ORIGINAL RESEARCH article
Sensitivity of Sediment Magnetic Records to Climate Change during Holocene for the Northern South China Sea
- 1Key Laboratory of Marginal Sea Geology, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou, China
- 2Research School of Earth Sciences, Australian National University, Canberra, ACT, Australia
- 3University of Chinese Academy of Sciences, Beijing, China
- 4Guangzhou Marine Geological Survey, Guangzhou, China
Magnetic property has been proved to be a sensitive proxy to climate change for both terrestrial and marine sediments. Based on the schedule frame established by AMS 14C dating of foraminifera, detail magnetic analyses were performed for core PC24 sediments at sampling intervals of 2 cm to discuss magnetic sensitivity of marine sediment to climate during Holocene for the northern South China Sea. The results indicated that: (1) Concentration dependent magnetic parameters are positive corresponding to variation of temperature. The frequency dependent susceptibility coefficient basically reflected the variation in humidity; (2) χARM/SIRM was more sensitive to detrital magnetite particles and SIRM/χ was more effective to bioge χARM/SIRM and SIRM/χ are corresponding to precipitation and temperature, respectively; (3) the Holocene Megathermal in the study area was identified as 7.5–3.4 cal. ka BP. The warmest stage of Holocene for the study area should be during 6.1–3.9 cal. ka BP; (4) The 8 ka cold event was characterized as cold and dry during 8.55–8.25 cal. ka BP; (5) During early and middle Holocene, the climate combinations were warm dry and cold wet. It turned to warm and wet after 2.7 cal. ka BP.
The South China Sea (SCS), one of the largest margin seas in the world, is located between the Pacific Ocean and the Asian continent. The SCS can be subdivided into northwestern, southwestern, and eastern sub-basins (He and Chen, 1987; Liu, 1992). As the most frequent activity area of East Asian monsoon, it has become a hot area of climate research (Chen et al., 2003; Wei et al., 2006; Wan et al., 2007; Hu et al., 2012). As suggested by Han and Fyfe (1995) and Wang (2009), it is an important place for paleoenvironment and paleoclimate research and can be considered as another natural laboratory besides the Chinese Loess Plateau for the study of regional response to global climate change and its driving forces.
During the last decades, magnetic properties has been proven to be sensitive proxies to climate change and has been widely applied in climatic and environmental evolution research using loess-paleosol sequences, ice cores as well as marine sediments (Moreno et al., 2002; Maher, 2007; Heslop and Roberts, 2013; Zan et al., 2015). Previous studies suggested that marine sediment was one of the most important signal carriers of climate change. Therefore, marine sediment magnetic records have been becoming another focus of paleaoclimate research (Arai et al., 1997; Kissel et al., 1999; Oldfield et al., 2003; Tang et al., 2003; Kumar et al., 2005; Sangode et al., 2007; Xu et al., 2011; Larrasoaña et al., 2015). Many magnetic results of the SCS sediments were reported since the past decade. However, previous research indicated that sediment magnetic response to climate change varied much among different regions within the South China Sea (SCS) (Wang et al., 1993; Hou et al., 1996; Kissel et al., 2003; Yim et al., 2004; Yang et al., 2007; Ouyang et al., 2014a). Zhang et al. (2010) compared many cores within the SCS and pointed out that the SCS could be divided into at least two regions according to variation characteristics of magnetic susceptibility. Magnetic susceptibility (MS) varied parallel with the calcium carbonate percent content and foraminifera δ18O curves during late Quaternary at the region close to Dongsha Islands. However, a mirror image relationship was appeared between variation of magnetic susceptibility and calcium carbonate percent content during late Quaternary at western and southern SCS. Many factors such as water depth and early diagenesis can affect the MS variation characteristics. In addition, different climate change response might play more important role on sediments magnetic properties. For example, previous comparison between DP1144 and ODP1143 indicated that different climate change response was appeared between the northern and southern SCS (Jin and Jian, 2008).
In the present study, a detailed environmental magnetic analysis was performed for a sediment core PC24 collected from the northern SCS. Our main aim is to identify the dynamic of sediment magnetic variation and it sensitivity and magnetic response to climate change during Holocene for the northern SCS.
Materials and Methods
Sampling and Geological Background
The 7.6-m-long piston core (PC24) studied here was recovered by the Guangzhou Marine Geological Survey in June, 2008, from the northwestern sub-basin (latitude/longitude: 17.4°N, 113.7°E) at a water depth of 3433 m (Figure 1). The recovered sediments consist of clayey silts that are yellow-gray and gray in the upper 1.01 m and gray from 1.01 to 7.6 m. Occasional fine yellow sand layers are preserved throughout the core. The studied core was split and one half was continuously sampled by inserting plastic cubes (2 × 2 × 2 cm3) into the split face of core sections. Sediment at the base of each cube was then cut away with a non-magnetic knife, and the cubes were sealed with plastic end-pieces and clear polyethylene tape. In total, 380 magnetic samples were taken, along with bulk sediment samples at the same depths.
Figure 1. (A) Study area and location of the studied core PC24 and cores for comparison (redrawn from Ouyang et al., 2014a), and (B) Sediment lithology of PC24 (redrawn from Ouyang et al., 2014b). The solid and dashed arrows denote surface-water circulation pattern in the SCS during winter and summer, respectively.
We attempted to extract foraminifera from the sediment to obtain a δ18O record for the whole core, but failed because the site lies below the calcite compensation depth (CCD). The CCD is located between water depths of 3000 and 3500 m in the study area, although variable positions have been reported (Rottman, 1979; Thunell et al., 1992; Miao et al., 1994; Wang et al., 1995; Wei et al, 1997). Fortunately, foraminifera were obtained for some layers and an age model was developed for the last 9160 cal a BP. Therefore, magnetic properties and its sensitivity to climate change were discussed only for Holocene recorded by the upper 190 cm sediments (95 magnetic samples) in the present paper.
Grain size and concentration of magnetic minerals of a sample can be identified from magnetic properties (Thompson and Oldfield, 1986; Verosub and Roberts, 1995; Evans and Heller, 2003). A suite of mineral magnetic measurements were made on samples from the studied PC24 sediments. The low-field magnetic susceptibility (χ) was measured for all discrete samples using a Kappabridge MFK1-FA (AGICO) magnetic susceptibility meter at both low (976 Hz) and high (15,616 Hz) frequencies (defined as χlf and χhf). Frequency-dependent susceptibility χfd% (reflecting the contribution of superparamagnetic (SP) particles to magnetic susceptibility) was calculated by the equations: χfd = χlf–χhf and χfd% = 100 × (χlf–χhf)/χlf (Evans and Heller, 2003). The temperature dependence of susceptibility (κ-T curves) was measured in an argon atmosphere for nine representative samples from room temperature to 700°C using the Kappabridge MFK1-FA equipped with a CS-4 heating device. These measurements were performed at the Guangzhou Institute of Geochemistry, Chinese Academy of Sciences. All other magnetic measurements were carried out at the Australian National University. An anhysteretic remanent magnetization (ARM) was imparted to all samples in a 0.05 mT direct current (DC) bias field with a superimposed 100 mT peak AF. Magnetic susceptibility of ARM was obtained by dividing ARM with the DC bias field. An isothermal remanent magnetization (IRM) was imparted in a 900 mT DC field and a 300 mT backfield, which are treated here as a saturation IRM (SIRM) and a IRM−300, respectively a using a 2-G Enterprises 760 pulse magnetizer. S-ratios (S−300) were calculated as S−300 = (1-IRM−300mT/SIRM)/2, following the definition of Bloemendal et al. (1992). Hysteresis loops with a maximum applied field of 0.5 T, IRM acquisition curves with a maximum applied field of 1.0 T, and backfield demagnetization curves were measured for tens of representative samples using a Princeton Measurements Corporation MicroMagTM 3900 vibrating sample magnetometer (VSM). Values of the saturation magnetization (Ms), saturation remanent magnetization (Mrs) and coercivity (Bc) were obtained from the hysteresis loops, while the coercivity of remanence (Bcr) was determined from the backfield IRM demagnetization curves. Cumulative log-Gaussian (CLG) analyses were completed for all IRM acquisition curves using the IRMUNMIX2_2 and the IRM_CLG1 routines (Kruiver et al., 2001; Heslop et al., 2004).
Twenty bulk samples (10 cm space) were selected for elemental analysis. Concentration of major elements (Al, Ba, Ca, Fe, K, Mg, Mn, Na, Si, and Ti) was measured using the method of X-ray fluorescent spectrum instrument and melting glass. Content of trace elements including rare earth elements was determined by an inductively coupled plasma mass spectrometry using melting method. These elemental analyses were performed at the ALS chemex (Guangzhou) Co., Ltd. Subsamples of ca. 0.5 g were digested for 6 h with < 10% HCl at room temperature and then heated in a water bath for up to 2 h at 80°C to completely remove carbonate. They were again oven-dried at 80°C after being washed at least 6 times to pH > 6 with distilled water. Sequentially, concentration of total organic carbon (TOC) and δ13CTOC were measured using an Elementar IsoPrime 100 isotope ratio mass spectrometry (IRMS) instrument interfaced with an Elementar PYRO cube instrument for elemental analysis (EA) at the State Key Laboratory of Isotope Geochemistry, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences.
Though the date frame of the whole core need further analysis, the dates upper sediments were accurately given by the results of AMS 14C dating for foraminifera (mainly Globorotalia menardii and Globigerinoides sacculifer). The radiocarbon ages for upper sediments from the studied core PC24 are given in 1 Table 1 and Figure 2.
Figure 2. Age-depth models for upper sediments of the studied core (PC24). (A) AMS 14C calibrated ages; (B) ages (triangles) using for sedimentary rate and date calculation for every stage and each sediment depth and calculated date of each depth for upper 190 cm sediments.
The calibrated radiocarbon ages vary nearly linear with depth for the upper 189 cm sediments (Figure 2A). However, the ages from the depth 169 to 269 cm rarely increases (Table 1 and Figure 2A). The foraminifera selection results indicated that the total materials for radiocarbon age measurements within the upper 189 cm and the 269 cm sediments were more than 8 mg and less than 3 mg, respectively. Therefore, although the other ages of the upper 189 cm sediments are reasonable, the radiocarbon age of the 269 cm sediments should be much different from its real age and it was incredible. The date for the sediment at depth of 269 cm was ignored during date frame establishment. Sedimentary rate for every stage using the four ages illustrated in Figure 2B. Apparently, sedimentary rate differed among different stages and it decreased sharply after 7350 cal. a BP. Therefore, date for each sediment depth was acquired by stepwise calculation using different sedimentary rate and the analyzed AMS 14C results illustrated in Figure 2B. The calculated dates of each depth using in the following discussion for upper 0–190 cm sediments are illustrated in Figure 2B.
As the previous published research for the core PC24 (Ouyang et al., 2014a) suggested that both detrital (mainly pseudo single domain, PSD) and biogenic (mainly single domain, SD) magnetite were coexisted within core PC24 sediments. κ-T curves, hysteresis loops, IRM acquisition and backfield demagnetization curves, gradient acquisition plot of IRM acquisition curves from CLG analysis are illustrated at Figure 3 for representative samples.
Figure 3. Mineral magnetic properties for sediments from core PC24. Representative (A) κ-T curves, (B) hysteresis loops before and after paramagnetic slope correction, (C) IRM acquisition and backfield demagnetization curves, and (D) gradient acquisition plot (GAP) of IRM acquisition curves. The GAP is decomposed into 2 components due to detrital (magnetically softer, wide dispersion; component 1) and biogenic (magnetically harder, narrow dispersion; component 2) magnetite.
κ–T curves for 9 selected samples consistently reveal a major κ decrease at the Curie temperature of magnetite (Figure 3A), indicating the presence of magnetite within the studied sediments. For some samples, neoformation of magnetite via conversion of Fe-clay minerals is evident during heating (Deng et al., 2004; Zhang et al., 2012), which causes κ to increase above 300°C up to just below the Curie temperature of magnetite. The much higher κ values during cooling processes prove the production of new magnetite (Figure 3A). Some single domain (SD) magnetite particles are proved to be present within some samples by Hopkinson peaks in the heating curves (Figure 3A) (Dunlop and Özdemir, 2015). Hysteresis loops before and after paramagnetic slope correction (Figure 3B) indicated that paramagnetic components and low coercivity spectra were determined. According to the results of Hysteresis loops, IRM acquisition curves and Bcr values, low coercivity magnetic minerals were predominated the studied sediments (Figures 3B,C). Two low coercivity magnetic components were identified from the CLG analysis of IRM acquisition curves (Figure 3D) (Kruiver et al., 2001). For the analyzed samples, average contributions to the IRM of the two components are 50.3 and 49.6%, with average B1∕2 of 30.5 mT and 40.8 mT, respectively. These results indicate that the two magnetic components are magnetite with different grain sizes.
Mean Bcr/Bc and Mrs/Ms values for 20 analyzed samples are 2.33 and 0.25, respectively. As discussed within the previous article (Ouyang et al., 2014a), granularity of magnetic minerals reflected by Day-plot, King-plot and FORC diagrams suggested both detrital pseudo-single domain (PSD) and biogenic single domain (SD) magnetite particles (DM and BM, respectively) were concurrence within the studied sediments. As shown in the previous published article (Ouyang et al., 2014a), both non-interacting biogenic magnetite and a detrital magnetite were identified from the FORC diagrams (not shown here) of all sediments from the whole core PC24.
Vertical Variation of Magnetic Properties
The concentration dependent parameters χ, χARM, and SIRM appeared basically consistent variation trends (Figures 4A–C). Total content of magnetite reflected by these parameters remained relatively stable during 9.16–7.4 cal. ka BP, and increased to a high level following with a sharp decrease at 3.4 cal. ka BP. After experiencing a decreasing trend, they increased gradually after 2.7 cal. ka BP. Although content of different origin magnetite can't be calculated exactly, content of detrital and biogenic magnetite reflected by IRM_DM and IRM_BM varied reversely during 6.8–3.9 cal. ka BP (Figures 4H,I).
Figure 4. Stratigraphic variations of magnetic parameters. IRM_DM and IRM_BM present IRM carried by detrital and biogenic magnetite, respectively. The shaded areas represent the 8 ka cold event and the Holocene Megathermal, respectively.
The value of the S-ratio can reflect the relative amounts of high versus low coercivity magnetic minerals (Thompson and Oldfield, 1986; Verosub and Roberts, 1995; Evans and Heller, 2003). It is close to 1.0 for pure ferromagnetic samples, and decreases with increasing contribution of antiferromagnetic minerals. The pre-mentioned magnetic mineralogy results indicated that two components of magnetite with different grain size were coexisted within the studied sediments. As a result, the S−300 values of the studies sediment core were close to 1.0 (varied between 0.94 and 0.98, Figure 4D). Variation of S−300 may reflect the relative contribution of DM and BM to total magnetics.
Generally, variation of grain size dependent indicators χARM/SIRM and SIRM/χ was consistent in sediment cores. However, these two parameters varied oppositely within our studied sediment core (Figures 4F,G). During early and middle Holocene, both χARM/SIRM and SIRM/χ kept relatively stable. SIRM/χ increased sharply since 6.1 cal. ka BP and decreased to the lowest value at 3.4 cal. ka BP. High and low values of SIRM/χ and χARM/SIRM were appeared after 2.7 cal. ka BP, respectively.
Origin of Magnetic Particles
As pre-mentioned by coercivity distribution, both detrital (PSD) and biogenic (SD) magnetite were concurrence within the studied sediments (Figure 3D). Scatter plot between χlf and χARM illustrated within Figure 7B indicated that biogenic SD magnetite particles within the studied sediments played important contribution to χ of the studied sediments. The significant positive correlation between χlf and SIRM (Figure 7B) indicated that the variation of these two parameters was largely controlled by a common effect of type and concentration of magnetic minerals. Differed from many previous studies (Yu and Oldfield, 1989; Ouyang et al., 2013), no obvious correlation was appeared between χlf and χfd% (Figure 7A), indicating that superparamagnetic (SP) particles were not the main controller for magnetic susceptibility. However, some superparamagnetic (SP) magnetite particles might be also appeared within the studied sediments due to relatively high average value of χfd (average 4.54 × 10−9 m3/kg) and significant paramagnetic signals during hysteresis measurements (Figure 3B).
Many sources can bring the mentioned SP, PSD, and SD magnetic particles to marine sediments. However, magnetic minerals from different sources can play significant and different potential impact on sediment magnetic properties. Hilton (1987) pointed that eolian deposition and magnetic bacteria might be important in deep-ocean sediments. According to the results of provenance analysis for the study area, besides sediments carried by ocean current, some fluvial alluvial sediments as well as eolian dust can also be deposited at the station of the study core. Weathering materials around the study area can be transported by runoff to deposit in the sampling station. Meanwhile, eolian dusts as well as fly ash can be transported by wind to the waters (Liu et al., 2007, 2008, 2010; Wei et al., 2012). Therefore, the PSD and SP detrital magnetite should be from river input and north Asian eolian particles. In addition, eolian particles and river input might mainly contribute to SP and PSD magnetic particles, respectively. As suggested by the previous published article of the studied core, the biogenic SD magnetite particles should be from marine authigenesis or post-deposition bacterial action.
Dypvik and Harris (2001) pointed out that Th/U ratio was sensitive to redox condition. Th/U ratio below one indicated reducing conditions. The high values of this ratio (4.14–6.55) for the studied PC24 sediments indicated an oxidative deposition condition. Moreover, the relatively low value of SIRM/κ (10.9–17.2 kA/m) showed that no iron sulfide was present within the sediments and the influence of early reductive diagenesis on the sediments was very limited.
Sensitive Magnetic Parameters to Climatic Variation
Although concentration dependent magnetic parameters χlf, χARM and SIRM were sensitive to different grain size magnetic particles, a significant positive correlation was appeared among these parameters (Figure 7B). This correlation implies that total content of all magnetic particles is affected by a common factor. Total concentration of magnetic minerals within marine sediments was proved to be related to variation of temperature despite that sediment magnetic response to climate change differed from different regions within the SCS (Hou et al., 1996; Tang et al., 2003; Zhang et al., 2010; Ouyang et al., 2014a). Variation of χlf, χARM and SIRM for the studied core PC24 was coincident with variation of χlf for a previous reported core DSH-1C from the northern SCS before 6 cal. ka B.P (Figure 5B) (Luo et al., 2010). Generally, temperature can play important impact on sea level, weathering intension, and marine authigenesis (Chen et al., 2000). Though variation of TOC and δ13Corg was not exactly same to concentration dependent magnetic parameters, the changing trends of these proxies were consistent. Furthermore, a significant positive correlation was appeared between Al/Ti ratio, which can reflect weathering intensity of source area (Zhao and Yan, 1994; Huang et al., 2016), and concentration dependent magnetic parameter SIRM (Figure 8A). In addition, χlf, χARM and SIRM showed consistent variation trends with air temperature (AT) of the Pearl River Delta (PRD) (Fang et al., 1991), sea surface temperature (SST) of core NS02G (Kong et al., 2014) and core 17940 (Wang et al., 1999) during most stages (Figure 5). Therefore, concentration dependent magnetic parameters χlf, χARM and SIRM of the studied sediments might have a positive response to variation of temperature.
Figure 5. Variation of concentration dependent magnetic parameters and TOC contents and δ13Corg of the studied core PC24 compared with the low-field magnetic susceptibility of core DSH-1C (Luo et al., 2010), air temperature (AT) of the Pearl River Delta (PRD) (Fang et al., 1991), sea surface temperature (SST) of core NS02G (Kong et al., 2014) and core 17940 (Wang et al., 1999).
PSD and SP magnetite particles might be related to river runoff/precipitation and wind speed/dryness, respectively due to their sources and transportation dynamics. Previous research suggested that variation of Zr and Rb within sediments was controlled by unitary factor (Wronkiewicz and Condie, 1987). Furthermore, Dypvik and Harris (2001) pointed out that Zr/Rb ratio of sediments might reflect the strength of wind carrying. The consistent changing trends of χfd (%), Zr/Rb ratio of the studied core PC24 and clay % of core ODP 1144 indicated that χfd (%) should correspond to windy intensity. As Wang (1989) pointed, Rb/Sr ratio of marine sediments can reflect the quantity of eolian dust input. High Rb/Sr reflects intense weathering of source and high eolian dust input (Huang et al., 2007; Wang et al., 2012; Luo et al., 2015). High χfd (%) reflects high contribution of SP particles to magnetic susceptibility (Thompson and Oldfield, 1986; Verosub and Roberts, 1995; Evans and Heller, 2003). The significant positive correlation between these two parameters (Figure 8B) indicated intense weathering dust varied simultaneously with SP magnetic particles within sediments (Zan et al., 2015). According to the transportation of dust, more dust deposition within marine sediments must be due to windy and dry climate. Therefore, χfd (%) of the studied sediments should be related to humidity of the study area. Higher Rb/Sr ratio and χfd (%) is corresponded to drier climate.
As pre-mentioned, χARM/SIRM varied reversely to SIRM/χ. Moreover, correlation analysis results indicated that a significant negative correlation was appeared between these two parameters for the studied sediments (R2 = 0.60). These results should be caused by the different relative contributions of the two components of magnetite during different periods. Comparing to the contribution of the two magnetite components to SIRM, contribution of DM and BM to SIRM was significant positive related to χARM/SIRM and SIRM/χ (Figure 9), respectively. Therefore, it can be speculated that χARM/SIRM was sensitive to detrital magnetite particles and SIRM/χ was effective to biogenic magnetite particles. Since SP particles do not carry any magnetic remanence, χARM/SIRM is specifically reflected the detrital PSD magnetic particles. Coarser particles can be transported into the study area within more humid climate due to higher runoff. Moreover, χARM/SIRM consistently varied with Zr/Rb ratio, χfd (%) and clay % of core ODP 1144 (Figure 6). Therefore, variation of χARM/SIRM should be consistent with dryness of the study area. As pre-mentioned, biogenic magnetite particles should be from marine authigenesis or post-deposition bacterial action. The basically consistent trends of SIRM/χ and relative sea level of the PRD (Fang et al., 1991) indicated that SIRM/χ might be corresponding to temperature which is related to seal level (Figure 6).
Figure 7. Scatter plot among magnetic parameters. (A) χlf versus χfd (%); (B) Relationship between χlf and χARM, and between χlf and SIRM.
Figure 9. Correlation between grain size dependent magnetic parameter and contribution of magnetic components to SIRM. (A) Contribution of detrital magnetite to SIRM and χARM/SIRM; (B) Contribution of biogenic magnetite to SIRM and SIRM/χ.
Summarily, climatic sensitive magnetic parameters include concentration and grain size dependent indicators. High values of χfd (%) and χARM/SIRM correspond to dry climate. Furthermore, χARM/SIRM should be more effective due to relatively low concentration of SP magnetic particles within the studied sediments. On the other hand, high values of concentration dependent magnetic parameters χlf, χARM and SIRM as well as SIRM/χ might reflect warm climate. On the contrary, low values of these parameters indicate wet or cool climate.
Climate Change During Holocene Recorded by Magnetic Properties
Generally, climate combinations are warm wet and cold dry at most regions. However, the magnetic results indicated that the climate combinations were warm dry and cold wet in the study area during early and middle Holocene. This decoupling of temperature and precipitation has been reported for the area from south China to the SCS (Yokoyama et al., 2011; Zhang et al., 2015). During 9.16–7.8 cal. ka BP, the concentration dependent magnetic parameters as well as χARM/SIRM and SIRM/χ kept relatively stable (Figure 4), indicating a relatively stable climate (including temperature and precipitation) during this period. The climate fluctuated frequently since 7.8 cal. ka BP. The Holocene climate fluctuations reflected by magnetic properties of PC24 sediments were basically consistent to the results of Shi et al. (1992). However, climate change recorded by magnetic properties of PC24 differed slightly from their results. According to Shi et al. (1992), the period during 8.5–3.0 ka BP was identified as the Holocene Megathermal, the latest Hysithermal, inland of China. However, the magnetic properties of core PC24 sediments indicated that the beginning and duration of the Holocene Megathermal for the study area were different. The values of concentration dependent magnetic parameters increased gradually from 7.5 cal. ka BP. The increasing χfd (%) from 7.5 cal. ka BP indicates climate grows drier. Increasing eolian dust input but low marine authigenesis should explain the highest values of χlf, χARM and SIRM with relatively low value of during 7.35–6.00 cal. ka BP. SIRM/χ reached its peak value during 6.1–3.9 cal. ka BP. Therefore, it seemed that the Holocene Megathermal in the study area of core PC24 was more appropriate during 7.5–3.4 cal. ka BP. This different duration of Holocene Megathermal might be significant for climate response because the same methods (AMS 14C) and low error (less than 100 years) of age determination used by previous research and the present study. This difference indicated that marine response to climate change was slower than inland. The duration 6.1–3.9 cal. ka BP should be identified as the Megathemal Maximum for the study area. The relatively low values of χARM/SIRM during the warmest stage of Holocene reveal a relative wet condition during this period. χlf, χARM, SIRM, and SIRM/χ decreased sharply from 3.4 cal. ka BP, indicating the climate got cool abruptly. Since 2.7 cal. ka BP, χlf, χARM, SIRM, and SIRM/χ increased and χARM/SIRM decreased gradually, indicating the climate became warm and wet.
According to Jin et al. (2007), it should be open to discussion whether there was a synchronous or similar event or not as the worldwide recorded 8.2 ka cooling event in China. However, the results indicated that a similar cold event as 8.2 ka cooling event was also recorded by magnetic properties of core PC24 sediments. From 8.55 to 8.25 cal. ka BP., values of χlf, χARM, SIRM, and SIRM/χ decreased slightly. Value of χfd (%) rose greatly and reached its highest value. These results indicated that the local climate of core PC24 during this stage was manifested as cold dry.
Approximately equal concentration of detrital PSD and biogenic SD magnetite and small part of SP particles were coexisted within the studied core (PC24) sediments. The concentration dependent magnetic parameters are positive corresponding to variation of temperature. Grain size dependent parameters χARM/SIRM and SIRM/χ of the studied core sediments varied reversely. Comparing to the contribution of detrital PSD and biogenic SD magnetite to SIRM, it can be deduced that magnetic parameters χARM/SIRM and SIRM/χ are sensitive to detrital and biogenic magnetite particles, respectively. Variations of χARM/SIRM and SIRM∕χ are corresponding to humidity and temperature, respectively.
The local climate of the study area fluctuated during Holocene. During early and middle Holocene, the climate combinations were warm dry and cold wet. It became warm and wet since 2.7 cal. ka BP. The Holocene Megathermal in the study area recorded by magnetic properties of core PC24 was appropriate during 7.5–3.4 cal. ka BP. The warmest stage of Holocene for the study area should be during 6.1–3.9 cal. ka BP. The cold event at 8 ka was characterized as cold and dry during 8.55–8.25 cal. ka BP.
All authors listed, have made substantial, direct and intellectual contribution to the work, and approved it for publication.
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.
This work was partially supported by the National Science Foundation of China (grant 41272384), the National Basic Research Project (grant 2010CB833405) and a grant from Youth Innovation Promotion Association of the Chinese Academy of Sciences (grant 2012262). The authors thank Luhua Xie for his help during TOC and δ13Corg measurements.
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Keywords: magnetic properties, sensitivity, climate change, Holocene, the northern South China Sea
Citation: Ouyang T, Li M, Zhao X, Zhu Z, Tian C, Qiu Y, Peng X and Hu Q (2016) Sensitivity of Sediment Magnetic Records to Climate Change during Holocene for the Northern South China Sea. Front. Earth Sci. 4:54. doi: 10.3389/feart.2016.00054
Received: 18 December 2015; Accepted: 18 April 2016;
Published: 06 May 2016.
Edited by:Qingsong Liu, Chinese Academy of Sciences, China
Reviewed by:Chuang Xuan, University of Southampton, UK
Xiaoqiang Yang, Sun Yat-Sen University, China
Weiguo Zhang, East China Normal University, China
Copyright © 2016 Ouyang, Li, Zhao, Zhu, Tian, Qiu, Peng and Hu. 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: Tingping Ouyang, email@example.com