Original Research ARTICLE
Magnetic Fabrics and Source Implications of Chisulryoung Ignimbrites, South Korea
- 1Department of Astronomy, Space Science, and Geology, Chungnam National University, Daejeon, Korea
- 2Department of Earth and Environmental Sciences, Korea University, Seoul, Korea
- 3Department of Marine Sciences and Convergent Technology, Hanyang University, Ansan, Korea
- 4Ochang Center, Korea Basic Science Institute, Cheongju, Korea
The anisotropy of magnetic susceptibility (AMS) of late Cretaceous ash-flow tuffs in Chisulryoung Volcanic Formation, southeastern Korea was studied to define the primary pyroclastic flow azimuth. AMS data revealed a dominant oblate fabric with a tight clustering of k3 (minimum axis of magnetic susceptibility) and shallow dispersal of k1 (maximum axis of magnetic susceptibility) and k2 (intermediate axis of magnetic susceptibility). Dominance of oblate fabrics indicates clast imbrications imposed by compaction and welding. Flow azimuth inferred from AMS data indicates the nearby intrusive welded tuff (IWT) as the source of calderas for ignimbrites. Such an inference is supported by geologic investigations, in which the IWT displays eutaxitic textures nearly parallel to its subvertical contacts. The results are compatible with a unique prolate fabric and an anomalously high inclination observed for the IWT, possibly produced by rheomorphic flows as the welded tuff is squeezed along the rough-surfaced dyke walls due to agglutination.
Ignimbrites are the deposits of pyroclastic density flows ejected from explosive volcanic eruptions. Ignimbrites contain volcanic glass shards, volcanic ash, pumice fragments, and lithic fragments. Loosely consolidated ignimbrites are formed when pyroclastic material is fluidized and poorly mixed due to immense explosions associated with hot volcanic ash. Instead, post depositional re-mobilization of pyroclastic material produces rheomorphic flow structures in densely welded ignimbrites. Paleomagnetic studies of ash-flow tuffs (ignimbrites) have shown that ignimbrites, whether densely welded or loosely consolidated, bear fine-grained iron oxides that can faithfully reflect an accurate record of the geomagnetic field during rapid post-emplacement cooling (e.g., Hatherton, 1954; Beck et al., 1977; Reynolds, 1977; Geissman, 1980; Geissman et al., 1983; Schlinger et al., 1986, 1988a,b, 1991; Rosenbaum, 1993; Palmer et al., 1996; Worm and Jackson, 1999; Gee et al., 2010).
The anisotropy of magnetic susceptibility (AMS) describes magnetic fabrics of rocks where AMS triaxial ellipsoids represent maximum (k1), intermediate (k2), and minimum (k3) susceptibility eigenvectors. AMS fabrics bear information on the current directions for sedimentary rocks, magmatic flow directions for igneous rocks, and deformational kinematics for metamorphic rocks. AMS is sensitive indicator of fabric elements within welded tuffs to yield a primary flow azimuth (Wolff et al., 1989). The fundamental basis for the successful application of AMS on ignimbrite relies on the physical alignment of fine-grained iron oxides within the welded tuff (Elston and Smith, 1970; Froggatt et al., 1981; Suzuki and Ui, 1982, 1983; Kamata and Mimura, 1983).
The Chisulryoung Volcanic Formation (CVF) forms an extrusive outlier (6 × 3 km) around Chisulryoung Mountain (765 m), south-eastern part of the Korean peninsula. The CVF roughly forms an elliptical basin as the sedimentary rocks that underlie the CVF showed centripetal dips (Figure 1). The CVF lies within a broad structural basin regarded as a down sag caldera (Figure 1). According to Reedman et al. (1987), the CVF was produced by a sequence of subaerial explosive silicic volcanism that involved an emplacement of thick ignimbrites intercalated with volcanoclastic sedimentary rocks.
Figure 1. Map of Chisulryoung Volcanic Formation (CVF) (after Park, 1990) and stereographic projections of anisotropy of magnetic susceptibility (AMS) data for 19 sites in A4 member. The inset was generated from the “Generic Mapping Tools (GMT)” version 5.2.1 distributed from the School of Ocean and Earth Science and Technology, University of Hawaii at Manoa (http://gmt.soest.hawaii.edu/). For each stereographic projection, eigenvectors are displayed on an equal area plot using the lower hemisphere projection with the convention that maximum (k1), intermediate (k2), and minimum (k3) susceptibility are represented as red squares, blue triangles, and green circles. Confidence ellipses were calculated on the basis of the Jelinek method (inner ellipses with darker colors) and the site parametric bootstrap statistics (outer ellipses with brighter colors).
The CVF includes mainly densely to weakly welded acidic ash-flow tuffs which have been divided into four members (A1, A2, A3, and A4) and three intervening volcano-sedimentary members (S1, S2, and S3) according to their crystal content, variations in volcanic clast size and type, and degree of welding (Park and Kim, 1985a,b; Park, 1990; Figure 1, Table 1). A sequence of A1/S1/A2/S2/A3 is the result of the first major eruptive cycle, which predates the intrusion of the Cheogwari granodiorite (hornblende K/Ar age of 76.3 ± 11.7 Ma; Reedman et al., 1989). The A4 member is a product of the second eruptive cycle and S3 represents sedimentations during the interval between the two major eruptive cycles (Reedman et al., 1989; Park, 1990). The U/Pb zircon ages of A1 and A4 members are 72.8 ± 1.7 Ma and 67.7 ± 2.1 Ma, respectively (Jeong et al., 2015). The A4 member was intruded by the Gadaeri granite (biotite K/Ar age of 63.9 ± 1.8 Ma; Reedman et al., 1989; Table 1). An intrusive welded tuff (IWT) plug (Figure 1), with an elliptical surface exposure (700 × 400 m), displays an eutaxitic texture nearly parallel to its subvertical contacts. The IWT cuts, hence it post-dates the Cheogwari granodiorite and S3. Indeed, the IWT yielded sericite K/Ar age of 65.1 ± 1.8 Ma, statistically contemporaneous to the second eruptive cycle. In particular, Reedman et al. (1987) proposed that the IWT would be the source for the CVF.
In the present study, our main goal is to use AMS to determine flow patterns of ignimbrites for the CVF and thereby locate the source vent. When combined with other observations including petrographic description and rock magnetic measurements, the AMS data would help define the source area of the CVF. The AMS analysis explored in the present study will likely work well in other ignimbrite units of late Cretaceous age in the southeastern Korea.
The base of the CVF rests unconformably on top of late-Cretaceous mudstones and sandstones of non-marine origin. Along the gorges of eastern side, ignimbrites occur in hornfels contact with the mudstone (Figure 2A), evidence of contact metamorphism caused by hot ash-flow tuffs (Figure 2B). At the very basal contact, dyke-like flames of dark mudstones intrude the tuff layer (Figure 2C), resulting from fluidization of wet sediments at the hot tuff contact (Kokelaar, 1982).
Figure 2. (A) Contact metamorphism produced hornfels along the mudstone-ignimbrite boundaries. (B) Hornfelsic mudstone-ignimbrite boundary in a magnified scale. (C) Dyke-like flames of dark mudstones intrude the tuff layer. (D) Devitrified shards developed in a loosely welded tuff. (E) Pumice-rich tuff contains phenocrysts of resorbed plagioclase. (F) Densely welded lithic-rich tuff. (G) Rheomorphic structure with highly flattened lenticular pumice fragments and concentration of pumice fiammes (highlighted with dashed lines).
The loosely welded massive pumice-rich tuff, with a maximum thickness of 120 m, crops out at the lower part of A4 member (Figures 2D,E). The upper part of A4 member, as much as 100–120 m thick, is densely welded lithic-rich tuff (Figures 2F,G). The densely welded tuff commonly has abundant lithic fragments, but shards and pumice are exceedingly rare (Figure 2F). The densely welded tuff displays rheomorphic flow structures with highly flattened lenticular pumice fragments and concentration of pumice fiammes (Figure 2G).
The lower part of A4 member contains phenocrysts of resorbed plagioclase and lesser amount of quartz and biotite together with lithic fragments in a matrix of devitrified shards (Figures 3A,B). The pumice is in lapilli size, and it is more coarsely crystallized than the matrix shards (Figures 3A,B). The groundmass is aphanitic, consisting of cryptocrystalline and spherulitic feldspars and quartz (Figures 3A,B). In many cases, ignimbrites contain feldspars and anhedral quartz phenocrysts in a matrix with a small amount of devitrified glass shards and pumice fragments (Figures 3C,D).
Figure 3. Thin section images and microstructures of CVF. Kfs, K-feldspars; Pl, plagioclase feldspar; Qz, quartz; plain polarized light (left panel) and crossed polarizers (right panels). (A,B) Loosely welded tuff with lithic fragments in a matrix of devitrified shards. (C,D) Loosely welded pumice-rich tuff with feldspars and anhedral quartz phenocrysts in a matrix of pumice fragments. (E,F) Welded rhyolitic tuff comprise from 30 to 50% of the broken pieces of mm-sized rhyolite fragments and resorbed plagioclase (50%), K-feldspar (20%), and quartz (5%). (G,H) Rheomorphic tuff showed well-developed eutaxitic textures. For welded-tuffs, orientation of welding plane is represented as double-sided arrows.
The upper part of A4 member contains abundant rhyolite lapilli and rhyolite blocks within a mainly devitrified brown glassy and spherulitic groundmass of shards and pumice fragments (Figures 3E,F). About 30–50% of rocks are occupied by broken pieces of mm-sized rhyolite fragments. Mineralogy of mm-sized rhyolite fragments includes resorbed plagioclase (50%), K-feldspar (20%), quartz (5%), and other minor accessory components of biotite, magnetite, and apatite (Figures 3E,F). In particular, plagioclase feldspar is replaced by sericite and K-feldspar along the fractures or crystal edges (Figures 3E,F). There is evidence that some cuspate shards appeared to have been squeezed between larger silicate minerals (Figures 3E,F). They are seen to be less than a few mm long and are generally replaced by axiolitic alkali feldspar. Phenocrysts are mainly of fragmented resorbed plagioclase and quartz, but also include biotite, sphene, and magnetite (Figures 3E,F). The most abundant phenocrysts are plagioclase, mostly irregular in shape with well-developed oscillatory or normal zoning (Figures 3E,F). The next abundant phenocrysts are K-feldspars and quartz, occurring as subhedral to euhedral crystals (Figures 3E,F). Quartz, K-feldspar, and plagioclase crystals are rarely more than a few millimeters long (Figures 3E,F).
Rheomorphic tuff showed well-developed eutaxitic textures and is composed predominantly of glass shards and pumice with minor amounts of lithic fragments and crystals in a reddish devitrified matrix (Figures 3G,H). For rheomorphic tuffs, orientation of rock fabrics runs parallel to the elongation of glass shards and to the flow banding within K-feldspar (Figures 3G,H).
Rock Magnetic Properties
A detailed paleomagnetic analysis of the CVF was reported elsewhere (Jeong et al., 2015), hence, only a new rock magnetic investigation is described here. For sample 27A, the alternating-field (AF) decays of natural remanent magnetization (NRM) were relatively hard, with median destructive field (MDF) of ~30 mT (Figure 4A). Thermal demagnetization on the sister sample 27T showed a narrow unblocking temperature spectrum of 500–600°C (Figure 4B). An initial plateau with relatively high MDF in AF demagnetization and a sharp drop of NRM near 580°C in thermal demagnetization are characteristics of fine-grained magnetite (Figure 4). Existence of the distributed coercivity (sample 22A in Figure 4A) and the distributed unblocking temperature spectra (sample 22T in Figure 4B) suggests a presence of coarse-grained magnetite. Most examples fall between these extremes (sample 26A, 26T, 29A, 29T), indicating that fine- to coarse-grained magnetite is the main remanence carrier (Figure 4).
Acquisition of isothermal remanent magnetization (IRM), back-field demagnetization of IRM, and strong-field magnetic hysteresis were measured to confirm rock magnetic properties inferred from demagnetization experiments. IRM was acquired by magnetizing a sample in a strong, uniform, DC magnetic field from 30 to 1000 mT produced by an impulse magnetizer (model ASC IM-10). A stepwise back-field was applied for the samples on which IRM was imparted to determine remanent coercivity. Room temperature magnetic hysteresis measurements in a maximum field of 1.0 T were performed on an alternating gradient force magnetometer. Hysteresis loops were obtained from 109 chips. Hysteresis parameters of saturation magnetization (Ms), saturation remanence (Mrs), and coercive force (Bc) were determined after appropriate paramagnetic correction. Values of remanence coercivity (Bcr) were obtained from back-field measurements.
The results can be classified into three categories. Most results (61 out of 109 chips) were Type A, characterized by a gradual increase of magnetization up to 300 mT in IRM acquisition with ~100 mT of remanent coercivity (22K, 29K in Figure 5A). The ratio of Mrs/Ms and Bcr/Bc for the 61 chips (Figure 5B) lie in the pseudo-single-domain (PSD) range according to the conventional criteria (Day et al., 1977) or PSD trend curves (Dunlop, 2002). Type B results (42 out of 109 chips) showed a rapid increase of magnetization during acquisition of IRM and a quick decay of IRM during back-field demagnetization (26K, 27K in Figure 5A). In a Day plot, Type B results showed slight bias toward superparamagnetic contribution (Figure 5B). Type C data (6 out of 109 chips) showed a continuous increase of magnetization with increasing field (27L, 27M in Figure 5A). For Type C, the saturation is not achieved up to a maximum field of 1 T, and the remanence coercivity was > 300 mT (27L, 27M in Figure 5A). Type C data showed values of Mrs/Ms ≈ 0.4 and Bcr/Bc ≈ 2.5 (Figure 5B). It is very likely that Type C bears more than two components of magnetic minerals, with a wide range of grain size distribution for each magnetic mineral. Presence of dual components may compromise the fidelity of magnetic fabric analysis. Hence, Type C samples were excluded in further AMS analysis. It is fortunate that Type C results were found only from six chips from three paleomagnetic samples collected to the eastern side of site 27.
Figure 5. (A) Examples of normalized isothermal remanent magnetization (IRM) acquisition and the back-field demagnetization curves. For 22 and 29K, a gradual increase of magnetization up to 300 mT in IRM acquisition with ~100 mT of remanent coercivity was observed. A rapid increase of magnetization during acquisition of IRM and a quick decay of IRM during back-field demagnetization was observed for 26 and 27K. For 27L and 27M, the saturation was not achieved up to a maximum field of 1T, and the remanence coercivity was >300 mT. (B) Hysteresis data in a Day plot (Day et al., 1977) with the single-domain and multidomain mixing trend curves (Dunlop, 2002).
Applying the AMS analysis on the first eruptive cycle was impossible as the rocks are not fully exposed and caldera boundaries are mostly uncertain or lacking. Hence, in the present study, we focused only on the AMS studies on the second eruptive cycle (A4 and the IWT), which are the last product of pyroclastic activity with well-confined basin-like caldera structure (Figures 1, 6). A total of 263 oriented samples were collected at nineteen sites from the A4 member (Figure 1). We also collected 45 oriented samples at five sites from the IWT (Figure 6). It is undoubtedly true that magnetic interpretation of pyroclastics is dependent on the structural correction to restore the paleo-horizons. It would be fair to mention that no structural correction was employed in the present study as the degree of bedding tilts was unavailable.
Figure 6. Stereographic projections of anisotropy of magnetic susceptibility AMS and characteristic remanent magnetization (ChRM) data for 5 sites in the intrusive welded tuff (IWT). For each stereographic projection, eigenvectors are displayed on an equal area plot using the lower hemisphere projection with the convention that maximum (k1), intermediate (k2), and minimum (k3) susceptibility are represented as red squares, blue triangles, and green circles. Confidence ellipses were calculated on the basis of the Jelinek method (inner ellipses with darker colors) and the site parametric bootstrap statistics (outer ellipses with brighter colors).
AMS was determined by measuring magnetic susceptibility (k) induced along different directions for each sample. We used a computerized magnetic susceptibility meter on a Kappabridge KLY-2, following a rotatable scheme with 15 measuring positions (Jelinek, 1976). The results were then analyzed using a commonly used software “PmagPy” (Tauxe, 2010), where confidence ellipses were calculated on the basis of the Jelinek method (inner ellipses) and the site parametric bootstrap statistics (outer ellipses) (Figures 1, 6). Eigenvalue of normalized mean magnetic susceptibility and directions of the associated eigenvectors for k1, k2, and k3 are provided (Tables 2, 3). Eigenvectors were displayed on an equal area plot using the lower hemisphere projection with the convention that maximum (k1), intermediate (k2), and minimum (k3) susceptibility are represented as squares, triangles, and circles (Figures 1, 6). For A4 member, the result was compatible with the oblate fabrics with a tight clustering of k3 near the vertical and a distributed k1 and k2 directions at shallower foliation planes (Figure 1). Contrary to A4 member, the IWT showed a distinctive prolate fabric with high inclination of k1 (Figure 6).
Mean magnetic susceptibilities were clustered in the range from 5.5 × 10−5 SI to 7.3 × 10−3 SI (Figure 7A). The degree of anisotropy Pj (Jelinek, 1981) was <1.101 (Tables 4, 5). Specimen level data were tabulated with eigenvalues and directions of the associated eigenvectors for k1, k2, and k3 (Supplementary data repository, Data-1.xls in Excel format). In particular, the IWT showed a very low degree of anisotropy (Pj < 1.05) (Figure 7A). There is a general correlation that the degree of anisotropy was inversely proportional to the mean values of magnetic susceptibility (Figure 7A). In fact, results with high bulk susceptibility have low degree of anisotropy while those with low bulk susceptibility have high degree of anisotropy (Figure 7A).
Figure 7. (A) Mean values of magnetic susceptibility are inversely proportional to the degree of anisotropy (Pj). (B) Magnetic fabric was analyzed by comparing Pj in relation to the shape parameter (T). While the A4 member showed a prevalent oblate fabric, the IWT showed a dominance of prolate fabric.
When magnetic fabric was analyzed in terms of Pj vs. shape parameter (T) (Jelinek, 1981), results for A4 member are biased toward positive shape parameters (with two exceptionally low values of T > −0.08), suggesting a prevalent oblate fabric due to welding process (Figure 7B). A notably distinct negative trend with T < −0.11 was observed for the IWT (Figure 7B), indicating a predominant prolate fabric.
The successful application of AMS method relies on the fact that the k1 aligns parallel to the flow azimuth of ignimbrites. This consensus is true in the case of a normal fabric where the elongation of PSD or MD grains of magnetite commonly parallels the flow azimuth. On the other hand, it has been shown that SD magnetite exhibits an “inverse” fabric where the k3 aligned along the elongated axes of the samples (Potter and Stephenson, 1988; Rochette, 1988; Ort et al., 1999). Thus, it is necessary to avoid the presence of an inverse fabric that can compromise the past flow direction. Several lines of experimental observations indicate that PSD and MD magnetites are the main remanence carriers. First, both AF and thermal demagnetization spectra showed typical characteristics of PSD and MD magnetite (Figure 4). Second, acquisition of IRM and back-field demagnetization IRM also demonstrated the presence of PSD and MD magnetites (Figure 5A). Third, values of remanence ratio from the magnetic hysteresis measurements were 0.2–0.3, suggesting fine-grained non-SD magnetite as remanence carriers (Figure 5B). Thus, we can safely exclude the presence of an inverse fabric for A4 member and the IWT.
In terms of lithologic ground, ignimbrites are dominated by felsic minerals such as quartz, k-feldspar and plagioclase. There is a possibility that these silicates host magnetite inclusions along the cleavage planes. Then it is natural to consider that magnetite inclusions within silicates would be finer than those in the matrix. If so, AMS would be controlled by relatively coarser grains of magnetite while remanent magnetization would be dominated by relatively finer grains. The best candidate for such a bimodal behavior would be the type B samples (Figure 5). To check a possible composite nature of the AMS fabric, difference between AMS and anisotropy of partial anhysteretic remanent magnetization (partial AARM) was compared. In general, AMS fabrics and partial AARM tensors are similar unless there is a composite fabric (Aubourg et al., 1995, 2000; Werner and Borradaile, 1996; Robion et al., 1999; Rochette et al., 1999; Trindade et al., 1999). In practice, a composite fabric may cause distinctively different directional patterns among AMS, soft partial AARM, and hard partial AARM (Aubourg and Robion, 2002). In a spirit of Aubourg and Robion (2002), soft partial AARM (0–30 mT) and hard partial AARM (30–100 mT) were produced in a bias DC field of 100 μT. Samples were AF demagnetized to 100 mT before each partial ARM acquisition experiment. We set AC boundary at 30 mT because AF demagnetization of NRM typically yielded median destructive field of ≈30 mT. Directions of AMS, soft partial AARM, and hard partial AARM are consistent with one another, indicating that azimuthal direction inferred from AMS is not compromised by the composite fabric (Figure 8). Decreasing degree of anisotropy with increasing magnetite content (Figure 7A) may reflect an isotropic rather than preferential accretion of finer grains, and the resulting partial AARM tensor became more triaxial than the oblate AMS fabric (Figure 8).
Figure 8. Stereographic projections of anisotropy of magnetic susceptibility (AMS), anisotropy of partial anhysteretic remanent magnetization (partial AARM). Soft partial AARM (0–30 mT) and hard partial AARM (30–100 mT) were produced in a bias DC field of 100 μT. Samples were AF demagnetized to 100 mT before each partial ARM acquisition experiment. For each stereographic projection, eigenvectors are displayed on an equal area plot using the lower hemisphere projection with the convention that maximum (k1), intermediate (k2), and minimum (k3) susceptibility are represented as red squares, blue triangles, and green circles. Confidence ellipses were calculated on the basis of the Jelinek method (inner ellipses with darker colors) and the site parametric bootstrap statistics (outer ellipses with brighter colors).
For A4 member, the magnetic foliations were prevailing while magnetic lineation was weakly developed (Figure 1). Occurrence of prominent oblate fabrics in A4 member (Figure 1) indicates imbrications of pyroclastic material imposed by compaction and welding (Grunder et al., 2004). It is conjectured here that magnetite was probably oriented by laminar pyroclastic density flows in the later stages of pyroclastic transport.
There are two similar but fundamentally different opinions in determining the flow patterns of ignimbrites. The first opinion describes that magnetic minerals align themselves parallel to the flow azimuth and the magnetic foliation reflects the imbrication process. In principle, the AMS ellipsoid of k1 and k2 forms the plane of welding in ignimbrites, on which k1 lies parallel to the flow azimuth (e.g., Wolff et al., 1989; Rochette et al., 1992, 1999; Palmer and MacDonald, 2002; Bolle et al., 2010; Ort et al., 2013). If so, ignimbrites may reveal k3 pole distribution of magnetic foliation and have distinctive bilobed dispersal patterns traverse to flow direction (e.g., MacDonald and Palmer, 1990; Palmer et al., 1991; Palmer and MacDonald, 1999, 2002). The second opinion adopts analogy to the imbrication of stream clasts, as the plane of magnetic foliation (k1 and k2) tilts downward and upstream (Hillhouse and Wells, 1991; Petronis and Geissman, 2009). Then, the flow direction is indicated by the azimuthal orientation of the downward end of k1 on stereographic projections.
The preceding discussion on either opinion indicates that the flow azimuth of ignimbrites can be determined by connecting mean directions of k1 or k3 between neighboring sites. In the present study, pyroclastic flow directions of ignimbrites inferred by simply tracing back the directions of k1 or k3 are practically identical (Figure 9). Such intriguing directional similarity in tracing k1 or k3 is valid under the imposed limits of directional confidence of k1, k2, and k3 for the Jelinek method (darker colors) and the site parametric bootstrap analysis (brighter colors) (Figure 9). Hence, for each site, flow azimuth of ignimbrites was graphically expressed by connecting lines from k1 to k3 directions in ring plots (Figure 9). Estimated flow azimuth of individual sites was diverging at the northern and southern ends, but was converging at the central bottleneck area (Figure 9). Sites in western margin showed southeastern flow azimuth while those in eastern margin revealed southwestern flow azimuth (Figure 9). It is puzzling that vectorial flow direction from k1 to k3 is prevailingly upward, difficult to imagine unless pyroclastic surges produce inverted welding structure. Although we cannot completely rule out the possibility, a local tectonic displacement or a regional tilting may alter the geometry of welding foliation.
Figure 9. For each site, flow azimuth of ignimbrites was graphically expressed by connecting lines between k1 and k3 directions in ring plots. Directional confidence of k1, k2, and k3 was displayed for the Jelinek method (darker colors) and the site parametric bootstrap analysis (brighter colors). Assuming a single source area, the geometrically most probable source would be close to the vicinity of the IWT.
Assuming a single source area, the geometrically most probable source would be close to the vicinity of the IWT (Figure 9). Our interpretation is in accordance with the earlier inference that the IWT would be the source of the CVF (Reedman et al., 1987). It can therefore be concluded that the IWT is the source of A4 member (Figure 9). It also matches well with the geochemical data where the ratio of Zr/TiO2 and Nb/Y showed tight clustering for A4 member and the IWT (Park, 1990). However, it remains to be shown whether comparable studies on detrital zircon might come to the same conclusion.
A final point of discussion involves unique magnetic features observed in the IWT. As a secondary coherent viscous mass flow after the emplacement (Wolff and Wright, 1991), rheomorphism generally produces a prolate fabric (Ellwood, 1982). The IWT showed eutaxitic textures nearly parallel to its subvertical contacts (Park, 1990). For the IWT, AMS data indicated poor to moderate minimum and intermediate axial clusters but good to excellent maximum axial clusters, which are consistent with the dominant prolate fabric patterns with respect to a near-vertical vent wall (Wolff et al., 1989). In addition, the IWT exhibited an anomalously high angle of magnetic lineation (Figure 6). It is worthy of note that characteristic remanent magnetization of IWT also yielded an anomalously high magnetic inclination (Figure 6). Therefore, it is plausible that the rheomorphism is responsible for the high magnetic inclination and prolate AMS fabric of the IWT as the welded tuff is squeezed along the rough-surfaced dyke walls due to agglutination.
1. The anisotropy of magnetic susceptibility (AMS) of late Cretaceous ash-flow tuffs in (CVF) showed a dominant oblate fabric with a tight clustering of k3 (minimum axis of magnetic susceptibility) and shallow dispersal of k1 (maximum axis of magnetic susceptibility) and k2 (intermediate axis of magnetic susceptibility). Presence of predominant oblate fabrics in ignimbrites indicates clast imbrications imposed by compaction and welding.
2. Flow azimuth of ignimbrites inferred by tracing back the direction of k1 or k3 of each site is similar. Therefore, flow directions of ignimbrites were estimated from k1 to k3 directions in ring plots, strongly suggesting that the IWT is a potential source of caldera for ignimbrites. Such an inference is supported by geologic investigations, in which the IWT displays eutaxitic textures nearly parallel to its subvertical contacts.
3. A unique prolate fabric with an anomalously high magnetic inclination was observed for the IWT, resulting from rheomorphic flows as the welded tuff is squeezed along the rough-surfaced dyke walls due to agglutination.
HH and YY equally contributed to the draft of the work, data acquisition, and interpretation of data for the work. YY, SD, DS, and JK designed the work, revised the draft for intellectual merit, and maintained the integrity of investigation.
This work was supported by the Polar Academic Program (PD16010), Korea Polar Research Institute, 2016.
Conflict of Interest Statement
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Lae Hee Han and Su Min Lee provided tremendous help in the field.
The Supplementary Material for this article can be found online at: https://www.frontiersin.org/article/10.3389/feart.2016.00079
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Keywords: ignimbrites, anisotropy of magnetic susceptibility, chisulryoung, magnetic fabrics, welded tuff
Citation: Hong H, Yu Y, Doh S-J, Suk D and Kim J (2016) Magnetic Fabrics and Source Implications of Chisulryoung Ignimbrites, South Korea. Front. Earth Sci. 4:79. doi: 10.3389/feart.2016.00079
Received: 11 January 2016; Accepted: 02 August 2016;
Published: 17 August 2016.
Edited by:Qingsong Liu, Institute of Geology and Geophysics, China
Reviewed by:France Lagroix, Institut De Physique Du Globe De Paris, France
Maodu Yan, Institute of Tibetan Plateau Research, China
Copyright © 2016 Hong, Yu, Doh, Suk and Kim. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Yongjae Yu, email@example.com