Abstract:S U M M A R YStudy of the magnetostratigraphy of the earliest Jurassic (mainly Hettangian) section of Langmoos near Adnet in Austria (Northern calcareous Alps) provides a sequence of 10 magnetic polarity intervals. These intervals are often evident in the natural remanent magnetization. However, rather than a true magnetostratigraphic sequence, palaeomagnetic analyses reveal evidence for successive phases of magnetization within the section. Evidence includes (1) changes in lithology associated with changes in… Show more
“…2. In most cases (about 80%) and before any tectonic correction, J3 and J2 components display NE‐E declinations and positive inclinations (Figures 4a and 5 and Table 2), in agreement with previous data [ Mauritsch and Frisch , 1978; Channell et al , 1990, 1992; Heer , 1982; Gallet et al , 1993].…”
Section: Resultssupporting
confidence: 91%
“…Most part of the data set belongs to the former Stauffen‐Höllengebirge and Berchtesgaden nappes (lower and upper Tirolic units, respectively, in the new classification by Frisch and Gawlick [2003]) and part to the Göll‐Lammer unit [ Tollmann , 1973, 1985, 1987; Plöchinger , 1995], redefined as Juvavic‐Hallstatt Mélange [ Frisch and Gawlick , 2003]. Previous paleomagnetic data were mostly obtained in the north central part of the NCA [ Mauritsch and Frisch , 1978; Smathers , 1987; Channell et al , 1992; Heer , 1982; Gallet et al , 1993], mainly in the Liassic formations because of their well‐know magnetic signal (Table 1 and Figure 2); primary components of magnetization, which are characterized by dual polarities and carried by hematite were identified. Secondary directions were only poorly described or ignored.…”
Section: Geological Settingmentioning
confidence: 99%
“… First column is number of site on Figure 1; Site, name of the original site; Ref, references (M&F, Mauritsch and Frisch [1978]; Ch, Channell et al [1992], Heer [1982], and Gall, Gallet et al [1993]); Long, longitude; Lat, latitude; Locality, geographic names; Strike (right‐hand rule), dip; DD, dip direction; Obs, samples or sites; n/N, number of samples considered/number of samples analyzed; D, I, declination and inclination of the paleomagnetic vector (BAC, before any correction (in situ); ABC, after bedding correction); question marks indicate nonsense results; Pol, polarity; α 95 , K, Fisher [1953] statistical parameters. …”
Section: Geological Settingmentioning
confidence: 99%
“…The northern Calcareous Alps (NCA) belong to the upper Austroalpine megaunit (AU) of the Eastern Alps and represent one of the largest tectonostratigraphic units of the Alps. The application of paleomagnetism in this part of the orogen started very early [ Hargraves and Fischer , 1959], and continues until today [ Soffel , 1975; Mauritsch and Frisch , 1978, 1980; Heer , 1982; Becke and Mauritsch , 1985; Soffel and Wohl , 1986; Mauritsch and Becke , 1987; Channell et al , 1990, 1992; Channell and Stoner , 1994; Gallet et al , 1993, 1994, 1996, 1998; Haubold et al , 1999; Thöny et al , 2006]. These studies had different goals, such as the reconstruction of the nappe system evolution (characterization of rotations) or the platform configuration of this margin of the Tethys Ocean (Triassic and Jurassic magnetostratigraphy and paleogeographical reconstructions).…”
Section: Introductionmentioning
confidence: 99%
“…To shed some light on these problems, the central part of the NCA (south of Salzburg) has been examined in detail by studying 77 new sites and four magnetostratigraphic profiles. Previous data in the area (45 sites from Mauritsch and Frisch [1978], Heer [1982], Becke and Mauritsch [1985], Mauritsch and Becke [1987], Channell et al [1990, 1992], and Gallet et al [1993]) were also included in the interpretation.…”
[1] We present 81 paleomagnetic sites (Early Triassic to Early Cretaceous) from the central sector of the northern Calcareous Alps (NCA, Eastern Alps, Austria and Germany). Stepwise thermal demagnetization defines three magnetic directions mostly carried by low unblocking temperature and low-coercivity minerals: J3, 350°; J2, 500°; J1, 575°and 680°. J3 and J2 show positive inclinations, whereas J1 (very seldom) is of dual polarity. The fold tests show that a J3 can be interpreted as a postfolding and posttilting remagnetization and J2 as a postfolding and pre(syn)tilting. J1 can be considered as primary because of the occurrence of two polarities and evidence presented by other authors in the area. All three components show a systematic and significant clockwise rotation after comparing with the expected European references. J2 or J1 are marked by higher rotation values than J3. J2 shows different inclinations depending on the structural position (north or southward dips). Considering the structural evolution and the observed inclinations, the first postfolding and pretilting remagnetization event (J2) could have taken place between Late Cretaceous and Eocene times but certainly before the thrusting of the NCA over the Rhenodanubian Flysch and northward tilting caused by the stacking of the lower Austroalpine nappes. The second postfolding and posttilting remagnetization (J3) would have been acquired after the final thrusting of the NCA over Penninic units. From then, the NCA behaved as a set of rigid blocks recording the main stage of vertical axis clockwise rotation (65°in average) associated with the continental collision. The variable degree of rotation in the different positions (from 40°to 134°) can be explained by individual vertical axis rotation in a block system trying to adjust to space problems. The constant declination differences between J2 and J3 (25°in average) would reflect the rotation related with the lateral differences of shortening during the oblique thrust of the Austroalpine units over the Penninic units.
“…2. In most cases (about 80%) and before any tectonic correction, J3 and J2 components display NE‐E declinations and positive inclinations (Figures 4a and 5 and Table 2), in agreement with previous data [ Mauritsch and Frisch , 1978; Channell et al , 1990, 1992; Heer , 1982; Gallet et al , 1993].…”
Section: Resultssupporting
confidence: 91%
“…Most part of the data set belongs to the former Stauffen‐Höllengebirge and Berchtesgaden nappes (lower and upper Tirolic units, respectively, in the new classification by Frisch and Gawlick [2003]) and part to the Göll‐Lammer unit [ Tollmann , 1973, 1985, 1987; Plöchinger , 1995], redefined as Juvavic‐Hallstatt Mélange [ Frisch and Gawlick , 2003]. Previous paleomagnetic data were mostly obtained in the north central part of the NCA [ Mauritsch and Frisch , 1978; Smathers , 1987; Channell et al , 1992; Heer , 1982; Gallet et al , 1993], mainly in the Liassic formations because of their well‐know magnetic signal (Table 1 and Figure 2); primary components of magnetization, which are characterized by dual polarities and carried by hematite were identified. Secondary directions were only poorly described or ignored.…”
Section: Geological Settingmentioning
confidence: 99%
“… First column is number of site on Figure 1; Site, name of the original site; Ref, references (M&F, Mauritsch and Frisch [1978]; Ch, Channell et al [1992], Heer [1982], and Gall, Gallet et al [1993]); Long, longitude; Lat, latitude; Locality, geographic names; Strike (right‐hand rule), dip; DD, dip direction; Obs, samples or sites; n/N, number of samples considered/number of samples analyzed; D, I, declination and inclination of the paleomagnetic vector (BAC, before any correction (in situ); ABC, after bedding correction); question marks indicate nonsense results; Pol, polarity; α 95 , K, Fisher [1953] statistical parameters. …”
Section: Geological Settingmentioning
confidence: 99%
“…The northern Calcareous Alps (NCA) belong to the upper Austroalpine megaunit (AU) of the Eastern Alps and represent one of the largest tectonostratigraphic units of the Alps. The application of paleomagnetism in this part of the orogen started very early [ Hargraves and Fischer , 1959], and continues until today [ Soffel , 1975; Mauritsch and Frisch , 1978, 1980; Heer , 1982; Becke and Mauritsch , 1985; Soffel and Wohl , 1986; Mauritsch and Becke , 1987; Channell et al , 1990, 1992; Channell and Stoner , 1994; Gallet et al , 1993, 1994, 1996, 1998; Haubold et al , 1999; Thöny et al , 2006]. These studies had different goals, such as the reconstruction of the nappe system evolution (characterization of rotations) or the platform configuration of this margin of the Tethys Ocean (Triassic and Jurassic magnetostratigraphy and paleogeographical reconstructions).…”
Section: Introductionmentioning
confidence: 99%
“…To shed some light on these problems, the central part of the NCA (south of Salzburg) has been examined in detail by studying 77 new sites and four magnetostratigraphic profiles. Previous data in the area (45 sites from Mauritsch and Frisch [1978], Heer [1982], Becke and Mauritsch [1985], Mauritsch and Becke [1987], Channell et al [1990, 1992], and Gallet et al [1993]) were also included in the interpretation.…”
[1] We present 81 paleomagnetic sites (Early Triassic to Early Cretaceous) from the central sector of the northern Calcareous Alps (NCA, Eastern Alps, Austria and Germany). Stepwise thermal demagnetization defines three magnetic directions mostly carried by low unblocking temperature and low-coercivity minerals: J3, 350°; J2, 500°; J1, 575°and 680°. J3 and J2 show positive inclinations, whereas J1 (very seldom) is of dual polarity. The fold tests show that a J3 can be interpreted as a postfolding and posttilting remagnetization and J2 as a postfolding and pre(syn)tilting. J1 can be considered as primary because of the occurrence of two polarities and evidence presented by other authors in the area. All three components show a systematic and significant clockwise rotation after comparing with the expected European references. J2 or J1 are marked by higher rotation values than J3. J2 shows different inclinations depending on the structural position (north or southward dips). Considering the structural evolution and the observed inclinations, the first postfolding and pretilting remagnetization event (J2) could have taken place between Late Cretaceous and Eocene times but certainly before the thrusting of the NCA over the Rhenodanubian Flysch and northward tilting caused by the stacking of the lower Austroalpine nappes. The second postfolding and posttilting remagnetization (J3) would have been acquired after the final thrusting of the NCA over Penninic units. From then, the NCA behaved as a set of rigid blocks recording the main stage of vertical axis clockwise rotation (65°in average) associated with the continental collision. The variable degree of rotation in the different positions (from 40°to 134°) can be explained by individual vertical axis rotation in a block system trying to adjust to space problems. The constant declination differences between J2 and J3 (25°in average) would reflect the rotation related with the lateral differences of shortening during the oblique thrust of the Austroalpine units over the Penninic units.
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