Participants of the Open ARTS Community Workshop 2010

Group picture of the participants of the Open ARTS Community Workshop 2010 at the Kristineberg Marine Research Station.

Auditorium at the Open ARTS Community Workshop 2010

Auditorium at the Open ARTS Community Workshop 2010 at the Kristineberg Marine Research Station.

Artist's impression of CloudIce Satellite

An artist's impression of the CloudIce satellite, as proposed in the CloudIce Mission proposal for ESA Earth Explorer 8. (Image by Astrium SAS.)

SAT Group

Our group members April 2010. In front: Oliver Lemke, Thomas Kuhn, Salomon Eliasson, Isaac Moradi. In the back: Ajil Kottayil, Gerrit Holl, Johan Reponen, Stefan Buehler, Jana Mendrok, Mathias Milz.

Climatological mean of OLR and 850 hPa winds

June to September climatological mean of (a) OLR (W m−2) and 850 hPa winds (m s−1) and (b) daily OLR standard deviation. (c) The climatological mean of UTH (in %RH) and 500–200 hPa averaged winds (m s−1). The clima- tology is constructed using 11 years of data (1999–2009). (d) The standard deviation of daily UTH values. This is Figure 1 in xavier10:_variability_grl.

Distribution of CloudSat IWP

Distribution of CloudSat IWP between 60N and 60S on a 5° grid, based on data from July 2006 to August 2009. This is Figure 3 in seliassonxx:_assessing_acpd.

Comparison of integrated water vapor data over Kiruna

Comparison of integrated water vapor data over Kiruna from a number of different instruments. Overview of all time series used in the study. Instruments include a ground based GPS reciever, a ground based Fourier transform infrared spectrometer, a ground based microwave radiometer, a satellite based microwave radiometer and radiosondes. The comparison was the topic of the Master thesis by Simon Östman.

Sun dogs near Kiruna

During cold weather, a phenomenon known as diamond dust causes effects such as sun dogs. A faint halo is also visible.

Mean yearly UTH map from NOAA-17 AMSU-B data with the location of the ARM stations

Mean yearly UTH map from NOAA-17 AMSU-B data with the location of the ARM stations. This is figure 1 of moradixx:_comparing_arm_jgr, submitted 28 January 2010.

Collocations

Collocations between different satellite instruments can be used for various purposes. The figure shows the footprints of the CloudSat Cloud Profiling Radar, the Microwave Humidity Sounder on-board NOAA-18, and the High-Resolution Infrared Radiation Sounder on-board the same satellite. This is Figure 1 of hollxx:_collocating_amtd, submitted 29 January 2010.
Map data ©OpenStreetMap contributors, CC-BY-SA.

Polar Stratospheric Clouds

Polar Stratospheric Clouds over Kiruna, 2010-01-10.
Picture: Oliver Lemke

SAT Group

Our group members October 2008: Isaac Moradi, Mathias Milz, Stefan Bühler, Salomon Eliasson, Erik Johansson, Oliver Lemke, Gerrit Holl. Kiruna, 2008-10-29.

HIRS Channel Positions

Channel positions of the High Resolution Infrared Radiation Sounder (HIRS) on the satellite NOAA 14, relative to the atmospheric radiance spectrum. Gray bands indicate HIRS channel positions. For Channels 8-12 their shape indicates the shape of the channel response function (with arbitrary scaling). For Channels 1-7 only the center positions are shown, because these channels overlap significantly. Smooth black curves show Planck functions for different temperatures. The temperatures are 225 K, 250 K, 275 K, and 299.71 K, where the latter corresponds to the surface temperature. The blue curve shows the atmospheric spectrum for a tropical atmosphere, calculated on a frequency grid with 2.5 cm-1 resolution. This is Figure 1 of buehlerxx:_efficient_jqsrt. It was created by Ajil Kottayil.

Difference of the median binned UTH values for

AIRS - AMSU-B-16 vs AMSU-B-16 (left) and HSB - AMSU-B-16 vs AMSU-B-16 (right) for January 2003. The solid white line is the mean and the dashed white line the standard deviation of the differences for 1% RH bins. Darker shades indicate higher number of measurements. This is Figure 2 of an article in GRL.

Mashrab Kuvatov

Mashrab Kuvatov after his PhD defense.

Halo

Halo in the morning at the Space Campus in Kiruna, 2009-03-25.
Picture: Oliver Lemke

Having fun at -33°C

If you happen to be in a place below -30°C, get a cup of hot water and throw it up in the air! Follow this link to see more pictures
Picture: Oliver Lemke

Stellar Plate Snowflakes

Stellar Plates: These common snowflakes are thin, plate-like crystals with six broad arms that form a star-like shape. Their faces are often decorated with amazingly elaborate and symmetrical markings.
Picture: Ken Libbrecht (http://snowcrystals.com/)

The Sun is going to rise very soon.

Kiruna, 25 December 2008.
Picture: Isaac Moradi

Polar Stratospheric Clouds

Polar Stratospheric Clouds over Kiruna, 2008-12-19.
Picture: Martin Wieser

Median UTH from AMSU-B on NOAA-16

Median UTH from AMSU-B on NOAA 16. Upper tropospheric humidity (UTH) is an important parameter of the climate system. Our goal is to derive a UTH data set from operational satellite microwave data. More details can be found on the project page, or in the recent JGR paper.

Summer in the north

Torne river near Vittangi, July 2008.
Picture: Stefanie Buehler

Halo

Halo at the Space Campus in Kiruna, 2008-03-27.
Picture: Hans Weber

Aurora Borealis

Aurora Borealis over Kiruna, 2007-03-11.
Picture: Oliver Lemke

Merry Christmas

Merry Christmas! God jul!
Picture: Oliver Lemke

Polar Stratospheric Clouds

Polar Stratospheric Clouds over Kiruna, 2007-12-16.
Picture: Uwe Raffalski

Start of the skiing season!

Kiruna, 2007-11-10. Start of the skiing season!

Light phenomenon in Kiruna.

Light phenomenon in Kiruna, Sweden, 2007-11-08.
Picture: Uwe Raffalski
Retouching: Oliver Lemke

2D histogram Tb20-Tb18 versus Tb18

2D histogram of AMSU-B Channel 20 minus Channel 18 brightness temperature differences (Tb20-Tb18), versus Channel 18 brightness temperatures (Tb18). Clouds lead to negative Tb20-Tb18, and to very cold Tb18. This can be used to filter out clouds from AMSU-B humidity measurements. The figure is part of Figure 1 of an article in ACP.

AMSU-B Swath

This image shows a swath of the AMSU-B instrument which plays an important role in our research. You can find AMSU related articles in our publication list.

OLR versus surface temperature

Calculated OLR at 100 hPa as a function of surface temperature for the five different radiosonde classes. The solid line is a linear fit to the data from all five classes. The grey shaded area shows the one standard deviation variability of clear-sky CERES/TRMM data. For details see John et al. (2006).

Congratulations Dr. Kuvatov!

Mashrab after his PhD defence.