentropes is examined. The extratropics here refer to the region outside the Hadley circulation.
Of particular interest is whether the distribution of temperature and wind corresponding to a constant potential vorticity PV along isentropes resembles the observed, and the implications of PV homogenization along isentropes for the role of the tropics. With the assumption that PV is homogenized along isentropes, it is found that the temperature distribution in the extratropical troposphere may be determined by a linear, first-order partial differential equation.
When the observed surface temperature distribution and tropical lapse rate are used as the boundary conditions, the solution of the equation is close to the observed temperature distribution except in the upper troposphere adjacent to the Hadley circulation, where the troposphere with no PV gradient is considerably colder. Consequently, the jet is also stronger. It is also found that the meridional distribution of the balanced zonal wind is very sensitive to the meridional distribution of the tropopause temperature.
The result may suggest that the requirement of the global momentum balance has no practical role in determining the extratropical temperature distribution. The authors further investigated the sensitivity of the extratropical troposphere with constant PV along isentropes to changes in conditions at the tropical boundary the edge of the Hadley circulation.
It is found that the temperature and wind distributions in the extratropical troposphere are sensitive to the vertical distribution of PV at the tropical boundary. With a surface distribution of temperature that decreases linearly with latitude, the jet maximum occurs at the tropical boundary and moves with it.
The overall pattern of wind distribution is not sensitive to the change of. Streaks and vortices in near-wall turbulence. This paper presents evidence that organization of wall-normal motions plays almost no role in the creation of streaks.
This evidence consists of the theory of streak generation not requiring the existence of organized vortices, extensive quantitative comparisons between the theory and direct numerical simulations, including examples of large variation in average spacing of the streaks of different scalars simultaneously present in the flow, and an example of the scalar streaks in an artificially created purely random flow.
The sand that makes up the north polar dunes is dark. Each spot and streak is composed of the dune sand. The bright surfaces are all covered with frost. Illumination is from the lower left. The meter scale also indicates a distance of feet.
We present evidence for stratospheric mass transport into, and remaining in, the troposphere in an intense midlatitude cyclone. Coupled with parcel back-trajectory calculations, the analyses suggest two mechanisms contributed to the mass exchange: 1 A region of dynamical ly-induced exchange occurred on the cyclone's southern edge. Parcels originally in the stratosphere crossed the jet core and experienced dilution by turbulent mixing with tropospheric air.
Air with lower-stratospheric values of ozone and water vapor was left in the troposphere. The strength of the latter process may be atypical. These results, combined with other research, suggest that precipitation-induced diabatic effects can significantly modify, either decreasing or increasing parcel potential vorticity, depending on parcel trajectory configuration with respect to jet core and maximum heating regions. In addition, these results underscore the importance of using not only PV but also chemical constituents for diagnoses of stratosphere- troposphere exchange STE.
The depletion and recovery of Antarctic ozone plays a major role in changes of Southern Hemisphere SH tropospheric climate. It is the last quest for Tideborns, and will guide them to Archosaur where their future quests are located.
PWpedia Explore. Main Page All Pages. Lists Arc Codes Aerogear Pets. Gamepedia support Report a bad ad Help Wiki Contact us. Explore Wikis Community Central. Register Don't have an account? Tideborn Quests. Edit source History Talk 0. Bone Shard of Rigidity. Bone Twisted Cloth Cap. Bone-Bladed Chain Coif. Bone-Dust Headband. Bone-Laden Helmet. Bonegrinder's Bauble. Boreal Cap of Compulsion. Boreal Cap of the Conjuror. Boreal Cap of the Exhumer. Boreal Cap of the Frozen Flame. Boreal Coif of Carnage.
Boreal Coif of the Assassin. Boreal Coif of the Diviner. Boreal Coif of the Warden. Boreal Cowl of the Fang. Boreal Cowl of the Tender. Boreal Cowl of the Unwavering. Boreal Helm of Havok. Boreal Helm of the Light. Boreal Helm of the Performer. Boreal Helm of the Revenant. Boreal Helm of the Zealot. Bottled Frost Essence. Boundless Helm Symbol of Below. Boundless Helm Symbol of Compassion. Boundless Helm Symbol of Devotion. Boundless Helm Symbol of Growth.
Boundless Helm Symbol of Hate. Boundless Helm Symbol of Infestation. Boundless Helm Symbol of Integrity. Boundless Helm Symbol of Judgment. Boundless Helm Symbol of Stillness. Boundless Helm Symbol of Storms. Boundless Helm Symbol of Terror. Boundless Helm Symbol of Wildfire. Boundless Helm Symbol of the Brood. Boundless Helm Symbol of the Depths. Boundless Helm Symbol of the Farceur.
Boundless Helm Symbol of the Skeptic. Boundless Helm Symbol of the Warmonger. Bravado's Helm. Brawler's Last Grasp. Brell's Blessed Helm. Brellian Champion Helm. Brellian Enforcer's Cap. Brellium Chainmail Coif. Brellium Platemail Helm. Brigand's Circlet. Brigand's Sunken Treasure. Bright Celestine Faycite Shard. Bright Volcanic Shard. Brightly Pulsating Chronal Shear. Brightly Pulsating Crystallized Cosgrove Shard. Brilliant Cut Sodalite.
Brilliant Cut Tourmaline. Brilliant Fragment of an Innocent Dream. Brilliant Sapphire of the Infiltrator. Brilliant Sodalite of Aggression. Brilliant Sodalite of Alacrity. Brilliant Sodalite of Battle. Brilliant Sodalite of Celerity. Brilliant Sodalite of Dexterity. Brilliant Sodalite of Efficiency. Brilliant Sodalite of Extension. Brilliant Sodalite of Ferocity. Brilliant Sodalite of Haste. Brilliant Sodalite of Healing. Brilliant Sodalite of Minor Aggression. Brilliant Sodalite of Minor Alacrity.
Brilliant Sodalite of Minor Battle. Brilliant Sodalite of Minor Celerity. Brilliant Sodalite of Minor Dexterity. Brilliant Sodalite of Minor Efficiency.
Brilliant Sodalite of Minor Extension. Brilliant Sodalite of Minor Ferocity. Brilliant Sodalite of Minor Haste. Brilliant Sodalite of Minor Healing. Brilliant Sodalite of Minor Potency. Brilliant Sodalite of Minor Quickening. Brilliant Sodalite of Minor Sight. Brilliant Sodalite of Minor Sundering. Brilliant Sodalite of Minor Virility. Brilliant Sodalite of Potency. Brilliant Sodalite of Pure Aggression.
Brilliant Sodalite of Pure Alacrity. Brilliant Sodalite of Pure Battle. Brilliant Sodalite of Pure Celerity. Brilliant Sodalite of Pure Dexterity. Brilliant Sodalite of Pure Efficiency. Brilliant Sodalite of Pure Extension. Brilliant Sodalite of Pure Ferocity. Brilliant Sodalite of Pure Haste. Brilliant Sodalite of Pure Healing. Brilliant Sodalite of Pure Potency. Brilliant Sodalite of Pure Quickening. Brilliant Sodalite of Pure Sight.
Brilliant Sodalite of Pure Sundering. Brilliant Sodalite of Pure Virility. Brilliant Sodalite of Quickening. Brilliant Sodalite of Sight. Brilliant Sodalite of Sundering. Brilliant Sodalite of Virility. Brilliant Tourmaline of Aggression. Brilliant Tourmaline of Alacrity. Brilliant Tourmaline of Battle. Brilliant Tourmaline of Celerity. Brilliant Tourmaline of Dexterity. Brilliant Tourmaline of Efficiency. Brilliant Tourmaline of Extension.
Brilliant Tourmaline of Ferocity. Brilliant Tourmaline of Haste. Brilliant Tourmaline of Healing. Brilliant Tourmaline of Minor Aggression. Brilliant Tourmaline of Minor Alacrity. Brilliant Tourmaline of Minor Battle. Brilliant Tourmaline of Minor Celerity. Brilliant Tourmaline of Minor Dexterity. Brilliant Tourmaline of Minor Efficiency. Brilliant Tourmaline of Minor Extension. Brilliant Tourmaline of Minor Ferocity.
Brilliant Tourmaline of Minor Haste. Brilliant Tourmaline of Minor Healing. Brilliant Tourmaline of Minor Potency. Brilliant Tourmaline of Minor Quickening.
Brilliant Tourmaline of Minor Sight. Brilliant Tourmaline of Minor Sundering. Brilliant Tourmaline of Minor Virility. Brilliant Tourmaline of Potency. Brilliant Tourmaline of Pure Aggression. Brilliant Tourmaline of Pure Alacrity. Brilliant Tourmaline of Pure Battle. Brilliant Tourmaline of Pure Celerity. Brilliant Tourmaline of Pure Dexterity. Brilliant Tourmaline of Pure Efficiency. Brilliant Tourmaline of Pure Extension.
Brilliant Tourmaline of Pure Ferocity. Brilliant Tourmaline of Pure Haste. Brilliant Tourmaline of Pure Healing. Brilliant Tourmaline of Pure Potency. Brilliant Tourmaline of Pure Quickening. Brilliant Tourmaline of Pure Sight. Brilliant Tourmaline of Pure Sundering. Brilliant Tourmaline of Pure Virility. Brilliant Tourmaline of Quickening. Brilliant Tourmaline of Sight. Brilliant Tourmaline of Sundering. Brilliant Tourmaline of Virility. Brilliant White Pearl.
Brilliantly Pulsating Chronal Shear. Brilliantly Pulsating Crystallized Cosgrove Shard. Brittle Ruby Fragment of Brawn. Brittle Slate of Keenness. Brittle Yellow Stone. Broken Chunk of Coal. Broken Crypt Stone of Fortitude. Broken Limestone of Focus. Broken Rock of Rejuvenation. Broken Shard of Chaos. Broken Skull of Silence.
Broken Volcanic Shard. Bronze Brigandine Coif. Bronze Helm. Bronzed Crystalline Oscillator Model I. Bronzed Crystalline Oscillator Model V. Bronzed Crystalline Oscillator Model X. Bronzed Ingot of Insanity. Brother Xave's Headband.
Brown Rust Fine Plate Helm. Brownie Cut Gemstone. Bruiser's Spiked Helm. Brutal Energeiac Chain Coif. Bubonian Bandage Turban. Buccaneer's Energeiac Chain Coif. Buccaneer's Energeiac Leather Cowl.
Buccaneer's Energeiac Plate Helm. Buccaneer's Energeiac Silk Hat. Burden of Truth. Burning Acid Shard. Burning Crypt Stone Fragment. Burning Wood Coal.
Burnished Aquamarine. Burnished Bloodstone. Burnished Helm of Contemplation. Burnished Moonstone. Burnished Turquoise. Burynai Hide Cap. Cabilis Scale Cap. Calcified Ringmail Coif. Calcified Steel Helmet.
Calculating Differential Gear. Calloused Shell Helm. Candle of Hollow Souls. Canyon Queen Crown. Cap of Celestial Discipline. Cap of Detonation. Cap of Drowned Souls. Cap of Enrapturement. Cap of Flowing Time. Cap of Matter. Cap of Mirrors. Cap of Pestilence. Cap of Strife. Cap of Transcended Immortality. Cap of the Arcane Order. Cap of the Collective Initiate. Cap of the Craft Keeper. Cap of the Elite Orcs.
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Catarina's Crown of the Priestess. Cauldron-Cursed Shard of Power. Cazicite Sapphire Tiara. Celestrium Bestialcry Cowl. Celestrium Cowl of the Disciplined Animus. Celestrium Deathwatch Helm.
Celestrium Earthwall Helm. Celestrium Egoshatter Cap. Celestrium Fatecaster Coif. Celestrium Firetorrent Cap. Celestrium Graceheart Helm.
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