45 resultados para PELARGONIUM HORTORUM


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En la actualidad la mayoría de plantas sufren pérdidas debido a las enfermedades que les provocan los hongos. Uno de estos grupos amenazado por el ataque de los hongos son las especies de la familia Orchidaceae, especies que se encuentran amenazadas y con numerosas especies en peligro de extinción. Uno de los problemas sanitarios más destacados es Botrytis cinerea, hongo patógeno cosmopolita, causante de enfermedades importantes en muchas plantas tales como frutas, verduras, accesiones de viveros, plantas ornamentales y huertos cultivos (Jarvis 1977; Elad et al., 2007). Este género es uno de los grupos de hongos más ampliamente conocido y distribuido. Contiene 22 especies (Hennebert 1973; Yohalem et al., 2003) y un híbrido (B. allii) (Yohalem & Alabama, 2003) vinculado a las etapas sexuales y un amplio número de huéspedes específicos (Beever y Weds, 2000); infecta más de 200 especies vegetales distintas (Williamson et al., 2007). Dada la importancia de este patógeno se realiza un estudio de caracterización morfológica y molecular del hongo, aislado de plantas de orquídeas cultivadas en condiciones de invernadero, de hortalizas y plantas frutales, con síntomas de necrosis, atizonamientos y pudriciones. El análisis de las características morfológicas (presencia de esclerocios, tamaño de conidios, presencia de estructuras sexuales in vitro) y fenotípicas (crecimiento micelial a diferentes temperaturas, germinación de esporas), nos permitió determinar características importantes del comportamiento del hongo y establecer cuáles son las mejores condiciones para su patogenicidad. Se afianzo este trabajo con estudios moleculares a través del análisis de la región ribosomal ITS1-ITS4. Entre los aislados estudiados se identificaron dos especies diferentes, Botrytis cinerea y B. fabiopsis, esta última conocida como especifica de Vicia faba, se lo aisló de una planta de Pelargonium sp. Se hizo un análisis filogenético para comparar estas dos especies, encontrándose que B. fabiopsis está estrechamente relacionada con B. cinerea y B. elliptica, pero lejanamente relacionado con B. fabae. Además, se analizó las poblaciones de los aislados de Botrytis, para ello se seleccionaron tres parejas de cebadores microsatelites con altos porcentajes de polimorfismo. Al analizar la similaridad entre los aislados se determinaron tres grupos de poblaciones de B. cinerea entre los cuales Botrytis fabiopsis comparte un grupo grande con B. cinerea. La diferenciación genética no fue significativa entre la población de aislados de orquídeas y hortalizas, la diferencia génica que fue muy baja, lo que sugiere que la especificidad de Botrytis no está dada por los hospederos, aunque la posibilidad de la especificidad con algún cultivo no puede descartarse. ABSTRACT Most plants suffer diseases caused by fungi. Orchidaceae is one of the threatened groups with many endangered species. Included into the most important problems in plant health is Botrytis cinerea, a cosmopolitan pathogen which causes major diseases in many plants of agronomic interest such as fruits, vegetables, planthouses accessions and ornamental plants (Jarvis, 1977; Elad et al, 2007). The genus Botrytis is one of the most widely and disseminated fungi. The genus contains 22 species (Hennebert 1973; Yohalem et al, 2003) and a hybrid (B. allii) (Yohalem & Alabama, 2003) linked to the sexual stages of a large number of specific hosts (Beever & Weds, 2000); infects over 200 different plant species (Williamson et al., 2007). Due to the importance of this pathogen, a study of morphological and molecular characterization of the fungus was carried out. Fungi samples were isolated from orchid plants grown in greenhouse conditions, vegetables and fruits with signs of necrosis, blight and rottening. To establish the best conditions for pathogenicity, behavioral characteristics of the fungus were studied through the analysis of morphological characteristics (presence of sclerotia, conidia size, sexual structures in vitro) and mycelial growth at different temperatures. To complete the characterization of the fungi, a molecular study was performed via the analysis of ribosomal ITS1-ITS4 region. Two different species were identified: Botrytis cinerea and Botrytis fabiopsis (known by specificity to Vicia faba). B. fabiopsis was isolated from a plant of the genus Pelargonium. A phylogenetic analysis was carried out to compare these two species leading to the conclusion that B. fabiopsis is closely related to B. cinerea and B. elliptica, but distantly related to B. fabae. The populations of Botrytis isolates were also analyzed. Three pairs of microsatellite primers with high percentages of polymorphism were selected. A similarity analysis showed three groups of populations of B. cinerea, including Botrytis fabiopsis. The genetic differentiation was not significant among the populations of isolates from orchids and vegetables; genetic differences were very low, suggesting that the specificity of Botrytis species is not given by the hosts.

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The present-day condition of bipolar glaciation characterized by rapid and large climate fluctuations began at the end of the Pliocene with the intensification of the Northern Hemisphere continental glaciations. The global cooling steps of the late Pliocene have been documented in numerous studies of Ocean Drilling Program (ODP) sites from the Northern Hemisphere. However, the interactions between oceans and between land and ocean during these cooling steps are poorly known. In particular, data from the Southern Hemisphere are lacking. Therefore I investigated the pollen of ODP Site 1082 in the southeast Atlantic Ocean in order to obtain a high-resolution record of vegetation change in Namibia between 3.4 and 1.8 Ma. Four phases of vegetation development are inferred that are connected to global climate change. (1) Before 3 Ma, extensive, rather open grass-rich savannahs with mopane trees existed in Namibia, but the extension of desert and semidesert vegetation was still restricted. (2) Increase of winter rainfall dependent Renosterveld-like vegetation occurred between 3.1 and 2.2 Ma connected to strong advection of polar waters along the Namibian coast and a northward shift of the Polar Front Zone in the Southern Ocean. (3) Climatically induced fluctuations became stronger between 2.7 and 2.2 Ma and semiarid areas extended during glacial periods probably as the result of an increased pole-equator thermal gradient and consequently globally enhanced atmospheric circulation. (4) Aridification and climatic variability further increased after 2.2 Ma, when the Polar Front Zone migrated southward and the influence of Atlantic moisture brought by the westerlies to southern Africa declined. It is concluded that the positions of the frontal systems in the Southern Ocean which determine the locations of the high-pressure cells over the South Atlantic and the southern Indian Ocean have a strong influence on the climate of southern Africa in contrast to the climate of northwest and central Africa, which is dominated by the Saharan low-pressure cell.

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To address the connection between tropical African vegetation development and high-latitude climate change we present a high-resolution pollen record from ODP Site 1078 (off Angola) covering the period 50-10 ka BP. Although several tropical African vegetation and climate reconstructions indicate an impact of Heinrich Stadials (HSs) in Southern Hemisphere Africa, our vegetation record shows no response. Model simulations conducted with an Earth System Model of Intermediate Complexity including a dynamical vegetation component provide one possible explanation. Because both precipitation and evaporation increased during HSs and their effects nearly cancelled each other, there was a negligible change in moisture supply. Consequently, the resulting climatic response to HSs might have been too weak to noticeably affect the vegetation composition in the study area. Our results also show that the response to HSs in southern tropical Africa neither equals nor mirrors the response to abrupt climate change in northern Africa.

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Glacial-interglacial fluctuations in the vegetation of South Africa might elucidate the climate system at the edge of the tropics between the Indian and Atlantic Oceans. However, vegetation records covering a full glacial cycle have only been published from the eastern South Atlantic. We present a pollen record of the marine core MD96-2048 retrieved by the Marion Dufresne from the Indian Ocean ~120 km south of the Limpopo River mouth. The sedimentation at the site is slow and continuous. The upper 6 m (spanning the past 342 Ka) have been analysed for pollen and spores at millennial resolution. The terrestrial pollen assemblages indicate that during interglacials, the vegetation of eastern South Africa and southern Mozambique largely consisted of evergreen and deciduous forests. During glacials open mountainous scrubland dominated. Montane forest with Podocarpus extended during humid periods was favoured by strong local insolation. Correlation with the sea surface temperature record of the same core indicates that the extension of mountainous scrubland primarily depends on sea surface temperatures of the Agulhas Current. Our record corroborates terrestrial evidence of the extension of open mountainous scrubland (including fynbos-like species of the high-altitude Grassland biome) for the last glacial as well as for other glacial periods of the past 300 Ka.

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Influx of aeolian pollen trapped in marine sediments off Namibia provides a wind variation record for the last 135 kyr. The influx of major pollen components is derived from the southwest African desert/semi-desert zone and shows six periods during which enhanced southeast trade winds contributed to strong upwelling and reduced sea surface temperatures. The most prominent of these occurred during 17-23 cal. kyr, 42-56 kyr and before 130 kyr B.P. Correspondence between the pollen influx record and the Vostok deuterium isotope record suggests that pronounced glacial Antarctic cooling was accompanied by intensification of the southeast trades throughout the Late Quaternary. However, during 42-23 kyr B.P. the combination of strong Antarctic glaciation with a decrease of wind zonality induced by low latitude precessional insolation changes caused strong alongshore winds and Ekman pumping that resulted in strong upwelling and reduced sea surface temperatures without pollen influx enhancement.

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To better understand Holocene vegetation and hydrological changes in South Africa, we analyzed pollen and microcharcoal records of two marine sites GeoB8331 and GeoB8323 from the Namaqualand mudbelt offshore the west coast of South Africa covering the last 9900 and 2200 years, respectively. Our data corroborate findings from literature that climate developments apparently contrast between the summer rainfall zone (SRZ) and winter rainfall zone (WRZ) over the last 9900 years, especially during the early and middle Holocene. During the early Holocene (9900-7800 cal.yr BP), a minimum of grass pollen suggests low summer rainfall in the SRZ, and the initial presence of Renosterveld vegetation indicates relatively wet conditions in the WRZ. Towards the middle Holocene (7800-2400 cal. yr BP), a rather moist savanna/grassland rich in grasses suggests higher summer rainfall in the SRZ resulting from increased austral summer insolation and a decline of fynbos vegetation accompanied by an increasing Succulent Karoo vegetation in the WRZ possibly suggests a southward shift of the Southern Hemisphere westerlies. During the last 2200 years, a trend towards higher aridity was observed for the SRZ, while the climate in the WRZ remained relatively stable. The Little Ice Age (ca. 700-200 cal. yr BP) was rather cool in both rainfall zones and drier in the SRZ while wetter in the WRZ.

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A high resolution marine pollen record from site GeoB1023, west of the northern Namib desert provides data on vegetation and climate change for the last 21 ka at an average resolution of 185 y. Pollen and spores are mainly delivered to the site by the Cunene river and by surface and mid-tropospheric wind systems. The main pollen source areas are located between 13°S and 21°S, which includes the northern Namib desert and semi-desert, the Angola-northern Namibian highland, and the north-western Kalahari. The pollen spectra reflect environmental changes in the region. The last glacial maximum (LGM) was characterised by colder and more arid conditions than at present, when a vegetation with temperate elements such as Asteroideae, Ericaceae, and Restionaceae grew north of 21°S. At 17.5 ka cal. B.P., an amelioration both in temperature and humidity terminated the LGM but, in the northern Kalahari, mean annual rainfall in the interval 17.5-14.4 ka cal. B.P. was probably 100-150 mm lower than at present (400-500 mm/y). The Late-glacial to early Holocene transition includes two arid periods, i.e. 14.4-12.5 and 10.9-9.3 ka cal. B.P. The last part of the former period may be correlated with the Younger Dryas. The warmest and most humid period in the Holocene occurred between 6.3 and 4.8 ka cal. B.P. During the last 2000 years, human impact, as reflected by indications of deforestation, enhanced burning and overgrazing, progressively intensified.