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Examples of in situ vertical concentration profiles of water vapor achieved with the SDLA spectrometer operated from stratospheric balloons at mid and high latitudes The high dynamical range
Lucilla Alfonsi
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Photo Credit Jouni Jussila
Figure 3 Group of Paleomagnetism in Crary s laboratories Mc Murdo Antarctica Cape Roberts Project October November 1997 The ANDRILL project is a new international project focused in
AURORA at JUPITER Photo Credit R Prangé NASA Space Telescope Science Institute
Airglow more precisely nightglow spectrometer diagram spectral range spectral response stability controller card picture at El Leoncito site
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Organization ODIN
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AURORA on Earth Photo Credit Jouni Jussila Finland
Examples of in situ vertical concentration profiles of methane yielded by the SDLA spectrometer in the troposphere and the lower stratosphere at mid and high latitudes The concentration
This image of Polar Mesospheric Clouds PMC from the Aeronomy of Ice in the Mesosphere Cloud Imaging and Particle Size AIM CIPS instrument on July 14 2009 in the northern polar region The
The AIM Aeronomy of Ice in the Mesosphere spacecraft returned
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Geomagnetic activity indices are numeric parameters designed to give global and synthetic information about the perturbations of the Earth s magnetic field in general or more specifically
How we do it Airglow more precisely nightglow spectrometer diagram spectral range spectral response
Daily erythemal UV doses
h ganymede auroras 0 > 14 Feb 2009 00 17 2 8K janc 035 s gif 10 May 2007 16 58 15K m0125c gif 10 May 2007 16 58 4 0K mail archives html 20 Feb 2009 23 03 12K
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Figure 1 The electron density profile model used in AIP
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have been downlinked by NASA Up to now PROMISS is running nominally in a very stable temperature environment Our ULB colleagues have processed the housekeeping data of the MSG and in this graph you can find the temperature profile since the activation of PROMISS into MSG February 4 2004 Following the desiderata of belgian scientists a new table upload took
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Cassini Interdisciplinary Investigation Aeronomy Magnetosphere Solar Wind Interaction IDS
Abstract with link to full article through ScienceDirect Reprinted from Icarus vol 154 pp 350 371 copyright 2001 with permission from Elsevier No further distribution is allowed Next page Return to
Artist Rendition of Aeronomy of Ice in the Mesosphere AIM
Figure 4 Phases of smear slide preparation The last picture shows an assemblage viewed by a polarized light microscope crossed nicols at 1250x magnification Patrizia Pantani INGV of Pisa is
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Click to enlarge the image Red sprites
Reprinted from Icarus vol 154 pp 350 371 copyright 2001 with permission from Elsevier No further distribution is allowed Next page Return to
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