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Proceedings of 2 nd International Symposium on Lightning and Storm-Related Phenomena ISL-SRP 2017 – May 10-11, 2017, Aurillac (Cantal, France) www.labofoudre.com GEOMORPHIC AND GEOMAGNETIC PERSPECTIVES ON LIGHTNING STRIKES IN THE LESOTHO HIGHLANDS, SOUTHERN AFRICA Jasper KNIGHT 1 *, Stefan W. GRAB 1 , Susan J. WEBB 2 , Kirsten O’BRIEN 2 , and Nasreen MAYET 1 1 School of Geography, Archaeology and Environmental Studies, University of the Witwatersrand, Private Bag 3, Wits 2050, Johannesburg, South Africa 2 School of Geosciences, University of the Witwatersrand, Private Bag 3, Wits 2050, Johannesburg, South Africa *e-mail address ([email protected]) Abstract Although there has been much work on the atmospheric physics of lightning flashes and on atmospheric and ionospheric physics generally, much less is known of the controls on and interactions between cloud-to-ground lightning strokes and the near-Earth surface, including microclimatology, topography, relief, vegetation, soils and geology. Such information is vital, however, given the high risk posed to people and the environment in areas of high lightning hazard. Here we describe some key geomorphic and geomagnetic impacts of cloud-to-ground lightning strikes on the land surface, based on field evidence from Lesotho, southern Africa, where strike frequency is higher than the global average and where the lightning detection system run by the South African Weather Services allows for relatively accurate spatial and temporal data on strike occurrence. High concentration of strikes in the Maloti-Drakensberg mountains (~3400 m asl) in eastern Lesotho is a result of orographic driven summer thunderstorms. Clear geomorphic evidence exists in this region for the impact of lightning strikes along summit surfaces and around scarp edges, including localized areas of fresh and unweathered basalt bedrock surfaces that are fractured and have produced angular blocky debris. Some of this debris can be found up to 18 m distance from its source location. New magnetometer data from pilot study surveying of summit surfaces in this region show the locations and extent of remanent remagnetization of magnetite within the basalt, which is picked up as a clear geomagnetic anomaly, when compared to induced field background values which reflect the strength and position of Earth’s magnetic field at the time of basalt cooling in the Jurassic. It is notable that the geomagnetic signature imprinted by contemporary lightning strikes can be identified and mapped even if there is no surface geomorphic evidence for a recent strike. This suggests that the geomagnetic signature can exist for a long period (perhaps several centuries or longer) following the strike event, as well as penetrate several metres into bedrock below the ground surface. These are important new areas of lightning research, which have implications for understanding the role of lightning strikes in shaping the land surface, and in lightning hazard risk assessment. Key words: Basalt; Climatology; Mountain geomorphology; Remagnetization; Remanant field Introduction Global satellite datasets show that there is a high incidence of lightning flashes in low latitude areas relative to the global average, with <50 flashes/km 2 /yr -1 recorded in the Congo and Zaire region of central tropical Africa [1] . A major reason for this spatial pattern on a global scale is the generation of both cloud-to-ground and cloud-cloud lightning associated with atmospheric instability and thunderstorms [2] . Within thundercloud convection systems, very rapid air parcel uplift results in adiabatic expansion, cooling, and release of latent heat, which is one of the primary drivers of thundercloud development [3,4] . In central Africa, this thundercloud formation is intimately associated with seasonal migration of the intertropical convergence zone (ITCZ), broadly corresponding to the location of the rising limb of the Hadley cell. In some areas such as the southwest Indian Ocean, lightning flashes within tropical cyclones and storms represent 50–100% of total lightning activity [5] , highlighting the importance of atmospheric instability in determining the macroscale lightning climatology of a region. Lightning imaging sensor data from the Congo basin show highest lightning incidences from October to March, and lowest values from June to August, in association with ITCZ migration [6] . There are also significant diurnal variations in flash density, with highest values recorded in the mid/late afternoon which is related to mesoscale thunderstorm development [6,7] . Terrestrial lightning detection networks in addition to satellite based systems provide data on the locations and timing of lightning flashes at fairly high resolution, but there are relatively few studies that have Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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GEOMORPHIC AND GEOMAGNETIC PERSPECTIVES ON LIGHTNING STRIKES IN THE LESOTHO HIGHLANDS, SOUTHERN

AFRICA

Jasper KNIGHT1*, Stefan W. GRAB1, Susan J. WEBB2, Kirsten O’BRIEN2, and Nasreen MAYET1

1School of Geography, Archaeology and Environmental Studies, University of the Witwatersrand, Private Bag 3, Wits 2050, Johannesburg, South Africa

2School of Geosciences, University of the Witwatersrand, Private Bag 3, Wits 2050, Johannesburg, South Africa *e-mail address ([email protected])

Abstract Although there has been much work on the atmospheric physics of lightning flashes and on atmospheric and ionospheric physics generally, much less is known of the controls on and interactions between cloud-to-ground lightning strokes and the near-Earth surface, including microclimatology, topography, relief, vegetation, soils and geology. Such information is vital, however, given the high risk posed to people and the environment in areas of high lightning hazard. Here we describe some key geomorphic and geomagnetic impacts of cloud-to-ground lightning strikes on the land surface, based on field evidence from Lesotho, southern Africa, where strike frequency is higher than the global average and where the lightning detection system run by the South African Weather Services allows for relatively accurate spatial and temporal data on strike occurrence. High concentration of strikes in the Maloti-Drakensberg mountains (~3400 m asl) in eastern Lesotho is a result of orographic driven summer thunderstorms. Clear geomorphic evidence exists in this region for the impact of lightning strikes along summit surfaces and around scarp edges, including localized areas of fresh and unweathered basalt bedrock surfaces that are fractured and have produced angular blocky debris. Some of this debris can be found up to 18 m distance from its source location. New magnetometer data from pilot study surveying of summit surfaces in this region show the locations and extent of remanent remagnetization of magnetite within the basalt, which is picked up as a clear geomagnetic anomaly, when compared to induced field background values which reflect the strength and position of Earth’s magnetic field at the time of basalt cooling in the Jurassic. It is notable that the geomagnetic signature imprinted by contemporary lightning strikes can be identified and mapped even if there is no surface geomorphic evidence for a recent strike. This suggests that the geomagnetic signature can exist for a long period (perhaps several centuries or longer) following the strike event, as well as penetrate several metres into bedrock below the ground surface. These are important new areas of lightning research, which have implications for understanding the role of lightning strikes in shaping the land surface, and in lightning hazard risk assessment. Key words: Basalt; Climatology; Mountain geomorphology; Remagnetization; Remanant field Introduction Global satellite datasets show that there is a high incidence of lightning flashes in low latitude areas relative to the global average, with <50 flashes/km2/yr-1 recorded in the Congo and Zaire region of central tropical Africa[1]. A major reason for this spatial pattern on a global scale is the generation of both cloud-to-ground and cloud-cloud lightning associated with atmospheric instability and thunderstorms[2]. Within thundercloud convection systems, very rapid air parcel uplift results in adiabatic expansion, cooling, and release of latent heat, which is one of the primary drivers of thundercloud development[3,4]. In central Africa, this thundercloud formation is intimately associated with seasonal migration of the intertropical convergence zone (ITCZ), broadly corresponding to the location of the rising limb of the Hadley cell. In some areas such as the southwest Indian Ocean, lightning flashes within tropical cyclones and storms represent 50–100% of total lightning activity[5], highlighting the importance of atmospheric instability in determining the macroscale lightning climatology of a region. Lightning imaging sensor data from the Congo basin show highest lightning incidences from October to March, and lowest values from June to August, in association with ITCZ migration[6]. There are also significant diurnal variations in flash density, with highest values recorded in the mid/late afternoon which is related to mesoscale thunderstorm development[6,7]. Terrestrial lightning detection networks in addition to satellite based systems provide data on the locations and timing of lightning flashes at fairly high resolution, but there are relatively few studies that have

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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described and analysed these data. For example, the role of land surface topography has most commonly been examined in these studies, by correlating flash density with elevation, relief and aspect derived from digital elevation models (DEMs). In Colombia, Aranguren et al. identify a clear relationship between cloud to ground flash density and elevation, based on high-resolution spatial data[8]. In Colorado, USA, elevations higher than 3200 m and below 1829 m are positively related to flash density, whereas there is no clear pattern between these elevation values, probably due to relief and vegetation[9,10]. In the Drakensberg mountains of southern Africa, data from the South African Weather Services (SAWS) show that the relationship of flash locations to elevational bands varies between adjacent 12 km2 study plots, suggesting that thundercloud origin (by orographic effects, advection across open landscapes or cloud funneling through mountain valleys) is more important than land surface elevation per se[7]. This result is similar to a study in southern Brazil by Bourscheidt et al. which shows that lightning density is significantly related to land surface slope rather than its altitude alone[11]. A drawback in such studies is that terrestrial lightning detection systems, working by triangulation, only give locational accuracies to around 500 m [12], and thus there is uncertainty in the accuracy of such data used for mapping against land surface features[13]. New statistical models, however, are able to better resolve the spatial resolution of cloud-to-ground lightning flashes[14]. In addition to lightning location, there is a significant lack of studies that have examined the role of other land surface properties, such as urban morphology, vegetation, soils and geology, in influencing lightning flash density or properties[15]. Neuwirth et al. note that there are different flash density values between the city of Salzburg and adjacent rural areas of the northern Austrian Alps, and attribute this to electromagnetic induction effects of city buildings[16]. Likewise, Qie et al. note that across plateau areas of China, thunderstorms can have different electrical field properties both spatially and during different phases of thundercloud development[17]. Despite this range of research topics, there is still limited understanding of lightning–land surface interactions, and lightning as a geomorphic agent for example is not considered in land surface models[18]. Suitable locations in which to investigate this topic of lightning–land surface interactions, however, are exposed mountain environments in low latitude areas. The reasons for this are (1) mountains commonly have little to no vegetation and soil, have exposed bedrock outcrops, are of high elevation, and have steep slopes. These properties facilitate rapid orographic uplift of summer weather systems and accompanying convective instability and thundercloud development[19]. Such mountains also have terrain-scale factors such as high roughness that appear to be associated with higher flash densities[20]. (2) Low latitude areas generally have higher flash densities than high latitude areas, and have been previously identified as lightning hotspots[1]. (3) The continental interiors of low latitude areas, such as central regions of Africa, also experience greater seasonal heating of the land surface due to continentality effects, thus resulting summer thunderstorms are of particularly high energy. For these reasons, low latitude mountains are of particular interest with respect to lightning studies. The purpose of this paper is to discuss the signatures that cloud-to-ground lightning strikes have upon exposed land surfaces in low latitude mountains. This is a critically under-researched area, although some recent studies are now highlighting the impacts of high-energy lighting strikes on landscape geomorphology on exposed mountains[18,21]. It is useful to consider such a landscape-scale approach, however, given the relationship of lightning strikes to hazards such as wildfires and electrocution of people and animals, which have significant implications for regional-scale risk analysis[2,22,23]. This paper (i) briefly introduces the study area and methods of field data collection used, (ii) discusses the evidence for geomorphological and geomagnetic impacts upon the land surface in the study area, and informed by other studies globally, and (iii) identifies future research directions for lightning–land surface studies. Study area Although taking a wider overview, this study builds from field evidence for lightning impacts in the Maloti-Drakensberg mountain range of eastern Lesotho, southern Africa (Fig. 1). Topographically, this region has the highest mountain summits in southern Africa, reaching a maximum of 3488 m asl and with several more summits over 3400 m asl. Throughout the region, these summits have mainly flat tops and steep cliffed sides, resulting from the flat disposition of the underlying flood basalts which comprise the regional bedrock[24]. Basalt beds of the Drakensberg Group form part of the wider Karoo Igneous Province[25] and are present across most of Lesotho and into adjacent areas of the KwaZulu-Natal and Eastern Cape provinces in South Africa. These basalt flows, 1.5 km thick in total with beds

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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variably 1–50 m thick, are relatively uniform in mineralogy, have relatively constant thickness throughout the area which is indicative of eruption onto a flat land surface[26]. Some variations in geochemistry between northern and southern Lesotho suggest eruption at the same time but from different volcanic centres. 40Ar/39Ar dating suggest basalt deposition around 177–180 Ma [27]. The uppermost basalt flows (Upper Senqu unit) in the study area around Sani Pass have a typical composition of around 52% SiO2, 15% AlO2, 10% FeO, 10% CaO and 7% MgO [28]. Although several studies have examined bedrock geology and mineralogy(29,30), there is less information regarding the relationship of the basalt flows to the nature of the land surface, including its topography, slope[24,31], soils and ecosystems[32,33]. Mean annual rainfall in the Sani Pass area of eastern Lesotho (2001–5) is 767 mm with pronounced aridity in the winter (May–August). Mean annual temperatures for the same period is 5.8oC [34]. Marginal periglacial environments are observed above ~3000 m asl in the region, with some evidence for a seasonally active layer[35].

Fig. 1. (A) Location of the study area in eastern Lesotho, with areas over 2800 m asl shaded; (B) local view of the Kotisephola summit area. Some previous studies have shown that the Maloti-Drakensberg region experiences high lightning flash intensity (<14 flashes/km2/yr-1)[12,36]. This is considered to be a high level of lightning activity, which can be contextualized by considering that Florida experiences the highest levels of lightning activity in the USA of only 9 flashes/km2/yr-1 [36]. The impacts of lighting on the land surface were investigated from the Kotisephola summit region (3365 m asl) which is located some 10 km NW from Sani Pass in eastern Lesotho (Fig. 1). Methodological approach and methods of data collection and analysis This study draws from several methodological approaches applied to the field study area in eastern Lesotho. This theoretical background is first described in detail, and then followed by a description of how data were collected in the field. (1) Spatial and temporal patterns of cloud-to-ground lightning flashes in the region were examined from SAWS data. The SAWS lightning location system uses 19 sensors located across South Africa that can detect all cloud-to-ground lightning discharges in South Africa, Lesotho and Swaziland (eSwatini)[37]. This system has been operational since February 2006 and can detect lightning strikes with a median of 500 m location accuracy and a 95% efficiency measure[37,38]. For ease, we used subsampled data for the period 1 January 2006–31 December 2011 over the Sani–Kotisephola region. In total, this included a record of >7200 individual strikes. For analysis of their topographic context,

B

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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these data were draped over a DEM derived from ASTER, which is a product of Met1 and NASA and obtained from www.reverb.echo.nasa.gov. (2) Field data on the distribution of lightning impact sites on the Kotisephola summit area were collected by systematic field walking. The positions of the identified features were tagged with a handheld Garmin GPS (locational accuracy ±3 m) and were then integrated into a GIS for further spatial analysis. In total, some 91 impact sites were identified on a geomorphological basis, using three criteria. (i) Visual identification of whether the land surface was affected by lightning, based on whether the rock surface was jagged and angular, rather than smooth or rounded; whether the rock surface had lichen present or not; and whether the rock surface had a grey colouration from the original bedrock or was weathered to a brown colour. (ii) Visual identification and measurement of the debris patterns of blasted rock. Debris composed of jagged rocks with freshly exposed surfaces that was scattered in all directions (even upslope) around the feature was used as evidence that it was produced from lightning impact. (iii) Geomagnetic interference associated with the lightning-induced overprinting of the regional magnetic field, as observed qualitatively with a compass needle. If the needle swayed when placed near to the feature, then magnetic interference caused by lightning was qualitatively confirmed. These field observations were used in combination to evaluate the confidence with which any particular geomorphic feature can be attributed to lightning impact on the land surface[7]. (3) The spatial distribution of potential lightning strikes can be evaluated based on the distribution and intensity of geomagnetic anomalies on the near surface (uppermost few m). Induced magnetism is recorded in the minerals contained within rocks, and this magnetic field broadly corresponds to the Earth’s regional geomagnetic field at the time of mineral formation or deposition[39,40]. The presence of magnetite and other metal-rich minerals within the basalt bedrock of the study area means that this palaeo-geomagnetic induced field is relatively well imaged. The remanent field corresponds to any sources of overprinting of the induced field, and is associated in particular with high-energy lightning strikes on the land surface. Previous work has shown that lightning induced remanent magnetization (LIRM) can be measured clearly within surface rocks[41-43]. The reason for this is that the air surrounding lightning can be heated up to 30 000 K and the ground temperatures can reach 2000 K. These temperatures may rock minerals to be temporarily heated above their Curie point (which, for magnetite, is 580oC)[43], changing both mineral composition and overprinting the palaeo-geomagnetic field with the contemporary field at the time of lightning induction. The ratio between the remanent and induced fields is known as the Königsberger ratio (Q) with high Q values indicative of lightning strike overprinting[44]. This overprinting is readily identifiable because (i) the strength of the remanent field is several orders of magnitude larger than variability in the induced field, and (ii) the remanent field produces ‘hotspots’ that can be clearly identified. The intensity of the magnetic field from lightning decreases as an inverse function of the distance from the lightning bolt[45]. LIRM generates strong magnetic fields in the surface, which have gradients of several tens of nT m-1, and can extend from a few metres up to tens of metres distance. The LIRM is detectable within a few metres of the lightning strike location[44]. The direction of magnetisation of LIRM is not dependent on the earth’s magnetic field at the site, but solely the magnetic field associated with the lightning’s electric field in the ground[45]. The pattern of the electric current once it penetrates the ground is not known, but it has been suggested that the current flows for a short distance vertically and for a longer distance horizontally[44,46]. This theoretical approach was used to identify the locations of potential lightning strikes in the field through geomagnetic surveying across selected sites around the summit of Kotisephola. This was undertaken through closely-spaced grid transects using a magnetometer. The instrumentation used was a G-859 Mining Mag Cs-vapour magnetometer with integrated NovAtel Smart Antenna and GPS, manufactured by Geometrics. Field observations were used to identify the most suitable sites for magnetometer survey, based on geomorphic evidence for lightning strikes. Grid lines at 1 m spacing were surveyed, and measurements were taken every 0.2 s with the magnetometer which was carried as a backpack by an operator. The magnetic and GPS data were downloaded and exported to Geosoft software. GPS data were converted to UTM coordinates. The grid cell size plotted was 0.75 m dimensions. Profile lines were extracted from Geosoft and plotted in Mag2dc. Diurnal correction data from the Hermanus Magnetic Observatory were obtained for the days that the surveys were performed. Results from the preliminary study on summits at Kotisephola, eastern Lesotho, are presented here.

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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Results Regional lightning climatology Climate in terms of synoptic circulation patterns has been considered as a control on lightning patterns. Analysis of SAWS data for a circular region of 2 km diameter focused on the Kotisephola summit region (12.57 km2) for the period 2006–11 shows that this area has a lightning strike density of 12.68 flashes/km2/yr-1 (±1 SD of 7.23). This record can also be differentiated by elevation and time (Fig. 2) showing, first, interannual and seasonal variability in lightning activity in this area and, second, that lightning strikes show a relationship to landscape topography and elevation[7]. Analysis of these data shows that there are complex relationships between the land surface, atmospheric processes and resulting lightning climatology[7]. Orographic uplift enhances convective activity and lightning generation, and thus lightning activity broadly increases with elevation[12].

Fig. 2. Lightning climatology of the Kotisephola summit region, 2006–11 (data from SAWS). (A) Lighting strikes by elevation, (B) aspect, (C) number per year, (D) number per month. Whiskers refer to ±1 SD. Geomorphological evidence Summits in the study area have a thin and discontinuous soil and scrub vegetation cover with weathered basalt bedrock surfaces readily visible. Fresh bedrock surfaces are grey and rough whereas weathered surfaces are oxidised to a brown-red colour and are notably smooth and lichen-covered. These visual properties mean that fresh surfaces are easily identified. In the Kotisophola summit region, Mayet et al. mapped the locations of lightning strike sites, using the three field criteria discussed above[7]. In total, 91 strike locations were identified, of which 54% recorded all three criteria (fresh bedrock surfaces, debris scatters, magnetic imprint) (Fig. 3). Although many of these sites are clustered there are no particular spatial patterns that can be identified, but many sites are located around the margins of the flat summits, at scarp edges. In part this is due to any soil being thinnest in these locations and bedrock surfaces being most common; but it is also due to a higher concentration of Earth’s positive charge being focused at topographic outliers in the landscape[44]. The most significant geomorphological signature of lightning strikes is the formation of broken-up rock surfaces and the related generation of loose, angular debris[18]. Broken-up rock surfaces are identified on the basis of the presence of fresh (grey) rather than weathered (brown) rock surfaces. In area, these fresh surfaces vary from a few cm2 where edges may have been chipped off the sides of rock protrusions, to areas of up to 0.5 m2 where larger slabs of the bedrock surface have been excavated and displaced.

(A) (B)

(C) (D)

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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Fig. 3. Location of lightning strikes (black circles) in the Kotisophola summit region (redrawn after Mayet et al., 2016). Areas above 3300 m asl are shaded; contours derived from ASTER data are at 20 m intervals. Red circles L1–L4 correspond to the positions of magnetometer surveys (Fig. 7). Figure 4 shows examples of lightning impacts on the land surface. The excavation of bedrock slabs generates a rough and fresh rock surface (Fig. 4A). This process also gives rise to the formation of angular, blocky debris, previously interpreted in this region as a result of periglacial frost shattering[18]. The propagation of lightning energy through the rock results in the expansion of pre-existing lines of weakness, and the generation of new fractures. Pre-existing fractures are widened and extend deeper into the rock body. These are important because this increases the instability of the land surface and makes it more likely that subsequent mass movements can take place. Widened fractures also increase the area exposed to subaerial biological and chemical weathering. New fractures can also be formed. These are identified because they have closed, zigzag, angular outlines and cut through or across pre-existing weaknesses in the bedrock (Fig. 4A, B). The direction and nature of fracture propagation is shown in Figure 4C by the presence of plumose grooves emanating outwards from a single point (located near the hammer). Several summits in the study area have been examined for the presence of fractured rock surfaces indicative of lightning impacts. The greatest visual qualitative impacts however are seen near the scarp edge where rock surfaces are likely preconditioned to show fractures. A prominent example is shown in Figure 4D. Here, a large wedge-shaped depression (4 m2) excavated at the top of the scarp face has generated fractured debris. The wedge is up to 6 m high and 2 m wide at its base. A large block (117x96x92 cm, estimated mass 2580 kg) has been displaced and rotated in a downslope direction, whilst other debris has been variously rolled or thrown (mainly) downslope but also on the rock surface immediately surrounding the lightning-strike area (Fig. 4D). The location of the dispersed debris was measured from this wedge source area, plotted in Figure 5. Excluding outliers, there is a weak negative relationship (R² = 0.0091) between block volume and distance travelled from source (n=21), with block volumes of <168 kg mass and distances travelled of <18 m. Some of the largest clasts have travelled the longest distances, similar to patterns observed in avalanche-dominated alluvial fans[47]. At this location, the scarp edge is aligned 070–250o and has an indented morphology, influenced by the orientation of dominant bedrock fracture sets, which are aligned 040–220o and 140–320o. Thus, wedge-shaped failures may have been influenced by bedrock weaknesses.

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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Fig. 4. Examples of lightning strike impacts on the land surface. (A) Fresh, fractured bedrock surface, (B) new fractures and brecciated bedrock fragments, (C) plumose pattern along a fresh bedrock fracture face, (D) displaced large boulder at a position near the summit scarp edge, discussed in the text.

Fig. 5. Plot of the location of lightning-generated debris (black circles), by distance and direction, from source (plot centre). These data refer to the lightning strike site shown in Fig. 4D. Also shown is the orientation of the scarp edge and bedrock fracture sets. Elsewhere around the scarp edge, other wedge-shaped structures are found. A typical example is shown in Figure 6, in which newly excavated rock can be clearly identified by its light, unweathered

A B

C D

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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colour. Knight and Grab list a range of sizes of these rock failures, with displaced rock volumes of <8.45 m3 [18].

Fig. 6. Example of a wedge-shaped rock failure caused by lightning. Displaced rock fragments can be identified. Geomagnetic evidence A pilot survey was conducted at four sites at the Kotisephola summit (locations marked in Fig. 3). Site Lesotho 1 focused on a small area slightly away from the scarp edge and located around one upstanding bedrock protrusion which exhibited a distinctive magnetic disturbance (based on evidence from the compass), even though the bedrock is highly weathered and lichen-covered (Fig. 7A). Site Lesotho 2 is on a relatively flat summit area between the two scarp edges present at the site (Fig. 7B). At both sites, a number of hotspots were identified which correspond to high intensity geomagnetic anomalies. Maximum and minimum values from the surveyed sites are presented in Table 1. At site 1, the difference between highest and lowest values was only 3316 nT, but this was based on measured localities 3 m apart and results in a geomagnetic gradient of 1105 nT m-1 which is much larger than the gradient suggested for a typical lightning strike[48]. Sites 3 and 4 covered a smaller area and were located on the highest summit, approximately 30 m and 25 m above the altitude of site 1, respectively. Here, the land surface is rockier, more weathered, and less easily traversed (Fig. 8). Notable geomagnetic hotspots are also identified (Fig. 7C, D). These sites have a larger range of measured geomagnetic intensities than the lower sites (Table 1), which may reflect higher lightning incidence. Table 1. The minimum and maximum intensities for the surveyed sites and their intensity differences.

Survey site Minimum (nT) Maximum (nT) Difference (nT) Lesotho 1 27197.3 30513.5 3316.2 Lesotho 2 27758.2 29205.5 1447.3 Lesotho 3 19563.2 38946.0 19382.8 Lesotho 4 24496.7 36749.6 12252.9

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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(A)

(B)

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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Fig. 7. Magnetometer survey results for Lesotho sites (A) site 1, (B) site 2, (C) site 3, (D) site 4. Survey lines are shown as the thin black lines. A significant bedrock protrusion affected by lightning at site 1 is shown in the photo.

(C)

(D)

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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Fig. 8. Viewpoint of the highest survey area, on the summit of Kotisephola. (A) The weathered scarp edge, (B) intensely weathered and partly disaggregated surface boulders. Discussion Lightning has potential to affect the land surface in several different ways[49,50]. Most commonly, in the literature, impacts include fulgurite[50,51], forest fires[23,52] and human mortality[53,54]. Lightning is also known to cause bedrock and masonry fractures[18,55,56] but these have not been fully described. This present study shows that lightning can give rise to several different types of signatures identified from field evidence. These can be considered as unambiguous and diagnostic evidence for lightning impacts on the land surface. Lightning and the land surface Cloud-to-ground lightning strikes are associated with high energy release into the surrounding environment upon stroke contact. Currents of lightning strikes have been estimated at 109–1010 J of energy per flash, which is usually discharged as 3–5 strokes over 200–300 ms duration, and with a charge transfer of 20 C [57]. Apart from mineral recrystallization where temperatures exceed the Curie point, any moisture present within the rock, in particular within fractures, would be instantaneously converted to water vapour and the gas would expand rapidly, resulting in in an explosive effect within the rock fracture, forcing the fracture apart and scattering broken rock debris for some distance[18,21,58,59]. This scenario provides a strong theoretical basis for considering how lightning can impact on land surface geomorphology and slope sediment supply. The fact that there is a clear (qualitative) magnetic anomaly when a compass is passed over the site where fresh, angular bedrock surfaces are found confirms unambiguously that their formation is due to lightning and not an alternative mechanism such as frost shattering. Lightning geophysical impacts Several studies have examined the geomagnetic impacts of lightning on near surface rocks[40,42-44,48]. In South Africa, several studies have examined in detail the 3-dimensional distribution of magnetic signatures at the meteorite impact site at Vredefort, where planar rock surfaces have been strongly affected by lightning. At this site, Carpozen et al. show that remanent magnetization at depth within 10 m-long boreholes is due to impact remagnetization, whereas higher in the profile, magnetization is more confidently due to lightning[48]. Strength of the LIRM decreases with depth – it is strongest in the upper 2 m but still recognizable to 8 m depth. Further, they found that the total field intensity and declination varies spatially, thus that the signature of lightning overprinting of the remanent field is not spatially consistent and that its depth also varies spatially. Building from this, Salminen et al. showed that at Vredefort there is evidence that magnetite grains present in the parent rock were oxidized to maghemite, but that this was dependent on lightning energy and thus the degree of rock heating[43]. It is very likely that such changes also exist in minerals within the basalt bedrock at Kotisephola, although this is yet to be tested. What is still unclear is the extent to which multiple, repeated lightning strikes in the same region have an overprinting effect on the signatures of older strikes; whether the geomagnetic signal of a strike decreases over time and thus its longevity as a signal in the rocks; or whether the surface geomagnetic signal decreases over time as a consequence of subaerial weathering. For example, weathering rates in the Drakensberg highlands (which include the Kotisephola area) are estimated to be 6 m/Ma based on 36Cl dating[60], thus 2 m depth could be

(A) (B)

Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa

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Proceedings of 2nd International Symposium on Lightning and Storm-Related Phenomena ISL-SRP 2017 – May 10-11, 2017, Aurillac (Cantal, France)

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uncovered in 330 000 years. (This excludes any potential excavation of the rock surface by lightning or other processes.) Thus, there is a potentially long time period over which lightning signatures may exist in the landscape. Verrier and Rochette showed that different lightning strokes can have different intensities (in kA) [42], which may then suggest that larger strikes penetrate deeper and give rise to bigger geomagnetic anomalies than weaker strikes. Although this is a logical deduction, this is still an untested hypothesis. Conclusions and future research directions In the Lesotho highlands region, several independent lines of evidence exist for the role of lightning strikes in shaping land surface geomorphology and its geomagnetic properties. Fresh and unweathered bedrock surfaces that show fresh fractures, angular faces and where angular debris has been excavated reflect the explosive impacts of lightning on the land surface, generating new rock fractures and producing loose debris. It is notable that some of this debris is found <18 m distance from its source location. Data from magnetometer surveys across lightning-affected summit areas show the extent of mineral remagnetization. This is identified as a geomagnetic anomaly, in which the remanent field is overprinted on the background induced field. It is notable that the geomagnetic signature by contemporary lightning strikes can be identified and mapped even if there is no surface geomorphic evidence for a recent strike, which suggests that these geomagnetic signatures can be present in the landscape for a long time (centuries to millennia?), although there is little research on this topic. Lightning–land surface studies represent an important research theme[49] because of (i) the importance of lightning as a source of hazard risk in many parts of the world[54], and (ii) potential implications for changing hazard risk as a result of human modification of the land surface through urbanization, geoengineering, and the effects of climate change[22]. The latter is already suggested through climate models to increase lightning hazard risk in the USA by 12±5% per 1oC of global warming[61]. These represent important future research directions. References [1] H.J. Christian, R.J. Blakeslee, D.J. Boccippio, W.L. Boeck, D.E. Buechler, K.T. Driscoll, S.J. Goodman, J.M. Hall, W.J. Koshak, D.M. Mach, M.F. Stewart, J. Geophys. Res. Atmos. 2003, 108, D1, 4005, doi:10.1029/2002JD002347. [2] C.G. Price, Surv. Geophys. 2013, 34, 755–767. [3] E.E. Ávila, R.E. Bürgesser, N.E. Castellano, A.B. Collier, R.H. Compagnucci, A.R.W. Hughes, J. Atmos. Solar-Terr. Phys. 2010, 72, 1114–1121. [4] S.R. Sharma, V. Cooray, M. Fernando, J. Atmos. Solar-Terr. Phys. 2011, 73, 483–487. [5] C. Bovalo, C. Barthe, N. Bègue, Nat. Haz. Earth Syst. Sci. 2012, 12, 2659–2670. [6] S. Soula, J.K. Kasereka, J.F. Georgis, C. Barthe, Atmos. Res. 2016, 178–179, 304–319. [7] N. Mayet, J. Knight, S.W. Grab, S. Afr. Geogr. J. 2016, 98, 321–336. [8] D. Aranguren, J. López, J. Inampués, H. Torres, H. Betz, J. Atmos. Solar-Terr. Phys. 2017, 154, 182–189. [9] B.J. Vogt, S.J. Hodanish, Monthly Weather Rev. 2014, 142, 2353–2360. [10] B.J. Vogt, S.J. Hodanish, Appl. Geogr. 2016, 75, 93–103. [11] V. Bourscheidt, O. Pinto Junior, K.P. Naccarato, I.R.C.A. Pinto, Atmos. Res. 2009, 91, 508–513. [12] M. Gijben, S. Afr. J. Sci. 2012, 108, Article 740, doi:10.4102/sajs.v108i3/4.740. [13] U. Sonnadara, V. Kathriarachchi, V. Cooray, R. Montano, T. Götschl, J. Atmos. Solar-Terr. Phys. 2014, 112, 31–37. [14] T.R. Etherington, G.L.W. Perry, Comp. Geosci. 2017, 98, 38–45. [15] R. Vishnu, S. Murali Das, S. Sampath, G. Mohan Kumar, J. Lightning Res. 2010, 2, 12–24. [16] C. Neuwirth, W. Spitzer, T. Prinz, J. Lightning Res. 2012, 4, 166–172. [17] X. Qie, T. Zhang, G. Zhang, T. Zhang, X. Kong, Atmos. Res. 2009, 91, 244–249. [18] J. Knight, S.W. Grab, Geomorphol. 2014, 204, 61–70. [19] C.B. Schaaf, J. Wurman, R.M. Banta, Bull. Am. Met. Soc. 1988, 69, 272–277. [20] K.L. Cummins, 31st Int. Conf. Lightning Protection (ICLP), 2012, Vienna, Austria, 9pp. [21] J. Knight, Geol. Today 2007, 23, 11–12. [22] D.G. Woolford, C.B. Dean, D.L. Martell, J. Cao, B.M. Wotton, Environmetrics 2014, 25, 406–416. [23] S. Veraverbeke, B.M. Rogers, M.L. Goulden, R.R. Jandt, C.E. Miller, E.B. Wiggins, J.T. Randerson, Nature Clim. Change, 2017, 7, 529–534. [24] B.P. Moon, M.J. Selby, Geogr. Ann. 1983, 65A, 135–145. [25] A.R. Duncan, J.S. Marsh, in The Geology of South Africa, 2006, M.R. Johnson, C.R. Anhaeusser, R.J. Thomas (Eds), 501–520. [26] F.G. Bell, D.R. Haskins, Eng. Geol. 1997, 175–198. [27] R.A. Duncan, P.R. Hooper, J. Rehacek, J.S. Marsh, A.R. Duncan, J. Geophys. Res. 1997, 102, 18127–18138.

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Geomorphic and geomagnetic perspectives on lightning strikes in the Lesotho Highlands, Southern Africa