Jökull


Jökull - 01.06.2000, Qupperneq 53

Jökull - 01.06.2000, Qupperneq 53
Geirfinnur Jónsson and Leó Kristjánsson -580000 -570000 -560000 -550000 -540000 -530000 330000 340000 350000 360000 370000 -2000 nT -1000 nT 0 nT 1000 nT 2000 nT Figure 3. A contour map of the magnetic field over Mýrdalsjökull, based on results shown in Figure 2. Contour interval is 200 nT. Because of the wide spacing of lines the original data should always be kept in mind when inspecting this map and the following figure. Dotted line: topographic caldera cf. Figure 1. Coordinates: -x,y values of the Hjörsey-datum conical projection for Iceland, in meters. – Jafnsviðslínukort af segulfrávikinu á 2. mynd. Bil milli fluglína er mun meira en bil milli punkta eftir fluglínunni og verður því að skoða þessa mynd og þá næstu með það í huga. hy is reduced down to a common depth, in this case 1000 m below sea level. Individual columns are 200 m square and the working area is 251 x 251 poles, i.e. 50 x 50 km, which matches Figures 2-4. The magnetic field is calculated at a flight altitude of 2100 m us- ing an overall remanence intensity (Jrem) of 8 A/m, which is an estimate for Quaternary volcanics in Ice- land (Kristjánsson, 1970). Figure 5 shows the vertical component of the modelled field as a shaded reli- ef. Qualitatively its resemblance to Figure 4 is clear indicating that the topographic caldera is at least in part the cause of the magnetic bowl. Two perpendicular cross-sections over the magne- tic bowl are shown in Figure 6 along with the calcula- ted field due to the terrain. We generate a model incorporating a vertical cylindrical structure of elliptic cross-section, elongated SE-NW beneath the caldera. For best fit to the observations, the model was set to 52 JÖKULL No. 49
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