In the present study a non-motion-stabilized scanning Doppler lidar was operated on board of RV Polarstern in the Arctic (June 2014) and Antarctic (December 2015– January 2016). This is the first time that such a system measured on an icebreaker in the Antarctic. A method for a motion correction of the data in the post-processing is presented.
The wind calculation is based on vertical azimuth display (VAD) scans with eight directions that pass a quality control. Additionally a method for an empirical signal-tonoise ratio (SNR) threshold is presented, which can be calculated for individual measurement set-ups. Lidar wind profiles are compared to total of about 120 radiosonde profiles and also to wind measurements of the ship.
The performance of the lidar measurements in comparison with radio soundings generally shows small root mean square deviation (bias) for wind speed of around 1ms-1(0.1ms-1) and for wind direction of around 10 (1). The post-processing of the non-motion-stabilized data shows comparably high quality to studies with motion-stabilized systems.
Two case studies show that a flexible change in SNR threshold can be beneficial for special situations. Further the studies reveal that short-lived low-level jets in the atmospheric boundary layer can be captured by lidar measurements with a high temporal resolution in contrast to routine radio soundings. The present study shows that a non-motionstabilized Doppler lidar can be operated successfully on an
icebreaker. It presents a processing chain including quality control tests and error quantification, which is useful for further measurement campaigns.
Die polare Kryosphäre stellt einen Schlüsselfaktor für die Erforschung des Klimawandels dar. Insbesondere das Meereis und seine Schneebedeckung, die sich durch eine äußerst hohe und Zeitskalen-übergreifende Sensitivität gegenüber atmosphärischen Einflüssen auszeichnen, können als diagnostische Parameter für die Abschätzung von Veränderungen im Klimasystem herangezogen werden. Die komplexen Rückkopplungsmechanismen, durch die das Meereis mit der globalen Zirkulation der Atmosphäre und des Ozeans in Wechselwirkung steht, werden durch eine zusätzliche Schneeauflage deutlich verstärkt. Insofern tragen die saisonalen Veränderungen der physikalischen Eigenschaften des Schnees, und insbesondere der Beginn der Schneeschmelze, massgeblich zur lokalen und regionalen Energiebilanz sowie zur Meereismassenbilanz bei. In dieser Arbeit wird nun erstmals auf der Basis langjähriger Daten der satellitengestützten Mikrowellenfernerkundung, in Kombination mit Feldmessungen aus dem Weddellmeer während des Sommers 2004/2005, die Charakteristik der sommerlichen Schmelzperiode auf antarktischem Meereis untersucht. Die sommertypischen Prozesse zeichnen sich hier durch deutliche Unterschiede im Vergleich zu arktischem Meereis aus. Wie die Messungen vor Ort zeigen, kommt es während des antarktischen Sommers nicht zu einem kompletten Abschmelzen des Schnees. Vielmehr dominieren ausgeprägte Schmelz-Gefrier-Zyklen im Tagesgang, die eine Abrundung und Vergrösserung der Schneekristalle sowie die Bildung interner Eisschichten verursachen. Dies führt radiometrisch zu Mikrowellensignalen, deren Erfassung im Vergleich zu bestehenden Schmelzerkennungs-Methoden neue Ansätze erfordert. Durch den Vergleich von zeitlich hoch aufgelösten in-situ Messungen der physikalischen Schneeeigenschaften mit parallel dazu erfassten Satellitendaten, sowie durch eine Modellierung der mikrowellenradiometrischen Eigenschaften der Schneeauflage, konnte ein neuer Indikator entwickelt werden, über den das Einsetzen der typischen sommerlichen Schmelzperiode auf antarktischem Meereis identifiziert werden kann. Der DTBA-Indikator beschreibt die Tagesschwankung der radiometrischen Eigenschaften des Schnees und zeichnet sich durch ein Werteverhalten aus, das eine eindeutige Hervorhebung der Sommerphase innerhalb eines saisonalen Zyklus erkennen lässt. Der Indikator wurde verwendet, um mittels des neu entwickelten Schwellwertalgorithmus MeDeA das Einsetzen der sommerlichen Schmelzperiode für das gesamte antarktische Meereisgebiet zu bestimmen. Durch die Anwendung der neuen Methode auf die langjährigen Reihen der Satellitenmessungen konnte ein umfassender Datensatz erstellt werden, der für den Zeitraum von 1988 bis 2006 die räumliche und zeitliche Variabilität des Einsetzens der sommerlichen Schmelzperiode auf antarktischem Meereis beinhaltet. Die Ergebnisse zeigen, dass im Untersuchungszeitraum keine signifikanten Trends im Beginn des Schmelzens der Schneeauflage festzustellen sind, und dass das Schmelzen im Vergleich zur Arktis deutlich schwächer ausgeprägt ist. Eine Untersuchung der atmosphärischen Antriebe durch die Auswertung meteorologischer Reanalysen zeigt den grundlegenden Einfluss der zirkumpolaren Strömungsmuster auf die interannualen Schwankungen des Einsetzens und der Stärke der sommerlichen Schneeschmelze.
The presence of sea ice leads in the sea ice cover represents a key feature in polar regions by controlling the heat exchange between the relatively warm ocean and cold atmosphere due to increased fluxes of turbulent sensible and latent heat. Sea ice leads contribute to the sea ice production and are sources for the formation of dense water which affects the ocean circulation. Atmospheric and ocean models strongly rely on observational data to describe the respective state of the sea ice since numerical models are not able to produce sea ice leads explicitly. For the Arctic, some lead datasets are available, but for the Antarctic, no such data yet exist. Our study presents a new algorithm with which leads are automatically identified in satellite thermal infrared images. A variety of lead metrics is used to distinguish between true leads and detection artefacts with the use of fuzzy logic. We evaluate the outputs and provide pixel-wise uncertainties. Our data yield daily sea ice lead maps at a resolution of 1 km2 for the winter months November– April 2002/03–2018/19 (Arctic) and April–September 2003–2019 (Antarctic), respectively. The long-term average of the lead frequency distributions show distinct features related to bathymetric structures in both hemispheres.
In recent decades, the Arctic has been undergoing a wide range of fast environmental changes. The sea ice covering the Arctic Ocean not only reacts rapidly to these changes, but also influences and alters the physical properties of the atmospheric boundary layer and the underlying ocean on various scales. In that regard, polynyas, i.e. regions of open water and thin ice within thernclosed pack ice, play a key role as being regions of enhanced atmosphere-ice-ocean interactions and extensive new ice formation during winter. A precise long-term monitoring and increased efforts to employ long-term and high-resolution satellite data is therefore of high interest for the polar scientific community. The retrieval of thin-ice thickness (TIT) fields from thermal infrared satellite data and atmospheric reanalysis, utilizing a one-dimensional energy balance model, allows for the estimation of the heat loss to the atmosphere and hence, ice-production rates. However, an extended application of this approach is inherently connected with severe challenges that originate predominantly from the disturbing influence of clouds and necessary simplifications in the model set-up, which all need to be carefully considered and compensated for. The presented thesis addresses these challenges and demonstrates the applicability of thermal infrared TIT distributions for a long-term polynya monitoring, as well as an accurate estimation of ice production in Arctic polynyas at a relatively high spatial resolution. Being written in a cumulative style, the thesis is subdivided into three parts that show the consequent evolution and improvement of the TIT retrieval, based on two regional studies (Storfjorden and North Water (NOW) polynya) and a final large-scale, pan-Arctic study. The first study on the Storfjorden polynya, situated in the Svalbard archipelago, represents the first long-term investigation on spatial and temporal polynya characteristics that is solely based on daily TIT fields derived from MODIS thermal infrared satellite data and ECMWF ERA-Interim atmospheric reanalysis data. Typical quantities such as polynya area (POLA), the TIT distribution, frequencies of polynya events as well as the total ice production are derived and compared to previous remote sensing and modeling studies. The study includes a first basic approach that aims for a compensation of cloud-induced gaps in daily TIT composites. This coverage-correction (CC) is a mathematically simple upscaling procedure that depends solely on the daily percentage of available MODIS coverage and yields daily POLA with an error-margin of 5 to 6 %. The NOW polynya in northern Baffin Bay is the main focus region of the second study, which follows two main goals. First, a new statistics-based cloud interpolation scheme (Spatial Feature Reconstruction - SFR) as well as additional cloud-screening procedures are successfully adapted and implemented in the TIT retrieval for usage in Arctic polynya regions. For a 13-yr period, results on polynya characteristics are compared to the CC approach. Furthermore, an investigation on highly variable ice-bridge dynamics in Nares Strait is presented. Second, an analysis of decadal changes of the NOW polynya is carried out, as the additional use of a suite of passive microwave sensors leads to an extended record of 37 consecutive winter seasons, thereby enabling detailed inter-sensor comparisons. In the final study, the SFR-interpolated daily TIT composites are used to infer spatial and temporal characteristics of 17 circumpolar polynya regions in the Arctic for 2002/2003 to 2014/2015. All polynya regions combined cover an average thin-ice area of 226.6 -± 36.1 x 10-³ km-² during winter (November to March) and yield an average total wintertime accumulated ice production of about 1811 -± 293 km-³. Regional differences in derived ice production trends are noticeable. The Laptev Sea on the Siberian shelf is presented as a focus region, as frequently appearing polynyas along the fast-ice edge promote high rates of new ice production. New affirming results on a distinct relation to sea-ice area export rates and hence, the Transpolar Drift, are shown. This new high-resolution pan-Arctic data set can be further utilized and build upon in a variety of atmospheric and oceanographic applications, while still offering room for further improvements such as incorporating high-resolution atmospheric data sets and an optimized lead-detection.