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Shipboard Automated Meteorological and Oceanographic System (SAMOS) air-sea fluxes, version 2, 2005-2015

Along ship track bulk turbulent heat and momentum fluxes derived using one-minute interval data collected by the Shipboard Automated Meteorological and Oceanographic System (SAMOS) initiative. The fluxes are provided as three products derived using three widely accepted air-sea flux algorithms (Smith 1988, COARE 3.5, and a 2013 update of Bourassa 2006). Datasets are organized by ship and flux algorithm. The dataset uses SAMOS data from 19 research vessels with observations spanning 2005-2015. Data include heat and momentum fluxes, state variables adjusted to 10 meters, and multiple inputs and outputs from the flux algorithms. These data have wide use for satellite product and model evaluation; air-sea interaction, marine biology, chemistry and geoscience research activities; climate science, and marine geoinformatics. The data are concentrated in the oceans around North America, but select data are available from most ocean basins. Fluxes are derived from along cruise track navigational, meteorological, and oceanographic observations from 19 research vessels. Fluxes are derived at one-minute intervals (the same as the source observations) and take advantage of extensive quality control flags on the source SAMOS data. Additional QC flags are applied to the derived fluxes, height adjusted state variables, and other outputs of the flux algorithms. All data are provided in CF and ACDD compliant netCDF files, with extensive metadata. The uncompressed data volume is ca. 5 GB.

Shipboard Automated Meteorological and Oceanographic System (SAMOS) air-sea fluxes, version 3, 2005-2024

Along ship track bulk turbulent heat and momentum fluxes derived using one-minute interval data collected by the Shipboard Automated Meteorological and Oceanographic System (SAMOS) initiative. The fluxes are provided as three products derived using three widely accepted air-sea flux algorithms (Smith 1988, COARE 3.6, and a 2023 update of Bourassa 2006). Datasets are organized by ship and flux algorithm. The dataset uses SAMOS data from 47 research vessels with observations spanning 2005-2024. Data include heat and momentum fluxes, state variables adjusted to 10 meters, and multiple inputs and outputs from the flux algorithms. These data have wide use for satellite product and model evaluation; air-sea interaction, marine biology, chemistry and geoscience research activities; climate science, and marine geoinformatics. Data coverage is the global oceans, but is concentrated around North America. Fluxes are derived from along cruise track navigational, meteorological, and oceanographic observations from 47 research vessels. Fluxes are derived at one-minute intervals (the same as the source observations) and take advantage of extensive quality control flags on the source SAMOS data. Additional QC flags are applied to the derived fluxes, height adjusted state variables, and other outputs of the flux algorithms. All data are provided in CF and ACDD compliant netCDF files, with extensive metadata. The uncompressed data volume is ca. 180 GB per algorithm.

METOP GOME-2 - Water Vapour (H2O) - Global

Gidded Level 3 H2O total columns. The Earth's capacity to sustain life is attributed to two mechanisms: the greenhouse effect and the hydrological cycle. Water vapour in the atmosphere is a critical component of both processes and the main naturally occurring greenhouse gas in the Earth's climate system. Water in gaseous form varies more than other greenhouse gases. Monitoring atmospheric water vapour globally is essential to understand its climate impacts. Measurements of water vapor columns are derived from satellite observations of solar radiation in the ultraviolet and visible (430 – 450 nm) spectral ranges. A water vapour absorption band is detectable across some European Sentinel platforms (Sentinel-4, Sentinel-5P and 5), former (GOME and SCIAMACHY) and future instruments (CO2M). This absorption signature by water vapor is used to derive the shown concentrations with the Differential Optical Absorption Spectroscopy (DOAS) technique. The retrieval methodology, as applied to the fleet of available platforms, demonstrates several advantages, including optimal sensitivity and coverage characteristics across both oceans and continents, enhanced temporal sampling frequency for weather applications, and continuous extension of long-term datasets for climate study purposes. This is accomplished by DLR in the framework of the EUMETSAT's Satellite Application Facility on Atmospheric Composition (AC-SAF) monitoring where DLR generates operational GOME-2 / MetOp products.

Northern Eurasia Earth Science Partnership Initiative (NEESPI)

The Northern Eurasia Earth Science Partnership Initiative, or NEESPI, is a currently active, yet strategically evolving program of internationally-supported Earth systems science research, which has as its foci issues in northern Eurasia that are relevant to regional and Global scientific and decision-making communities (see NEESPI Mission Statement). This part of the globe is undergoing significant changes - particularly those changes associated with a rapidly warming climate in this region and with important changes in governmental structures since the early 1990s and their associated influences on land use and the environment across this broad expanse. How this carbon-rich, cold region component of the Earth system functions as a regional entity and interacts with and feeds back to the greater Global system is to a large extent unknown. Thus, the capability to predict future changes that may be expected to occur within this region and the consequences of those changes with any acceptable accuracy is currently uncertain. One of the reasons for this lack of regional Earth system understanding is the relative paucity of well-coordinated, multidisciplinary and integrating studies of the critical physical and biological systems. By establishing a large-scale, multidisciplinary program of funded research, NEESPI is aimed at developing an enhanced understanding of the interactions between the ecosystem, atmosphere, and human dynamics in northern Eurasia. Specifically, the NEESPI strives to understand how the land ecosystems and continental water dynamics in northern Eurasia interact with and alter the climatic system, biosphere, atmosphere, and hydrosphere of the Earth. The contemporaneous changes in climate and land use are impacting the biological, chemical, and physical functions of the northern Eurasia, but little data and fewer models are available that can be used to understand the current status of this expansive regional system, much less the influence of the northern Eurasia region on the Global climate. NEESPI seeks to secure the necessary financial and related institutional support from an international cadre of sponsors for developing a viable understanding of the functioning of northern Eurasia and the impacts of extant changes on the regional and Earth systems. Many types of ground and integrative (e.g., satellite; GIS) data will be needed and many models must be applied, adapted or developed for properly understanding the functioning of this cold and diverse regional system. Mechanisms for obtaining the requisite data sets and models and sharing them among the participating scientists are essential and require international and active governmental participation. (abridged text)

Schwerpunktprogramm (SPP) 1488: Planetary Magnetism (PlanetMag), Evolution of geomagnetic dipole moment and South Atlantic Anomaly

The geomagnetic field shields our habitat against solar wind and radiation from space. Due to the geometry of the field, the shielding in general is weakest at high latitudes. It is also anomalously weak in a region around the south Atlantic known as South Atlantic Anomaly (SAA), and the global dipole moment has been decreasing by nearly 10 percent since direct measurements of field intensity became possible in 1832. Due to our limited understanding of the geodynamo processes in Earths core, it is impossible to reliably predict the future evolution of both dipole moment and SAA over the coming decades. However, lack of magnetic field shielding as would be a consequence of further weakening of dipole moment and SAA region field intensity would cause increasing problems for modern technology, in particular satellites, which are vulnerable to radiation damage. A better understanding of the underlying processes is required to estimate the future development of magnetic field characteristics. The study of the past evolution of such characteristics based on historical, archeo- and paleomagnetic data, on time-scales of centuries to millennia, is essential to detect any recurrences and periodicities and provide new insights in dynamo processes in comparison to or in combination with numerical dynamo simulations. We propose to develop two new global spherical harmonic geomagnetic field models, spanning 1 and 10 kyrs, respectively, and designed in particular to study how long the uninterrupted decay of the dipole moment has been going on prior to 1832, and if the SAA is a recurring structure of the field.We will combine for the first time all available historical and archeomagnetic data, both directions and intensities, in a spherical harmonic model spanning the past 1000 years. Existing modelling methods will be adapted accordingly, and existing data bases will be complemented with newly published data. We will further acquire some new archeomagnetic data from the Cape Verde islands from historical times to better constrain the early evolution of the present-day SAA. In order to study the long-term field evolution and possible recurrences of similar weak field structures in this region, we will produce new paleomagnetic records from available marine sediment cores off the coasts of West Africa, Brazil and Chile. This region is weakly constrained in previous millennial scale models. Apart from our main aim to gain better insights into the previous evolution of dipole moment and SAA, the models will be used to study relations between dipole and non-dipole field contributions, hemispheric symmetries and large-scale flux patterns at the core-mantle boundary. These observational findings will provide new insights into geodynamo processes when compared with numerical dynamo simulation results.Moreover, the models can be used to estimate past geomagnetic shielding above Earths surface against solar wind and for nuclide production from galactic cosmic rays.

Schwerpunktprogramm (SPP) 1294: Bereich Infrastruktur - Atmospheric and Earth system research with the 'High Altitude and Long Range Research Aircraft' (HALO), Langwelliger Strahlungsantrieb durch Aerosol-Wolken-Wechselwirkungen: Satelliten und Klimamodelle im Vergleich zu HALO

Der Strahlungsantrieb durch anthropogene Aerosole aufgrund von Aerosol-Wolken-Wechselwirkungen ist die Hauptunsicherheit bezüglich des Antriebs des Klimawandels. Für Flüssigwasserwolken, die den Strahlungsantrieb im solaren (kurzwelligen) Spektrum dominieren, konnten mittlerweile einige Fortschritte in der Quantifizierung erzielt werden. Im Gegensatz dazu gibt es für den Strahlungsantrieb im langwelligen (terrestrischen) Spektralbereich nur sehr grobe Abschätzungen von Klimamodellen. In Vorarbeiten haben wir einen Vorschlag entwickelt, wir aktive Fernerkundung zur Charakterisierung von Eiskristallkonzentrationen und Aerosol benutzt werden könnte, um eine beobachtungsbasierte Abschätzung des Strahlungsantriebs durch Aerosol-Wolken-Wechselwirkungen im langwelligen Spektrum zu ermöglichen. Allerdings sind die Satellitendaten höchst unsicher und benötigen eine Validierung mit Referenzdaten. In FLASH wird vorgeschlagen, (i) die Satelliten-abgeleitete Eiskristallkonzentration sowie ihre Sensitivität bezüglich Temperatur, Vertikalwind und Aerosolbedingungen mit den neuen In-situ-Daten von HALO zu validieren bzw. evaluieren, (ii) die Ableitung der Eiskristallkonzentration vom Satelliten mit der von Lidar und Radar an Bord von HALO zu verifizieren, (iii) Klimamodelle zu evaluieren und zur Interpretation der statistischen Relationen zu benutzen, und (iv) schließlich eine Abschätzung des Strahlungsantriebs durch Aerosol-Wolken-Wechselwirkungen und seines Unsicherheitsbereichs zu erarbeiten. Die Rolle von FLASH im SPP 1294 ist es, die vorhandenen Daten auszuwerten und mit den Daten geplanter Kampagnen in integrierender Weise zu arbeiten mit dem Ziel, eine bessere Abschätzung des Aerosol-Wolken-Strahlungsantriebs zu erreichen, neue innovative Satellitendaten zu validieren, und die relevanten Parametrisierungen in Klimamodellen zu evaluieren und zu verbessern.

METOP GOME-2 - Cloud Fraction (CF) - Global

Gridded Level 3 cloud fraction derived from Metop/GOME observations. Cloud physical properties (cloud fraction, cloud top height, cloud optical thickness) are derived from GOME/GOME-2 observations using the OCRA (Optical Cloud Recognition Algorithm) and ROCINN (Retrieval of Cloud Information using Neural Networks). For more details please refer to relevant peer-review papers listed on the GOME and GOME-2 documentation pages: https://atmos.eoc.dlr.de/app/docs/ The Global Ozone Monitoring Experiment-2 (GOME-2) instrument continues the long-term monitoring of atmospheric trace gas constituents started with GOME / ERS-2 and SCIAMACHY / Envisat. Three instruments operate on board EUMETSAT's Meteorological Operational satellites MetOp-A, -B, and -C, launched in 2006, 2012, and 2018, respectively. GOME-2 measures a range of atmospheric trace constituents, with the emphasis on global ozone distribution. Furthermore, cloud properties and intensities of ultraviolet radiation are retrieved. These data are crucial for monitoring the atmospheric composition and the detection of pollutants. DLR generates operational GOME-2 / MetOp products in the framework of EUMETSAT's Satellite Application Facility on Atmospheric Composition Monitoring (AC-SAF).

GTS Bulletin: IUTJ14 EDZW - Observational data (Binary coded) - BUFR (details are described in the abstract)

The IUTJ14 TTAAii Data Designators decode as: T1 (I): Observational data (Binary coded) - BUFR T1T2 (IU): Upper air T1T2A1 (IUT): (used for satellite-derived sondes – see Note 3) A2 (J): 90°W - 180° southern hemisphere (Remarks from Volume-C: (CBS)SATELLITE RADIO OCCULTATION DATA)

Modelling of soil moisture in high spatial resolution for farmed grasslands in China based on airborne thermal data

In Inner Mongolia the heterogeneity of rainfall patterns, differences in grazing intensity and topography lead to strong temporal and spatial variability of soil moisture which has great effects on vegetation growth and influences CO2 and water fluxes. The spatial and temporal distribution and variability of near surface soil moisture will be modelled with a new approach using the atmospheric boundary layer model HIRVAC and thermal imagery obtained during the 2009 field campaign within the MAGIM research group. Thermal imagery was collected using a microlite aircraft which emerged as an adequate platform particularly for remote areas. The resulting soil moisture grids will allow for the analysis of spatial soil moisture variability at field and local scale. The high geometrical resolution (1 m) closes the gap between point surface and satellite measurements.

Süßwasserflüsse über dem Ozean I - Verdunstungsflüsse (FreshOcean)

Die Veränderung des globalen Wasserkreislaufs durch den Klimawandel ist eine der größten Herausforderungen für die Gesellschaft, da trockene Regionen trockener und feuchte Regionen feuchter werden. Das Problem besteht darin, dass 85 % der Verdunstung und 77 % der Niederschläge über den Ozeanen stattfinden und der globale Wasserkreislauf aufgrund der schwierigen Beobachtungsbedingungen über den Ozeanen nur unzureichend verstanden wird. Der Austausch von Süßwasser zwischen dem Ozean und der Atmosphäre findet jedoch in einer obersten dünnen Schicht der Meeresoberfläche statt, den so genannten Oberflächenfilm. Die Verdunstung von Wasserdampf aus den Oberflächenfilmen erhöht deren Salzgehalt, während der Niederschlag den Salzgehalt in den Oberflächenfilmen verringert. Das Hauptziel dieses Forschungsprojekts ist ein umfassendes Verständnis der Dynamik und der Veränderungen des Salzgehalts und der damit zusammenhängenden thermischen Felder in den ozeanischen Oberflächenfilmen und der oberflächennahen Schicht (NSL) sowie deren Zusammenhang mit den verdunstenden Süßwasserflüssen zu erzielen. Einer der Hauptpunkte dieser Arbeit ist, dass Süsswasserflüsse (Verdunstung minus Niederschlag) direkt auf die Meeresoberfläche einwirkt und daher vorwiegend den Salzgehalt der Oberflächenfilme quasi-instant beeinflusst, während die derzeitigen Methoden, die den Salzgehalt der gemischten Schicht verwenden, sich auf dekadischen Skalen beziehen. Eine umfassende Reihe von Experimenten wird in einer großmaßstäblichen Mesokosmenanlage an der Universität Oldenburg durchgeführt, in der die treibenden Kräfte für die Verdunstung kontrolliert werden können (Wassertemperatur, Windgeschwindigkeit, turbulente Vermischung, Lufttemperatur und -feuchtigkeit). Im Mittelpunkt steht eine Expedition in den Mittelatlantik mit seinem hohen Oberflächensalzgehalt, d. h. Verdunstungsraten übersteigen die Niederschlagsraten. Während der Expedition kommt ein funkgesteuertes Katamaran zum Einsatz, der in der Lage ist, Oberflächenfilme zu sammeln. Die Beobachtungen werden durch Messungen von Bojen, schiffsbasierten Messungen und Satelliten unterstützt. Die Arbeiten ergänzen die laufenden Aktivitäten zur Untersuchung des Zusammenhangs zwischen dem Salzgehalt der Oberflächenfilme und den Niederschlägen. Diese Arbeit ist ein erster Schritt, um zu verstehen, wie der Salzgehalt der Oberflächenfilme und der oberflächennahe Salzgehalt verwendet werden können, um dynamische Süsswasserflüsse zu integrieren und Parametrisierungen zur Extrapolation von Süsswasserflüssen unter Verwendung von satellitengestützten Salzgehaltsdaten zu entwickeln.

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